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3 October 2020

Julian Andres Klode: Google Pixel 4a: Initial Impressions

Yesterday I got a fresh new Pixel 4a, to replace my dying OnePlus 6. The OnePlus had developed some faults over time: It repeatedly loses connection to the AP and the network, and it got a bunch of scratches and scuffs from falling on various surfaces without any protection over the past year.

Why get a Pixel? Camera: OnePlus focuses on stuffing as many sensors as it can into a phone, rather than a good main sensor, resulting in pictures that are mediocre blurry messes - the dreaded oil painting effect. Pixel have some of the best camera in the smartphone world. Sure, other hardware is far more capable, but the Pixels manage consistent results, so you need to take less pictures because they don t come out blurry half the time, and the post processing is so good that the pictures you get are just great. Other phones can shoot better pictures, sure - on a tripod. Security updates: Pixels provide 3 years of monthly updates, with security updates being published on the 5th of each month. OnePlus only provides updates every 2 months, and then the updates they do release are almost a month out of date, not counting that they are only 1st-of-month patches, meaning vendor blob updates included in the 5th-of-month updates are even a month older. Given that all my banking runs on the phone, I don t want it to be constantly behind. Feature updates: Of course, Pixels also get Beta Android releases and the newest Android release faster than any other phone, which is advantageous for Android development and being nerdy. Size and weight: OnePlus phones keep getting bigger and bigger. By today s standards, the OnePlus 6 at 6.18" and 177g is a small an lightweight device. Their latest phone, the Nord, has 6.44" and weighs 184g, the OnePlus 8 comes in at 180g with a 6.55" display. This is becoming unwieldy. Eschewing glass and aluminium for plastic, the Pixel 4a comes in at 144g.

First impressions

Accessories The Pixel 4a comes in a small box with a charger, USB-C to USB-C cable, a USB-OTG adapter, sim tray ejector. No pre-installed screen protector or bumper are provided, as we ve grown accustomed to from Chinese manufacturers like OnePlus or Xiaomi. The sim tray ejector has a circular end instead of the standard oval one - I assume so it looks like the o in Google? Google sells you fabric cases for 45 . That seems a bit excessive, although I like that a lot of it is recycled.

Haptics Coming from a 6.18" phablet, the Pixel 4a with its 5.81" feels tiny. In fact, it s so tiny my thumb and my index finger can touch while holding it. Cute! Bezels are a bit bigger, resulting in slightly less screen to body. The bottom chin is probably impracticably small, this was already a problem on the OnePlus 6, but this one is even smaller. Oh well, form over function. The buttons on the side are very loud and clicky. As is the vibration motor. I wonder if this Pixel thinks it s a Model M. It just feels great. The plastic back feels really good, it s that sort of high quality smooth plastic you used to see on those high-end Nokia devices. The finger print reader, is super fast. Setup just takes a few seconds per finger, and it works reliably. Other phones (OnePlus 6, Mi A1/A2) take like half a minute or a minute to set up.

Software The software - stock Android 11 - is fairly similar to OnePlus' OxygenOS. It s a clean experience, without a ton of added bloatware (even OnePlus now ships Facebook out of box, eww). It s cleaner than OxygenOS in some way - there are no duplicate photos apps, for example. On the other hand, it also has quite a bunch of Google stuff I could not care less about like YT Music. To be fair, those are minor noise once all 130 apps were transferred from the old phone. There are various things I miss coming from OnePlus such as off-screen gestures, network transfer rate indicator in quick settings, or a circular battery icon. But the Pixel has an always on display, which is kind of nice. Most of the cool Pixel features, like call screening or live transcriptions are unfortunately not available in Germany. The display is set to display the same amount of content as my 6.18" OnePlus 6 did, so everything is a bit tinier. This usually takes me a week or two to adjust too, and then when I look at the OnePlus again I ll be like Oh the font is huge , but right now, it feels a bit small on the Pixel. You can configure three colour profiles for the Pixel 4a: Natural, Boosted, and Adaptive. I have mine set to adaptive. I d love to see stock Android learn what OnePlus has here: the ability to adjust the colour temperature manually, as I prefer to keep my devices closer to 5500K than 6500K, as I feel it s a bit easier on the eyes. Or well, just give me the ability to load a ICM profile (though, I d need to calibrate the screen then - work!).

Migration experience Restoring the apps from my old phone only restore settings for a few handful out of 130, which is disappointing. I had to spent an hour or two logging in to all the other apps, and I had to fiddle far too long with openScale to get it to take its data over. It s a mystery to me why people do not allow their apps to be backed up, especially something innocent like a weight tracking app. One of my banking apps restored its logins, which I did not really like. KeePass2Android settings were restored as well, but at least the key file was not restored. I did not opt in to restoring my device settings, as I feel that restoring device settings when changing manufactures is bound to mess up some things. For example, I remember people migrating to OnePlus phones and getting their old DND schedule without any way to change it, because OnePlus had hidden the DND stuff. I assume that s the reason some accounts, like my work GSuite account were not migrated (it said it would migrate accounts during setup). I ve setup Bitwarden as my auto-fill service, so I could login into most of my apps and websites using the stored credentials. I found that often that did not work. Like Chrome does autofill fine once, but if I then want to autofill again, I have to kill and restart it, otherwise I don t get the auto-fill menu. Other apps did not allow any auto-fill at all, and only gave me the option to copy and paste. Yikes - auto-fill on Android still needs a lot of work.

Performance It hangs a bit sometimes, but this was likely due to me having set 2 million iterations on my Bitwarden KDF and using Bitwarden a lot, and then opening up all 130 apps to log into them which overwhelmed the phone a bit. Apart from that, it does not feel worse than the OnePlus 6 which was to be expected, given that the benchmarks only show a slight loss in performance. Photos do take a few seconds to process after taking them, which is annoying, but understandable given how much Google relies on computation to provide decent pictures.

Audio The Pixel has dual speakers, with the earpiece delivering a tiny sound and the bottom firing speaker doing most of the work. Still, it s better than just having the bottom firing speaker, as it does provide a more immersive experience. Bass makes this thing vibrate a lot. It does not feel like a resonance sort of thing, but you can feel the bass in your hands. I ve never had this before, and it will take some time getting used to.

Final thoughts This is a boring phone. There s no wow factor at all. It s neither huge, nor does it have high-res 48 or 64 MP cameras, nor does it have a ton of sensors. But everything it does, it does well. It does not pretend to be a flagship like its competition, it doesn t want to wow you, it just wants to be the perfect phone for you. The build is solid, the buttons make you think of a Model M, the camera is one of the best in any smartphone, and you of course get the latest updates before anyone else. It does not feel like a only 350 phone, but yet it is. 128GB storage is plenty, 1080p resolution is plenty, 12.2MP is you guessed it, plenty. The same applies to the other two Pixel phones - the 4a 5G and 5. Neither are particularly exciting phones, and I personally find it hard to justify spending 620 on the Pixel 5 when the Pixel 4a does job for me, but the 4a 5G might appeal to users looking for larger phones. As to 5G, I wouldn t get much use out of it, seeing as its not available anywhere I am. Because I m on Vodafone. If you have a Telekom contract or live outside of Germany, you might just have good 5G coverage already and it might make sense to get a 5G phone rather than sticking to the budget choice.

Outlook The big question for me is whether I ll be able to adjust to the smaller display. I now have a tablet, so I m less often using the phone (which my hands thank me for), which means that a smaller phone is probably a good call. Oh while we re talking about calls - I only have a data-only SIM in it, so I could not test calling. I m transferring to a new phone contract this month, and I ll give it a go then. This will be the first time I get VoLTE and WiFi calling, although it is Vodafone, so quality might just be worse than Telekom on 2G, who knows. A big shoutout to congstar for letting me cancel with a simple button click, and to @vodafoneservice on twitter for quickly setting up my benefits of additional 5GB per month and 10 discount for being an existing cable customer. I m also looking forward to playing around with the camera (especially night sight), and eSIM. And I m getting a case from China, which was handed over to the Airline on Sep 17 according to Aliexpress, so I guess it should arrive in the next weeks. Oh, and screen protector is not here yet, so I can t really judge the screen quality much, as I still have the factory protection film on it, and that s just a blurry mess - but good enough for setting it up. Please Google, pre-apply a screen protector on future phones and include a simple bumper case. I might report back in two weeks when I have spent some more time with the device.

Ritesh Raj Sarraf: First Telescope

Curiosity I guess this would be common to most of us. While I grew up, right from the childhood itself, the sky was always an intriguing view. The Stars, the Moon, the Eclipses; were all fascinating. As a child, in my region, religion and culture; the mythology also built up stories around it. Lunar Eclipses have a story of its own. During Solar Eclipses, parents still insist that we do not go out. And to be done with the food eating before/after the eclipse. Then there s the Hindu Astrology part, which claims its own theories and drags in mythology along. For example, you ll still find the Hindu Astrology making recommendations to follow certain practices with the planets, to get auspicious personal results. As far as I know, other religions too have similar beliefs about the planets. As a child, we are told the Moon to be addressed as an Uncle ( ). There s also a rhyme around it, that many of us must have heard. And if you look at our god, Lord Mahadev, he s got a crescent on his head
Lord Mahadev
Lord Mahadev

Reality Fast-forward to today, as I grew, so did some of my understanding. It is fascinating how mankind has achieved so much understanding of our surrounding. You could go through the documentaries on Mars Exploration, for example; to see how the rovers are providing invaluable data. As a mere individual, there s a limit to what one can achieve. But the questions flow in free.
  • Is there life beyond us
  • What s out there in the sky
  • Why is all this the way it is

Hobby The very first step, for me, for every such curiosity, has been to do the ground work, with the resources I have. To study on the subject. I have done this all my life. For example, I started into the Software domain as: A curiosity => A Hobby => A profession Same was the case with some of the other hobbies, equally difficult as Astronomy, that I developed a liking for. Just did the ground work, studied on those topics and then applied the knowledge to further improve it and build up some experience. And star gazing came in no different. As a complete noob, had to start with the A B C on the subject of Astronomy. Familiarize myself with the usual terms. As so on PS: Do keep in mind that not all hobbies have a successful end. For example, I always craved to be good with graphic designing, image processing and the likes, where I ve always failed. Never was able to keep myself motivated enough. Similar was my experience when trying to learn playing a musical instrument. Just didn t work out for me, then. There s also a phase in it, where you fail and then learn from the failures and proceed further, and then eventually succeed. But we all like to talk about the successes. :-)

Astronomy So far, my impression has been that this topic/domain will not suit most of the people. While the initial attraction may be strong, given the complexity and perseverance that Astronomy requires, most people would lose interest in it very soon. Then there s the realization factor. If one goes with an expectation to get quick results, they may get disappointed. It isn t like a point and shoot device that d give you results on the spot. There s also the expectation side of things. If you are a person more accustomed to taking pretty selfies, which always come right because the phone manufacturer does heavy processing on the images to ensure that you get to see the pretty fake self, for the most of the times; then star gazing with telescopes could be a frustrating experience altogether. What you get to see in the images on the internet will be very different than what you d be able to see with your eyes and your basic telescope. There s also the cost aspect. The more powerful (and expensive) your telescope, the better your view. And all things aside, it still may get you lose interest, after you ve done all the ground work and spent a good chunk of money on it. Simply because the object you are gazing at is more a still image, which can quickly get boring for many. On the other hand, if none of the things obstruct, then the domain of Astronomy can be quite fascinating. It is a continuous learning domain (reminds me of CI in our software field these days). It is just the beginning for us here, and we hope to have a lasting experience in it.

The Internet I have been indebted to the internet right from the beginning. The internet is what helped me be able to achieve all I wanted. It is one field with no boundaries. If there is a will, there is a way; and often times, the internet is the way.
  • I learnt computers over the internet.
  • Learnt more about gardening and plants over the internet
  • Learnt more about fish care-taking over the internet
And many many more things. Some of the communities over the internet are a great way to participation. They bridge the age gap, the regional gap and many more. For my Astronomy need, I was glad to see so many active communities, with great participants, on the internet.

Telescope While there are multiple options to start star gazing, I chose to start with a telescope. But as someone completely new to this domain, there was a long way to go. And to add to that, the real life: work + family I spent a good 12+ months reading up on the different types of telescopes, what they are, their differences, their costs, their practical availability etc. The good thing is that the market has offerings for everything. From a very basic binocular to a fully automatic Maksutov-Cassegrain scope. It all would depend on your budget.

Automatic vs Manual To make it easy for the users, the market has multiple options in the offering. One could opt-in for a cheap, basic and manually operated telescope; which would require the user to do a lot of ground study. On the other hand, users also have the option of automatic telescopes which do the hard work of locating and tracking the planetary objects. Either option aside, the end result of how much you ll be able to observe the sky, still depends on many many more factors: Enthusiasm over time, Light Pollution, Clear Skies, Timing etc. PS: The planetary objects move at a steady pace. Objects you lock into your view now will be gone out of the FOV in just a matter of minutes.

My Telescope After spending so much of the time reading up on types of telescopes, my conclusion was that a scope with high aperture and focal length was the way to go forward. This made me shorten the list to Dobsonians. But the Dobsonians aren t a very cheap telescope, whether manual or automatic. My final decision made me acquire a 6" Dobsonian Telescope. It is a Newtonian Reflecting Telescope with a 1200mm focal length and 150mm diameter. Another thing about this subject is that most of the stuff you do in Astronomy; right from the telescope selection, to installation, to star gazing; most of it is DIY, so your mileage may vary with the end result and experience. For me, installation wasn t very difficult. I was able to assemble the base Dobsonian mount and the scope in around 2 hours. But the installation manual, I had been provided with, was very brief. I ended up with one module in the mount wrongly fit, which I was able to fix later, with the help of online forums.
Dobsonian Mount
Dobsonian Mount
In this image you can see that the side facing out, where the handle will go, is wrong. If fit this way, the handle will not withstand any weight at all.
Correct Panel Side
Correct Panel Side
The right fix of the handle base board. In this image, the handle is on the other side that I m holding. Because the initial fit put in some damage to the engineered wood, I fixed it up by sealing with some adhesive. With that, this is what my final telescope looks like.
Final Telescope
Final Telescope

Clear Skies While the telescope was ready, the skies were not. For almost next 10 days, we had no clear skies at all. All I could do was wait. Wait so much that I had forgotten to check on the skies. Luckily, my wife noticed clear skies this week for a single day. Clear enough that we could try out our telescope for the very first time.
Me posing for a shot
Me posing for a shot

Telescope As I said earlier, in my opinion, it takes a lot of patience and perseverance on this subject. And most of the things here are DIY. To start with, we targeted the Moon. Because it is easy. I pointed the scope to the moon, then looked into the finder scope to center it, and then looked through the eyepiece. And blank. Nothing out there. Turns out, the finder scope and the viewer s angle weren t aligned. This is common and the first DIY step, when you plan to use your telescope for viewing. Since our first attempt was unplanned and just random because we luckily spotted that the skies were clear, we weren t prepared for this. Lucky enough, mapping the difference in the alignment, in the head, is not very difficult. After a couple of minutes, I could make out the point in the finder scope, where the object if projected, would show proper in the viewer. With that done, it was just mesmerizing to see the Moon, in a bit more detail, than what I ve seen all these years of my life.
Moon
Moon
Moon
Moon
Moon
Moon
Moon
Moon
The images are not exactly what we saw with our eyes. The view was much more vivid than these pictures. But as a first timer, I really wanted to capture this first moment of a closer view of the Moon. In the whole process; that of ground work studying about telescopes, installation of the telescope, astronomy basics and many other things; the most difficult part in this entire journey, was to point my phone to the viewing eyepiece, to get a shot of the object. This requirement just introduced me to astrophotography. And then, Dobsonians aren t the best model for astrophotography, to what I ve learnt so far. Hopefully, I ll find my ways to do some DIY astrophotography with the tools I have. Or extend my arsenal over time. But overall, we ve been very pleased with the subject of Astronomy. It is a different feel altogether and we re glad to have forayed into it.

2 October 2020

Ian Jackson: Mailman vs DKIM - a novel solution

tl;dr: Do not configure Mailman to replace the mail domains in From: headers. Instead, try out my small new program which can make your Mailman transparent, so that DKIM signatures survive. Background and narrative DKIM NB: This explanation is going to be somewhat simplified. I am going to gloss over some details and make some slightly approximate statements. DKIM is a new anti-spoofing mechanism for Internet email, intended to help fight spam. DKIM, paired with the DMARC policy system, has been remarkably successful at stemming the flood of joe-job spams. As usually deployed, DKIM works like this: When a message is originally sent, the author's MUA sends it to the MTA for their From: domain for outward delivery. The From: domain mailserver calculates a cryptographic signature of the message, and puts the signature in the headers of the message. Obviously not the whole message can be signed, since at the very least additional headers need to be added in transit, and sometimes headers need to be modified too. The signing MTA gets to decide what parts of the message are covered by the signature: they nominate the header fields that are covered by the signature, and specify how to handle the body. A recipient MTA looks up the public key for the From: domain in the DNS, and checks the signature. If the signature doesn't match, depending on policy (originator's policy, in the DNS, and recipient's policy of course), typically the message will be treated as spam. The originating site has a lot of control over what happens in practice. They get to publish a formal (DMARC) policy in the DNS which advises recipients what they should do with mails claiming to be from their site. As mentioned, they can say which headers are covered by the signature - including the ability to sign the absence of a particular headers - so they can control which headers downstreams can get away with adding or modifying. And they can set a normalisation policy, which controls how precisely the message must match the one that they sent. Mailman Mailman is, of course, the extremely popular mailing list manager. There are a lot of things to like about it. I choose to run it myself not just because it's popular but also because it provides a relatively competent web UI and a relatively competent email (un)subscription interfaces, decent bounce handling, and a pretty good set of moderation and posting access controls. The Xen Project mailing lists also run on mailman. Recently we had some difficulties with messages sent by Citrix staff (including myself), to Xen mailing lists, being treated as spam. Recipient mail systems were saying the DKIM signatures were invalid. This was in fact true. Citrix has chosen a fairly strict DKIM policy; in particular, they have chosen "simple" normalisation - meaning that signed message headers must precisely match in syntax as well as in a semantic sense. Examining the the failing-DKIM messages showed that this was definitely a factor. Applying my Opinions about email My Bayesian priors tend to suggest that a mail problem involving corporate email is the fault of the corporate email. However in this case that doesn't seem true to me. My starting point is that I think mail systems should not not modify messages unnecessarily. None of the DKIM-breaking modifications made by Mailman seemed necessary to me. I have on previous occasions gone to corporate IT and requested quite firmly that things I felt were broken should be changed. But it seemed wrong to go to corporate IT and ask them to change their published DKIM/DMARC policy to accomodate a behaviour in Mailman which I didn't agree with myself. I felt that instead I shoud put (with my Xen Project hat on) my own house in order. Getting Mailman not to modify messages So, I needed our Mailman to stop modifying the headers. I needed it to not even reformat them. A brief look at the source code to Mailman showed that this was not going to be so easy. Mailman has a lot of features whose very purpose is to modify messages. Personally, as I say, I don't much like these features. I think the subject line tags, CC list manipulations, and so on, are a nuisance and not really Proper. But they are definitely part of why Mailman has become so popular and I can definitely see why the Mailman authors have done things this way. But these features mean Mailman has to disassemble incoming messages, and then reassemble them again on output. It is very difficult to do that and still faithfully reassemble the original headers byte-for-byte in the case where nothing actually wanted to modify them. There are existing bug reports[1] [2] [3] [4]; I can see why they are still open. Rejected approach: From:-mangling This situation is hardly unique to the Xen lists. Many other have struggled with it. The best that seems to have been come up with so far is to turn on a new Mailman feature which rewrites the From: header of the messages that go through it, to contain the list's domain name instead of the originator's. I think this is really pretty nasty. It breaks normal use of email, such as reply-to-author. It is having Mailman do additional mangling of the message in order to solve the problems caused by other undesirable manglings! Solution! As you can see, I asked myself: I want Mailman not modify messages at all; how can I get it to do that? Given the existing structure of Mailman - with a lot of message-modifying functionality - that would really mean adding a bypass mode. It would have to spot, presumably depending on config settings, that messages were not to be edited; and then, it would avoid disassembling and reassembling the message at at all, and bypass the message modification stages. The message would still have to be parsed of course - it's just that the copy send out ought to be pretty much the incoming message. When I put it to myself like that I had a thought: couldn't I implement this outside Mailman? What if I took a copy of every incoming message, and then post-process Mailman's output to restore the original? It turns out that this is quite easy and works rather well! outflank-mailman outflank-mailman is a 233-line script, plus documentation, installation instructions, etc. It is designed to run from your MTA, on all messages going into, and coming from, Mailman. On input, it saves a copy of the message in a sqlite database, and leaves a note in a new Outflank-Mailman-Id header. On output, it does some checks, finds the original message, and then combines the original incoming message with carefully-selected headers from the version that Mailman decided should be sent. This was deployed for the Xen Project lists on Tuesday morning and it seems to be working well so far. If you administer Mailman lists, and fancy some new software to address this problem, please do try it out. Matters arising - Mail filtering, DKIM Overall I think DKIM is a helpful contribution to the fight against spam (unlike SPF, which is fundamentally misdirected and also broken). Spam is an extremely serious problem; most receiving mail servers experience more attempts to deliver spam than real mail, by orders of magnitude. But DKIM is not without downsides. Inherent in the design of anything like DKIM is that arbitrary modification of messages by list servers is no longer possible. In principle it might be possible to design a system which tolerated modifications reasonable for mailing lists but it would be quite complicated and have to somehow not tolerate similar modifications in other contexts. So DKIM means that lists can no longer add those unsubscribe footers to mailing list messages. The "new way" (RFC2369, July 1998), to do this is with the List-Unsubscribe header. Hopefully a good MUA will be able to deal with unsubscription semiautomatically, and I think by now an adequate MUA should at least display these headers by default. Sender: There are implications for recipient-side filtering too. The "traditional" correct way to spot mailing list mail was to look for Resent-To:, which can be added without breaking DKIM; the "new" (RFC2919, March 2001) correct way is List-Id:, likewise fine. But during the initial deployment of outflank-mailman I discovered that many subscribers were detecting that a message was list traffic by looking at the Sender: header. I'm told that some mail systems (apparently Microsoft's included) make it inconvenient to filter on List-Id. Really, I think a mailing list ought not to be modifying Sender:. Given Sender:'s original definition and semantics, there might well be reasonable reasons for a mailing list posting to have different From: and and then the original Sender: ought not to be lost. And a mailing list's operation does not fit well into the original definition of Sender:. I suspect that list software likes to put in Sender mostly for historical reasons; notably, a long time ago it was not uncommon for broken mail systems to send bounces to the Sender: header rather than the envelope sender (SMTP MAIL FROM). DKIM makes this more of a problem. Unfortunately the DKIM specifications are vague about what headers one should sign, but they pretty much definitely include Sender: if it is present, and some materials encourage signing the absence of Sender:. The latter is Exim's default configuration when DKIM-signing is enabled. Franky there seems little excuse for systems to not readily support and encourage filtering on List-Id, 20 years later, but I don't want to make life hard for my users. For now we are running a compromise configuration: if there wasn't a Sender: in the original, take Mailman's added one. This will result in (i) misfiltering for some messages whose poster put in a Sender:, and (ii) DKIM failures for messages whose originating system signed the absence of a Sender:. I'm going to mine the db for some stats after it's been deployed for a week or so, to see which of these problems is worst and decide what to do about it. Mail routing For DKIM to work, messages being sent From: a particular mail domain must go through a system trusted by that domain, so they can be signed. Most users tend to do this anyway: their mail provider gives them an IMAP server and an authenticated SMTP submission server, and they configure those details in their MUA. The MUA has a notion of "accounts" and according to the user's selection for an outgoing message, connects to the authenticated submission service (usually using TLS over the global internet). Trad unix systems where messages are sent using the local sendmail or localhost SMTP submission (perhaps by automated systems, or perhaps by human users) are fine too. The smarthost can do the DKIM signing. But this solution is awkward for a user of a trad MUA in what I'll call "alias account" setups: where a user has an address at a mail domain belonging to different people to the system on which they run their MUA (perhaps even several such aliases for different hats). Traditionally this worked by the mail domain forwarding incoming the mail, and the user simply self-declaring their identity at the alias domain. Without DKIM there is nothing stopping anyone self-declaring their own From: line. If DKIM is to be enabled for such a user (preventing people forging mail as that user), the user will have to somehow arrange that their trad unix MUA's outbound mail stream goes via their mail alias provider. For a single-user sending unix system this can be done with tolerably complex configuration in an MTA like Exim. For shared systems this gets more awkward and might require some hairy shell scripting etc.
edited 2020-10-01 21:22 and 21:35 and -02 10:50 +0100 to fix typos and 21:28 to linkify "my small program" in the tl;dr


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1 October 2020

Russ Allbery: Review: Harrow the Ninth

Review: Harrow the Ninth, by Tamsyn Muir
Series: The Locked Tomb #2
Publisher: Tor
Copyright: 2020
ISBN: 1-250-31320-1
Format: Kindle
Pages: 510
Harrow the Ninth is a direct sequel to Gideon the Ninth and under absolutely no circumstances should you start reading here. You would be so lost. If you plan on reading this series, read the books as closely together as you can so that you can remember the details of the previous book. You may still resort to re-reading or searching through parts of the previous book as you go. Muir is doing some complex structural work with Harrow the Ninth, so it's hard to know how much to say about it without spoiling some aspect of it for someone. I think it's safe to say this much: As advertised by the title, we do get a protagonist switch to Harrowhark. However, unlike Gideon the Ninth, it's not a single linear story. The storyline that picks up after the conclusion of Gideon is interwoven with apparent flashbacks retelling the story of the previous book from Harrowhark's perspective. Or at least it might have been the story of the previous book, except that Ortus is Harrowhark's cavalier, Gideon does not appear, and other divergences from the story we previously read become obvious early on. (You can see why memory of Gideon the Ninth is important.) Oh, and one of those storylines is written in the second person. Unlike some books that use this as a gimmick, this is for reasons that are eventually justified and partly explained in the story, but it's another example of the narrative complexity. Harrow the Ninth is dropping a lot of clues (and later revelations) in both story events and story structure, many of which are likely to upend reader expectations from the first book. I have rarely read a novel that is this good at fulfilling the tricky role of the second book of a trilogy. Gideon the Ninth was, at least on the surface, a highly entertaining, linear, and relatively straightforward escape room mystery, set against a dying-world SF background that was more hinted at than fleshed out. Harrow the Ninth revisits and reinterprets that book in ways that add significant depth without feeling artificial. Bits of scenery in the first book take on new meaning and intention. Characters we saw only in passing get a much larger role (and Abigail is worth the wait). And we get a whole ton of answers: about the God Emperor, about Lyctors, about the world, about Gideon and Harrowhark's own pasts and backgrounds, and about the locked tomb that is at the center of the Ninth House. But there is still more than enough for a third book, including a truly intriguing triple cliffhanger ending. Harrow the Ninth is both satisfying in its own right and raises new questions that I'm desperate to see answered in the third book. Also, to respond to my earlier self on setting, this world is not a Warhammer 40K universe, no matter how much it may have appeared in the glimpses we got in Gideon. The God Emperor appears directly in this book and was not at all what I was expecting, if perhaps even more disturbing. Muir is intentionally playing against type, drawing a sharp contrast between the God Emperor and the dramatic goth feel of the rest of the universe and many of the characters, and it's creepily effective and goes in a much different ethical direction than I had thought. (That said, I will warn that properly untangling the ethical dilemmas of this universe is clearly left to the third book.) I mentioned in my review of Gideon the Ninth that I was happy to see more SF pulling unapologetically from fanfic. I'm going to keep beating that drum in this review in part because I think the influence may be less obvious to the uninitiated. Harrow the Ninth is playing with voice, structure, memory, and chronology in ways that I suspect the average reader unfamiliar with fanfic may associate more with literary fiction, but they would be wrongly underestimating fanfic if they did so. If anything, the callouts to fanfic are even clearer. There are three classic fanfic alternate universe premises that appear in passing, the story relies on the reader's ability to hold a canonical narrative and an alternate narrative in mind simultaneously, and the genre inspiration was obvious enough to me that about halfway through the novel I correctly guessed one of the fanfic universes in which Muir has written. (I'm not naming it here since I think it's a bit of a spoiler.) And of course there's the irreverence. There are some structural reasons why the narrative voice isn't quite as good as Gideon the Ninth at the start, but rest assured that Muir makes up for that by the end of the book. My favorite scenes in the series so far happen at the end of Harrow the Ninth: world-building, revelations, crunchy metaphysics, and irreverent snark all woven beautifully together. Muir has her characters use Internet meme references like teenagers, which is a beautiful bit of characterization because they are teenagers. In a world that's heavy on viscera, skeletons, death, and horrific monsters, it's a much needed contrast and a central part of how the characters show defiance and courage. I don't think this will work for everyone, but it very much works for me. There's a Twitter meme reference late in the book that had me laughing out loud in delight. Harrow the Ninth is an almost perfect second book, in that if you liked Gideon the Ninth, you will probably love Harrow the Ninth and it will make you like Gideon the Ninth even more. It does have one major flaw, though: pacing. This was also my major complaint about Gideon, primarily around the ending. I think Harrow the Ninth is a bit better, but the problem has a different shape. The start of the book is a strong "what the hell is going on" experience, which is very effective, and the revelations are worth the build-up once they start happening. In between, though, the story drags on a bit too long. Harrow is sick and nauseated at the start of the book for rather longer than I wanted to read about, there is one too many Lyctor banquets than I think were necessary to establish the characters, and I think there's a touch too much wandering the halls. Muir also interwove two narrative threads and tried to bring them to a conclusion at the same time, but I think she had more material for one than the other. There are moments near the end of the book where one thread is producing all the payoff revelations the reader has been waiting for, and the other thread is following another interminable and rather uninteresting fight scene. You don't want your reader saying "argh, no" each time you cut away to the other scene. It's better than Gideon the Ninth, where the last fifth of the book is mostly a running battle that went on way longer than it needed to, but I still wish Muir had tightened the story throughout and balanced the two threads so that we could stay with the most interesting one when it mattered. That said, I mostly noticed the pacing issues in retrospect and in talking about them with a friend who was more annoyed than I was. In the moment, there was so much going on here, so many new things to think about, and so much added depth that I devoured Harrow the Ninth over the course of two days and then spent the next day talking to other people who had read it, trading theories about what happened and what will happen in the third book. It was the most enjoyable reading experience I've had so far this year. Gideon the Ninth was fun; Harrow the Ninth was both fun and on the verge of turning this series into something truly great. I can hardly wait for Alecto the Ninth (which doesn't yet have a release date, argh). As with Gideon the Ninth, content warning for lots and lots of gore, rather too detailed descriptions of people's skeletons, restructuring bits of the body that shouldn't be restructured, and more about bone than you ever wanted to know. Rating: 9 out of 10

30 September 2020

Utkarsh Gupta: FOSS Activites in September 2020

Here s my (twelfth) monthly update about the activities I ve done in the F/L/OSS world.

Debian
This was my 21st month of contributing to Debian. I became a DM in late March last year and a DD last Christmas! \o/ I ve been busy with my undergraduation stuff but I still squeezed out some time for the regular Debian work. Here are the following things I did in Debian this month:

Uploads and bug fixes:

Other $things:
  • Attended the Debian Ruby team meeting. Logs here.
  • Mentoring for newcomers.
  • FTP Trainee reviewing.
  • Moderation of -project mailing list.
  • Sponsored trace-cmd for Sudip, ruby-asset-sync for Nilesh, and mariadb-mysql-kbs for William.

RuboCop::Packaging - Helping the Debian Ruby team! \o/ This Google Summer of Code, I worked on writing a linter that could flag offenses for lines of code that are very troublesome for Debian maintainers while trying to package and maintain Ruby libraries and applications! Whilst the GSoC period is over, I ve been working on improving that tool and have extended that linter to now auto-correct these offenses by itself! \o/
You can now just use the -A flag and you re done! Boom! The ultimate game-changer! Here s a quick demo for this feature: A few quick updates on RuboCop::Packaging: I ve also spent a considerable amount of time in raising awareness about this and in more general sense, about downstream maintenance.
As a result, I raised a bunch of PRs which got really good response. I got all of the 20 PRs merged upstream, fixing these issues.

Debian (E)LTS
Debian Long Term Support (LTS) is a project to extend the lifetime of all Debian stable releases to (at least) 5 years. Debian LTS is not handled by the Debian security team, but by a separate group of volunteers and companies interested in making it a success. And Debian Extended LTS (ELTS) is its sister project, extending support to the Jessie release (+2 years after LTS support). This was my twelfth month as a Debian LTS and third month as a Debian ELTS paid contributor.
I was assigned 19.75 hours for LTS and 15.00 hours for ELTS and worked on the following things:
(for LTS, I over-worked for 11 hours last month on the survey so only had 8.75 hours this month!)

LTS CVE Fixes and Announcements:

ELTS CVE Fixes and Announcements:
  • Issued ELA 274-1, fixing CVE-2020-11984, for uwsgi.
    For Debian 8 Jessie, these problems have been fixed in version 2.0.7-1+deb8u3.
  • Issued ELA 275-1, fixing CVE-2020-14363, for libx11.
    For Debian 8 Jessie, these problems have been fixed in version 2:1.6.2-3+deb8u4.
  • Issued ELA 278-1, fixing CVE-2020-8184, for ruby-rack.
    For Debian 8 Jessie, these problems have been fixed in version 1.5.2-3+deb8u4.
  • Also worked on updating the version of clamAV from v0.101.5 to v0.102.4.
    This was a bit tricky package to work on since it involved an ABI/API change and was more or less a transition. Super thanks to Emilio for his invaluable help and him taking over the package, finishing, and uploading it in the end.

Other (E)LTS Work:
  • Front-desk duty from 31-08 to 06-09 and from 28-09 onward for both LTS and ELTS.
  • Triaged apache2, cryptsetup, nasm, node-bl, plinth, qemu, rsync, ruby-doorkeeper, and uwsgi.
  • Marked CVE-2020-15094/symfony as not-affected for Stretch.
  • Marked CVE-2020- 9490,11993 /apache2 as ignored for Stretch.
  • Marked CVE-2020-8244/node-bl as no-dsa for Stretch.
  • Marked CVE-2020-24978/nasm as no-dsa for Stretch.
  • Marked CVE-2020-25073/plinth as no-dsa for Stretch.
  • Marked CVE-2020-15094/symfony as not-affected for Jessie.
  • Marked CVE-2020-14382/cryptsetup as not-affected for Jessie.
  • Marked CVE-2020-14387/rsync as not-affected for Jessie.
  • Auto EOL ed ark, collabtive, linux, nasm, node-bl, and thunderbird for Jessie.
  • Use mktemp instead of tempfile in bin/auto-add-end-of-life.sh.
  • Attended the fifth LTS meeting. Logs here.
  • General discussion on LTS private and public mailing list.

Until next time.
:wq for today.

27 September 2020

Norbert Preining: Cinnamon for Debian imminent possible removal from testing

Update 2020-09-30: The post has created considerable movement, and a PR request by Fedora developers to rebase cjs onto more current gjs and libmozjs78 is being tested. I have uploaded packages of cinnamon and cjs to experimental based on these patches (400 files, about 50000 lines of code touched, not what I normally like to have in a debian patch) and would appreciate testing and feedback. I have been more or less maintaining Cinnamon now for quite some time, but using it only sporadically due to my switch to KDE/Plasma. Currently, Cinnamon s cjs package depends on mozjs52, which also is probably going to be orphaned soon. This will precipitate a lot of changes, not the least being Cinnamon being removed from Debian/testing. I have pinged upstream several times, without much success. So for now the future looks bleak for cinnamon in Debian. If there are interested developers (Debian or not), please get in touch with me, or directly try to update cjs to mozjs78.

Iain R. Learmonth: Multicast IPTV

For almost a decade, I ve been very slowly making progress on a multicast IPTV system. Recently I ve made a significant leap forward in this project, and I wanted to write a little on the topic so I ll have something to look at when I pick this up next. I was aspiring to have a useable system by the end of today, but for a couple of reasons, it wasn t possible. When I started thinking about this project, it was still common to watch broadcast television. Over time the design of this system has been changing as new technologies have become available. Multicast IP is probably the only constant, although I m now looking at IPv6 rather than IPv4. Initially, I d been looking at DVB-T PCI cards. USB devices have become common and are available cheaply. There are also DVB-T hats available for the Raspberry Pi. I m now looking at a combination of Raspberry Pi hats and USB devices with one of each on a couple of Pis.
Two Raspberry Pis with DVB hats installed, TV antenna sockets showing Two Raspberry Pis with DVB hats installed, TV antenna sockets showing
The Raspberry Pi devices will run DVBlast, an open-source DVB demultiplexer and streaming server. Each of the tuners will be tuned to a different transponder giving me the ability to stream any combination of available channels simultaneously. This is everything that would be needed to watch TV on PCs on the home network with VLC. I ve not yet worked out if Kodi will accept multicast streams as a TV source, but I do know that Tvheadend will. Tvheadend can also act as a PVR to record programmes for later playback so is useful even if the multicast streams can be viewed directly. So how far did I get? I have built two Raspberry Pis in cases with the DVB-T hats on. They need to sit in the lounge as that s where the antenna comes down from the roof. There s no wired network connection in the lounge. I planned to use an OpenBSD box as a gateway, bridging the wireless network to a wired network. Two problems quickly emerged. The first being that the wireless card I had purchased only supported 2.4GHz, no 5GHz, and I have enough noise from neighbours that the throughput rate and packet loss are unacceptable. The second problem is that I had forgotten the problems with bridging wireless networks. To create a bridge, you need to be able to spoof the MAC addresses of wired devices on the wireless interface, but this can only be done when the wireless interface is in access point mode. So when I come back to this, I will have to look at routing rather than bridging to work around the MAC address issue, and I ll also be on the lookout for a cheap OpenBSD supported mini-PCIe wireless card that can do 5GHz.

Dirk Eddelbuettel: pkgKitten 0.2.0: Now with tinytest and new docs

kitten A new release 0.2.0 of pkgKitten just hit on CRAN today, or about eleven months after the previous release. This release brings support for tinytest by having pkgKitten::kitten() automagically call tinytest::puppy() if the latter package is installed (and the user did not opt out of calling it). So your newly created minimal package now also uses a wonderful yet tiny testing framework. We also added a new documentation site using the previously tweeted-about wrapper for Material for MkDocs I really dig. And last but not least we switched to BSPM-based Continued Integration (which I wrote about yesterday in R4 #30) and fixed one bug regarding the default NAMESPACE file.

Changes in version 0.2.0 (2020-09-27)
  • Continuous Integration uses the updated BSPM-based script on Travis and with GitHub Actions (Dirk in #11 plus earlier commits).
  • A new default NAMESPACE file is now installed (Dirk in #12).
  • A package documentation website was added (Dirk in #13).
  • Call tinytest::puppy if installed and not opted out (Dirk in #14).

More details about the package are at the pkgKitten webpage, the (new) pkgKitten docs site, and the pkgKitten GitHub repo. Courtesy of my CRANberries site, there is also a diffstat report for this release. If you like this or other open-source work I do, you can now sponsor me at GitHub. For the first year, GitHub will match your contributions.

This post by Dirk Eddelbuettel originated on his Thinking inside the box blog. Please report excessive re-aggregation in third-party for-profit settings.

26 September 2020

Andrew Cater: There's a Debian point release for Debian stable happening this weekend - 10.6

Nothing particularly new or unexpected: there's a point release happening at some point this weekend for Debian stable. Usual rules apply: if you've already got a system current and up to date, there's not much to do but the base files version will change at some point to reflect 10.6 when you next update. If you have media from 10.5, you may not _have_ to go and get media this weekend but it's always useful to get new media in due course. There's an updated kernel and an ABI bump. You _will_ need to reboot at some time to use the new kernel image.
This point release will contain security fixes, consequent changes etc. as usual - it is always good and useful to keep machines up to date.Working with the CD team to eventually test, build and release CD / DVD images and media as and when files gradually become available. As ever, this may take 12-16 hours. As ever, I'll post some blog entries as we go.Currently "sitting in Cambridge" via video link with Sledge, RattusRattus and Isy who are all involved in the testing and we'll have a great day, as ever.

Fran ois Marier: Repairing a corrupt ext4 root partition

I ran into filesystem corruption (ext4) on the root partition of my backup server which caused it to go into read-only mode. Since it's the root partition, it's not possible to unmount it and repair it while it's running. Normally I would boot from an Ubuntu live CD / USB stick, but in this case the machine is using the mipsel architecture and so that's not an option.

Repair using a USB enclosure I had to pull the shutdown the server and then pull the SSD drive out. I then moved it to an external USB enclosure and connected it to my laptop. I started with an automatic filesystem repair:
fsck.ext4 -pf /dev/sde2
which failed for some reason and so I moved to an interactive repair:
fsck.ext4 -f /dev/sde2
Once all of the errors were fixed, I ran a full surface scan to update the list of bad blocks:
fsck.ext4 -c /dev/sde2
Finally, I forced another check to make sure that everything was fixed at the filesystem level:
fsck.ext4 -f /dev/sde2

Fix invalid alternate GPT The other thing I noticed is this messge in my dmesg log:
scsi 8:0:0:0: Direct-Access     KINGSTON  SA400S37120     SBFK PQ: 0 ANSI: 6
sd 8:0:0:0: Attached scsi generic sg4 type 0
sd 8:0:0:0: [sde] 234441644 512-byte logical blocks: (120 GB/112 GiB)
sd 8:0:0:0: [sde] Write Protect is off
sd 8:0:0:0: [sde] Mode Sense: 31 00 00 00
sd 8:0:0:0: [sde] Write cache: enabled, read cache: enabled, doesn't support DPO or FUA
sd 8:0:0:0: [sde] Optimal transfer size 33553920 bytes
Alternate GPT is invalid, using primary GPT.
 sde: sde1 sde2
I therefore checked to see if the partition table looked fine and got the following:
$ fdisk -l /dev/sde
GPT PMBR size mismatch (234441643 != 234441647) will be corrected by write.
The backup GPT table is not on the end of the device. This problem will be corrected by write.
Disk /dev/sde: 111.8 GiB, 120034123776 bytes, 234441648 sectors
Disk model: KINGSTON SA400S3
Units: sectors of 1 * 512 = 512 bytes
Sector size (logical/physical): 512 bytes / 512 bytes
I/O size (minimum/optimal): 512 bytes / 512 bytes
Disklabel type: gpt
Disk identifier: 799CD830-526B-42CE-8EE7-8C94EF098D46
Device       Start       End   Sectors   Size Type
/dev/sde1     2048   8390655   8388608     4G Linux swap
/dev/sde2  8390656 234441614 226050959 107.8G Linux filesystem
It turns out that all I had to do, since only the backup / alternate GPT partition table was corrupt and the primary one was fine, was to re-write the partition table:
$ fdisk /dev/sde
Welcome to fdisk (util-linux 2.33.1).
Changes will remain in memory only, until you decide to write them.
Be careful before using the write command.
GPT PMBR size mismatch (234441643 != 234441647) will be corrected by write.
The backup GPT table is not on the end of the device. This problem will be corrected by write.
Command (m for help): w
The partition table has been altered.
Syncing disks.

Run SMART checks Since I still didn't know what caused the filesystem corruption in the first place, I decided to do one last check: SMART errors. I couldn't do this via the USB enclosure since the SMART commands aren't forwarded to the drive and so I popped the drive back into the backup server and booted it up. First, I checked whether any SMART errors had been reported using smartmontools:
smartctl -a /dev/sda
That didn't show any errors and so I kicked off an extended test:
smartctl -t long /dev/sda
which ran for 30 minutes and then passed without any errors. The mystery remains unsolved.

Dirk Eddelbuettel: #30: Easy, Reliable, Fast and Portable Linux and macOS Continuous Integration

Welcome to the 30th post in the rarified R recommendation resources series or R4 for short. The last post introduced BSPM. In the four weeks since, we have worked some more on BSPM to bring it to the point where it is ready for use with continuous integration. Building on this, it is now used inside the run.sh script that driven our CI use for many years (via the r-travis repo). Which we actually use right now on three different platforms: All three use the exact same script facilitating this, and run a matrix over Linux and macOS. You read this right: one CI setup that is portable and which you can take to your CI provider of choice. No lock-in or tie-in. Use what works, change at will. Or run on all three if you like burning extra cycles. This is already used by handful of my repos as well as by at least two repos of friends also deploying r-travis. How does it work? In a nutshell we are There are several customizations that are possible via environment variables We find this setup compelling. The scheme is simple: there really is just one shell script behind it which can also be downloaded and altered. The scheme is also portable as we can (as shown) rotate between CI provides. The scheme is also more flexible: in case of debugging needs one can simply run the script on a local Docker or VM instance. Lastly, the scheme moves away from single points of failure or breakage. Currently the script uses only BSPM as I had the hunch that it would a) work and b) be compelling. Adding support for RSPM would be equally easy, but I have no immediate need to do so. Adding BioConductor installation may be next. That is easy when BioConductor uses r-release; it may be little more challenging under r-devel to but it should work too. Stay tuned. In the meantime, if the above sounds compelling, give run.sh from r-travis a go! If you like this or other open-source work I do, you can now sponsor me at GitHub. For the first year, GitHub will match your contributions.

This post by Dirk Eddelbuettel originated on his Thinking inside the box blog. Please report excessive re-aggregation in third-party for-profit settings.

25 September 2020

Russell Coker: Bandwidth for Video Conferencing

For the Linux Users of Victoria (LUV) I ve run video conferences on Jitsi and BBB (see my previous post about BBB vs Jitsi [1]). One issue with video conferences is the bandwidth requirements. The place I m hosting my video conference server has a NBN link with allegedly 40Mb/s transmission speed and 100Mb/s reception speed. My tests show that it can transmit at about 37Mb/s and receive at speeds significantly higher than that but also quite a bit lower than 100Mb/s (around 60 or 70Mb/s). For a video conference server you have a small number of sources of video and audio and a larger number of targets as usually most people will have their microphones muted and video cameras turned off. This means that the transmission speed is the bottleneck. In every test the reception speed was well below half the transmission speed, so the tests confirmed my expectation that transmission was the only bottleneck, but the reception speed was higher than I had expected. When we tested bandwidth use the maximum upload speed we saw was about 4MB/s (32Mb/s) with 8+ video cameras and maybe 20 people seeing some of the video (with a bit of lag). We used 3.5MB/s (28Mb/s) when we only had 6 cameras which seemed to be the maximum for good performance. In another test run we had 4 people all sending video and the transmission speed was about 260KB/s. I don t know how BBB manages the small versions of video streams. It might reduce the bandwidth when the display window is smaller. I don t know the resolutions of the cameras. When you start sending video in BBB you are prompted for the quality with medium being default. I don t know how different camera hardware and different choices about quality affect bandwidth. These tests showed that for the cameras we had available a small group of people video chatting a 100/40 NBN link (the fastest Internet link in Australia that s not really expensive) a small group of people can be all sending video or a medium size group of people can watch video streams from a small group. For meetings of the typical size of LUV meetings we won t have a bandwidth problem. There is one common case that I haven t yet tested, where there is a single video stream that many people are watching. If 4 people are all sending video with 260KB/s transmission bandwidth then 1 person could probably send video to 4 for 65KB/s. Doing some simple calculations on those numbers implies that we could have 1 person sending video to 240 people without running out of bandwidth. I really doubt that would work, but further testing is needed.

Colin Watson: Porting Launchpad to Python 3: progress report

Launchpad still requires Python 2, which in 2020 is a bit of a problem. Unlike a lot of the rest of 2020, though, there s good reason to be optimistic about progress. I ve been porting Python 2 code to Python 3 on and off for a long time, from back when I was on the Ubuntu Foundations team and maintaining things like the Ubiquity installer. When I moved to Launchpad in 2015 it was certainly on my mind that this was a large body of code still stuck on Python 2. One option would have been to just accept that and leave it as it is, maybe doing more backporting work over time as support for Python 2 fades away. I ve long been of the opinion that this would doom Launchpad to being unmaintainable in the long run, and since I genuinely love working on Launchpad - I find it an incredibly rewarding project - this wasn t something I was willing to accept. We re already seeing some of our important dependencies dropping support for Python 2, which is perfectly reasonable on their terms but which is starting to become a genuine obstacle to delivering important features when we need new features from newer versions of those dependencies. It also looks as though it may be difficult for us to run on Ubuntu 20.04 LTS (we re currently on 16.04, with an upgrade to 18.04 in progress) as long as we still require Python 2, since we have some system dependencies that 20.04 no longer provides. And then there are exciting new features like type hints and async/await that we d like to be able to use. However, until last year there were so many blockers that even considering a port was barely conceivable. What changed in 2019 was sorting out a trifecta of core dependencies. We ported our database layer, Storm. We upgraded to modern versions of our Zope Toolkit dependencies (after contributing various fixes upstream, including some substantial changes to Zope s test runner that we d carried as local patches for some years). And we ported our Bazaar code hosting infrastructure to Breezy. With all that in place, a port seemed more of a realistic possibility. Still, even with this, it was never going to be a matter of just following some standard porting advice and calling it good. Launchpad has almost a million lines of Python code in its main git tree, and around 250 dependencies of which a number are quite Launchpad-specific. In a project that size, not only is following standard porting advice an extremely time-consuming task in its own right, but just about every strange corner case is going to show up somewhere. (Did you know that StringIO.StringIO(None) and io.StringIO(None) do different things even after you account for the native string vs. Unicode text difference? How about the behaviour of .union() on a subclass of frozenset?) Launchpad s test suite is fortunately extremely thorough, but even just starting up the test suite involves importing most of the data model code, so before you can start taking advantage of it you have to make a large fraction of the codebase be at least syntactically-correct Python 3 code and use only modules that exist in Python 3 while still working in Python 2; in a project this size that turns out to be a large effort on its own, and can be quite risky in places. Canonical s product engineering teams work on a six-month cycle, but it just isn t possible to cram this sort of thing into six months unless you do literally nothing else, and please can we put all feature development on hold while we run to stand still is a pretty tough sell to even the most understanding management. Fortunately, we ve been able to grow the Launchpad team in the last year or so, and so it s been possible to put Python 3 on our roadmap on the understanding that we aren t going to get all the way there in one cycle, while still being able to do other substantial feature development work as well. So, with all that preamble, what have we done this cycle? We ve taken a two-pronged approach. From one end, we identified 147 classes that needed to be ported away from some compatibility code in our database layer that was substantially less friendly to Python 3: we ve ported 38 of those, so there s clearly a fair bit more to do, but we were able to distribute this work out among the team quite effectively. From the other end, it was clear that it would be very inefficient to do general porting work when any attempt to even run the test suite would run straight into the same crashes in the same order, so I set myself a target of getting the test suite to start up, and started hacking on an enormous git branch that I never expected to try to land directly: instead, I felt free to commit just about anything that looked reasonable and moved things forward even if it was very rough, and every so often went back to tidy things up and cherry-pick individual commits into a form that included some kind of explanation and passed existing tests so that I could propose them for review. This strategy has been dramatically more successful than anything I ve tried before at this scale. So far this cycle, considering only Launchpad s main git tree, we ve landed 137 Python-3-relevant merge proposals for a total of 39552 lines of git diff output, keeping our existing tests passing along the way and deploying incrementally to production. We have about 27000 more lines of patch at varying degrees of quality to tidy up and merge. Our main development branch is only perhaps 10 or 20 more patches away from the test suite being able to start up, at which point we ll be able to get a buildbot running so that multiple developers can work on this much more easily and see the effect of their work. With the full unlanded patch stack, about 75% of the test suite passes on Python 3! This still leaves a long tail of several thousand tests to figure out and fix, but it s a much more incrementally-tractable kind of problem than where we started. Finally: the funniest (to me) bug I ve encountered in this effort was the one I encountered in the test runner and fixed in zopefoundation/zope.testrunner#106: IDs of failing tests were written to a pipe, so if you have a test suite that s large enough and broken enough then eventually that pipe would reach its capacity and your test runner would just give up and hang. Pretty annoying when it meant an overnight test run didn t give useful results, but also eloquent commentary of sorts.

Reproducible Builds: ARDC sponsors the Reproducible Builds project

The Reproducible Builds project is pleased to announce a donation from Amateur Radio Digital Communications (ARDC) in support of its goals. ARDC s contribution will propel the Reproducible Builds project s efforts in ensuring the future health, security and sustainability of our increasingly digital society.

About Amateur Radio Digital Communications (ARDC) Amateur Radio Digital Communications (ARDC) is a non-profit that was formed to further research and experimentation with digital communications using radio, with a goal of advancing the state of the art of amateur radio and to educate radio operators in these techniques. It does this by managing the allocation of network resources, encouraging research and experimentation with networking protocols and equipment, publishing technical articles and number of other activities to promote the public good of amateur radio and other related fields. ARDC has recently begun to contribute funding to organisations, groups, individuals and projects towards these and related goals, and their grant to the Reproducible Builds project is part of this new initiative. Amateur radio is an entirely volunteer activity performed by knowledgeable hobbyists who have proven their ability by passing the appropriate government examinations. No remuneration is permitted. Ham radio, as it is also known, has proven its value in advancements of the state of the communications arts, as well as in public service during disasters and in times of emergency. For more information about ARDC, please see their website at ampr.org.

About the Reproducible Builds project One of the original promises of open source software was that peer review would result in greater end-user security and stability of our digital ecosystem. However, although it is theoretically possible to inspect and build the original source code in order to avoid maliciously-inserted flaws, almost all software today is distributed in prepackaged form. This disconnect allows third-parties to compromise systems by injecting code into seemingly secure software during the build process, as well as by manipulating copies distributed from app stores and other package repositories. In order to address this, Reproducible builds are a set of software development practices, ideas and tools that create an independently-verifiable path from the original source code, all the way to what is actually running on our machines. Reproducible builds can reveal the injection of backdoors introduced by the hacking of developers own computers, build servers and package repositories, but can also expose where volunteers or companies have been coerced into making changes via blackmail, government order, and so on. A world without reproducible builds is a world where our digital infrastructure cannot be trusted and where online communities are slower to grow, collaborate less and are increasingly fragile. Without reproducible builds, we leave space for greater encroachments on our liberties both by individuals as well as powerful, unaccountable actors such as governments, large corporations and autocratic regimes. The Reproducible Builds project began as a project within the Debian community, but is now working with many crucial and well-known free software projects such as Coreboot, openSUSE, OpenWrt, Tails, GNU Guix, Arch Linux, Tor, and many others. It is now an entirely Linux distribution independent effort and serves as the central clearing house for all issues related to securing build systems and software supply chains of all kinds. For more about the Reproducible Builds project, please see their website at reproducible-builds.org.
If you are interested in ensuring the ongoing security of the software that underpins our civilisation, and wish to sponsor the Reproducible Builds project, please reach out to the project by emailing contact@reproducible-builds.org.

23 September 2020

Vincent Fourmond: Tutorial: analyze Km data of CODHs

This is the first post of a series in which we will provide the readers with simple tutorial approaches to reproduce the data analysis of some of our published papers. All our data analysis is performed using QSoas. Today, we will show you how to analyze the experiments we used to characterize the behaviour of an enzyme, the Nickel-Iron CO dehydrogenase IV from Carboxytothermus hydrogenoformans. The experiments we analyze here are described in much more details in the original publication, Domnik et al, Angewandte Chemie, 2017. The only things you need to know for now are the following: This means that we expect a response of the type: $$i(t) = \frac i_m 1 + \frac K_m [\mathrm CO ](t) $$ in which $$[\mathrm CO ](t) = \begin cases 0, & \text for t < t_0 \\ C_0 \exp \frac t_0 - t \tau , & \text for t\geq t_0 %> \end cases $$ To begin this tutorial, first download the files from the github repository (direct links: data, parameter file and ruby script). Start QSoas, go to the directory where you saved the files, load the data file, and remove spikes in the data using the following commands:
QSoas> cd
QSoas> l Km-CODH-IV.dat
QSoas> R
First fitThen, to fit the above equation to the data, the simplest is to take advantage of the time-dependent parameters features of QSoas. Run simply:
QSoas> fit-arb im/(1+km/s) /with=s:1,exp
This simply launches the fit interface to fit the exact equations above. The im/(1+km/s) is simply the translation of the Michaelis-Menten equation above, and the /with=s:1,exp specifies that s is the result of the sum of 1 exponential like for the definition of above. Then, load the Km-CODH-IV.params parameter files (using the "Parameters.../Load from file" action at the bottom, or the Ctrl+L keyboard shortcut). Your window should now look like this:
To fit the data, just hit the "Fit" button ! (or Ctrl+F). Including an offset The fit is not bad, but not perfect. In particular, it is easy to see why: the current predicted by the fit goes to 0 at large times, but the actual current is below 0. We need therefore to include an offset to take this into consideration. Close the fit window, and re-run a fit, but now with this command:
QSoas> fit-arb im/(1+km/s)+io /with=s:1,exp
Notice the +io bit that corresponds to the addition of an offset current. Load again the base parameters, run the fit again... Your fit window show now look like:
See how the offset current is now much better taken into account. Let's talk a bit more about the parameters: Taking into account mass-transport limitations However, the fit is still unsatisfactory: the predicted curve fails to reproduce the curvature at the beginning and at the end of the decrease. This is due to issues linked to mass-transport limitations, which are discussed in details in Merrouch et al, Electrochimica Acta, 2017. In short, what you need to do is to close the fit window again, load the transport.rb Ruby file that contains the definition of the itrpt function, and re-launch the fit window using:
QSoas> ruby-run transport.rb
QSoas> fit-arb itrprt(s,km,nFAm,nFAmu)+io /with=s:1,exp
Load again the parameter file... but this time you'll have to play a bit more with the starting parameters for QSoas to find the right values when you fit. Here are some tips: A successful fit should look like this:
Here you are ! I hope you enjoyed analyzing our data, and that it will help you analyze yours ! Feel free to comment and ask for clarifications.

About QSoasQSoas is a powerful open source data analysis program that focuses on flexibility and powerful fitting capacities. It is released under the GNU General Public License. It is described in Fourmond, Anal. Chem., 2016, 88 (10), pp 5050 5052. Current version is 2.2. You can download its source code or buy precompiled versions for MacOS and Windows there.

Vincent Fourmond: Define a function with inline Ruby code in QSoas

QSoas can read and execute Ruby code directly, while reading command files, or even at the command prompt. For that, just write plain Ruby code inside a ruby...ruby end block. Probably the most useful possibility is to define elaborated functions directly from within QSoas, or, preferable, from within a script; this is an alternative to defining a function in a completely separated Ruby-only file using ruby-run. For instance, you can define a function for plain Michaelis-Menten kinetics with a file containing:

ruby
def my_func(x, vm, km)
  return vm/(1 + km/x)
end
ruby end

This defines the function my_func with three parameters, , (vm) and (km), with the formula:

You can then test that the function has been correctly defined running for instance:

QSoas> eval my_func(1.0,1.0,1.0)
 => 0.5
QSoas> eval my_func(1e4,1.0,1.0)
 => 0.999900009999

This yields the correct answer: the first command evaluates the function with x = 1.0, vm = 1.0 and km = 1.0. For , the result is (here 0.5). For , the result is almost . You can use the newly defined my_func in any place you would use any ruby code, such as in the optional argument to generate-buffer, or for arbitrary fits:

QSoas> generate-buffer 0 10 my_func(x,3.0,0.6)
QSoas> fit-arb my_func(x,vm,km)

To redefine my_func, just run the ruby code again with a new definition, such as:
ruby
def my_func(x, vm, km)
  return vm/(1 + km/x**2)
end
ruby end
The previous version is just erased, and all new uses of my_func will refer to your new definition.


See for yourselfThe code for this example can be found there. Browse the qsoas-goodies github repository for more goodies !

About QSoasQSoas is a powerful open source data analysis program that focuses on flexibility and powerful fitting capacities. It is released under the GNU General Public License. It is described in Fourmond, Anal. Chem., 2016, 88 (10), pp 5050 5052. Current version is 2.1. You can download its source code or buy precompiled versions for MacOS and Windows there.

Russell Coker: Qemu (KVM) and 9P (Virtfs) Mounts

I ve tried setting up the Qemu (in this case KVM as it uses the Qemu code in question) 9P/Virtfs filesystem for sharing files to a VM. Here is the Qemu documentation for it [1].
VIRTFS="-virtfs local,path=/vmstore/virtfs,security_model=mapped-xattr,id=zz,writeout=immediate,fmode=0600,dmode=0700,mount_tag=zz"
VIRTFS="-virtfs local,path=/vmstore/virtfs,security_model=passthrough,id=zz,writeout=immediate,mount_tag=zz"
Above are the 2 configuration snippets I tried on the server side. The first uses mapped xattrs (which means that all files will have the same UID/GID and on the host XATTRs will be used for storing the Unix permissions) and the second uses passthrough which requires KVM to run as root and gives the same permissions on the host as on the VM. The advantages of passthrough are better performance through writing less metadata and having the same permissions in host and VM. The advantages of mapped XATTRs are running KVM/Qemu as non-root and not having a SUID file in the VM imply a SUID file in the host. Here is the link to Bonnie++ output comparing Ext3 on a KVM block device (stored on a regular file in a BTRFS RAID-1 filesystem on 2 SSDs on the host), a NFS share from the host from the same BTRFS filesystem, and virtfs shares of the same filesystem. The only tests that Ext3 doesn t win are some of the latency tests, latency is based on the worst-case not the average. I expected Ext3 to win most tests, but didn t expect it to lose any latency tests. Here is a link to Bonnie++ output comparing just NFS and Virtfs. It s obvious that Virtfs compares poorly, giving about half the performance on many tests. Surprisingly the only tests where Virtfs compared well to NFS were the file creation tests which I expected Virtfs with mapped XATTRs to do poorly due to the extra metadata. Here is a link to Bonnie++ output comparing only Virtfs. The options are mapped XATTRs with default msize, mapped XATTRs with 512k msize (I don t know if this made a difference, the results are within the range of random differences), and passthrough. There s an obvious performance benefit in passthrough for the small file tests due to the less metadata overhead, but as creating small files isn t a bottleneck on most systems a 20% to 30% improvement in that area probably doesn t matter much. The result from the random seeks test in passthrough is unusual, I ll have to do more testing on that. SE Linux On Virtfs the XATTR used for SE Linux labels is passed through to the host. So every label used in a VM has to be valid on the host and accessible to the context of the KVM/Qemu process. That s not really an option so you have to use the context mount option. Having the mapped XATTR mode work for SE Linux labels is a necessary feature. Conclusion The msize mount option in the VM doesn t appear to do anything and it doesn t appear in /proc/mounts, I don t know if it s even supported in the kernel I m using. The passthrough and mapped XATTR modes give near enough performance that there doesn t seem to be a benefit of one over the other. NFS gives significant performance benefits over Virtfs while also using less CPU time in the VM. It has the issue of files named .nfs* hanging around if the VM crashes while programs were using deleted files. It s also more well known, ask for help with an NFS problem and you are more likely to get advice than when asking for help with a virtfs problem. Virtfs might be a better option for accessing databases than NFS due to it s internal operation probably being a better map to Unix filesystem semantics, but running database servers on the host is probably a better choice anyway. Virtfs generally doesn t seem to be worth using. I had hoped for performance that was better than NFS but the only benefit I seemed to get was avoiding the .nfs* file issue. The best options for storage for a KVM/Qemu VM seem to be Ext3 for files that are only used on one VM and for which the size won t change suddenly or unexpectedly (particularly the root filesystem) and NFS for everything else.

22 September 2020

Russ Allbery: Review: Unconquerable Sun

Review: Unconquerable Sun, by Kate Elliott
Series: Sun Chronicles #1
Publisher: Tor
Copyright: 2020
ISBN: 1-250-19725-2
Format: Kindle
Pages: 526
Sun is the daughter and heir of the mercurial Queen-Marshal Eirene, ruler of the Republic of Chaonia. Chaonia, thanks to Eirene and her ancestors, has carved out a fiercely independent position between the Yele League and the Phene Empire. Sun's father, Prince Jo o, is one of Eirene's three consorts, all chosen for political alliances to shore up that fragile position. Jo o is Gatoi, a civilization of feared fighters and supposed barbarians from outside Chaonia who normally ally with the Phene, which complicates Sun's position as heir. Sun attempts to compensate for that by winning battles for the Republic, following in the martial footsteps of her mother. The publisher's summary of this book is not great (I'm a huge fan of Princess Leia, but that is... not the analogy that comes to mind), so let me try to help. This is gender-swapped Alexander the Great in space. However, it is gender-swapped Alexander the Great in space with her Companions, which means the DNA of this novel is half space opera and half heist story (without, to be clear, an actual heist, although there are some heist-like maneuvers). It's also worth mentioning that Sun, like Alexander, is not heterosexual. The other critical thing to know before reading, mostly because it will get you through the rather painful start, is that the most interesting viewpoint character in this book is not Sun, the Alexander analogue. It's Persephone, who isn't introduced until chapter seven. Significant disclaimer up front: I got a reasonably typical US grade school history of Alexander the Great, which means I was taught that he succeeded his father, conquered a whole swath of the middle of the Eurasian land mass at a very young age, and then died and left his empire to his four generals who promptly divided it into four uninteresting empires that no one's ever heard of, and that's why Rome is more important than Greece. (I put in that last bit to troll one specific person.) I am therefore not the person to judge the parallels between this story and known history, or to notice any damage done to Greek pride, or to pick up on elements that might cause someone with a better grasp of that history to break out in hives. I did enough research to know that one scene in this book is lifted directly out of Alexander's life, but I'm not sure how closely the other parallels track. Yele is probably southern Greece and Phene is probably Persia, but I'm not certain even of that, and some of the details don't line up. If I had to hazard a guess, I'd say that Elliott has probably mangled history sufficiently to make it clear that this isn't intended to be a retelling, but if the historical parallels are likely to bother you, you may want to do more research before reading. What I can say is that the space opera setup, while a bit stock, has all the necessary elements to make me happy. Unconquerable Sun is firmly in the "lost Earth" tradition: The Argosy fleet fled the now-mythical Celestial Empire and founded a new starfaring civilization without any contact with their original home. Eventually, they invented (or discovered; the characters don't know) the beacons, which allow for instantaneous travel between specific systems without the long (but still faster-than-light) journeys of the knnu drive. More recently, the beacon network has partly collapsed, cutting off the characters' known world from the civilization that was responsible for the beacons and guarded their secrets. It's a fun space opera history with lots of lost knowledge to reference and possibly discover, and with plot-enabling military choke points at the surviving beacons that link multiple worlds. This is all background to the story, which is the ongoing war between Chaonia and the Phene Empire mixed with cutthroat political maneuvering between the great houses of the Chaonian Republic. This is where the heist aspects come in. Each house sends one representative to join the household of the Queen-Marshal and (more to the point for this story) another to join her heir. Sun has encouraged the individual and divergent talents of her Companions and their cee-cees (an unfortunate term that I suspect is short for Companion's Companion) and forged them into a good working team. A team that's about to be disrupted by the maneuverings of a rival house and the introduction of a new team member whom no one wants. A problem with writing tactical geniuses is that they often aren't good viewpoint characters. Sun's tight third-person chapters, which is a little less than half the book, advance the plot and provide analysis of the interpersonal dynamics of the characters, but aren't the strength of the story. That lies with the interwoven first-person sections that follow Persephone, an altogether more interesting character. Persephone is the scion of the house that is Sun's chief rival, but she has no interest in being part of that house or its maneuverings. When the story opens, she's a cadet in a military academy for recruits from the commoners, having run away from home, hidden her identity, and won a position through the open entrance exams. She of course doesn't stay there; her past catches up with her and she gets assigned to Sun, to a great deal of mutual suspicion. She also is assigned an impeccably dressed and stunningly beautiful cee-cee, Tiana, who has her own secrets and who was my favorite character in the book. Somewhat unusually for the space opera tradition, this is a book that knows that common people exist and have interesting lives. It's primarily focused on the ruling houses, but that focus is not exclusive and the rulers do not have a monopoly on competence. Elliott also avoids narrowing the political field too far; the Gatoi are separate from the three rival powers, and there are other groups with traditions older than the Chaonian Republic and their own agendas. Sun and her Companions are following a couple of political threads, but there is clearly more going on in this world than that single plot. This is exactly the kind of story I think of when I think space opera. It's not doing anything that original or groundbreaking, and it's not going to make any of my lists of great literature, but it's a fun romp with satisfyingly layered bits of lore, a large-scale setting with lots of plot potential, and (once we get through the confusing and somewhat tedious process of introducing rather too many characters in short succession) some great interpersonal dynamics. It's the kind of book in which the characters are in the middle of decisive military action in an interstellar war and are also near-teenagers competing for ratings in an ad hoc reality TV show, primarily as an excuse to create tactical distractions for Sun's latest scheme. The writing is okay but not great, and the first few chapters have some serious infodumping problems, but I thoroughly enjoyed the whole book and will pre-order the sequel. One Amazon review complained that Unconquerable Sun is not a space opera like Hyperion or Use of Weapons. That is entirely true, but if that's your standard for space opera, the world may be a disappointing place. This is a solid entry in a subgenre I love, with some great characters, sarcasm, competence porn, plenty of pages to keep turning, a few twists, and the promise of more to come. Recommended. Followed by the not-yet-published Furious Heaven. Rating: 7 out of 10

21 September 2020

Kees Cook: security things in Linux v5.7

Previously: v5.6 Linux v5.7 was released at the end of May. Here s my summary of various security things that caught my attention: arm64 kernel pointer authentication
While the ARMv8.3 CPU Pointer Authentication (PAC) feature landed for userspace already, Kristina Martsenko has now landed PAC support in kernel mode. The current implementation uses PACIASP which protects the saved stack pointer, similar to the existing CONFIG_STACKPROTECTOR feature, only faster. This also paves the way to sign and check pointers stored in the heap, as a way to defeat function pointer overwrites in those memory regions too. Since the behavior is different from the traditional stack protector, Amit Daniel Kachhap added an LKDTM test for PAC as well. BPF LSM
The kernel s Linux Security Module (LSM) API provide a way to write security modules that have traditionally implemented various Mandatory Access Control (MAC) systems like SELinux, AppArmor, etc. The LSM hooks are numerous and no one LSM uses them all, as some hooks are much more specialized (like those used by IMA, Yama, LoadPin, etc). There was not, however, any way to externally attach to these hooks (not even through a regular loadable kernel module) nor build fully dynamic security policy, until KP Singh landed the API for building LSM policy using BPF. With this, it is possible (for a privileged process) to write kernel LSM hooks in BPF, allowing for totally custom security policy (and reporting). execve() deadlock refactoring
There have been a number of long-standing races in the kernel s process launching code where ptrace could deadlock. Fixing these has been attempted several times over the last many years, but Eric W. Biederman and Ernd Edlinger decided to dive in, and successfully landed the a series of refactorings, splitting up the problematic locking and refactoring their uses to remove the deadlocks. While he was at it, Eric also extended the exec_id counter to 64 bits to avoid the possibility of the counter wrapping and allowing an attacker to send arbitrary signals to processes they normally shouldn t be able to. slub freelist obfuscation improvements
After Silvio Cesare observed some weaknesses in the implementation of CONFIG_SLAB_FREELIST_HARDENED s freelist pointer content obfuscation, I improved their bit diffusion, which makes attacks require significantly more memory content exposures to defeat the obfuscation. As part of the conversation, Vitaly Nikolenko pointed out that the freelist pointer s location made it relatively easy to target too (for either disclosures or overwrites), so I moved it away from the edge of the slab, making it harder to reach through small-sized overflows (which usually target the freelist pointer). As it turns out, there were a few assumptions in the kernel about the location of the freelist pointer, which had to also get cleaned up. RISCV page table dumping
Following v5.6 s generic page table dumping work, Zong Li landed the RISCV page dumping code. This means it s much easier to examine the kernel s page table layout when running a debug kernel (built with PTDUMP_DEBUGFS), visible in /sys/kernel/debug/kernel_page_tables. array index bounds checking
This is a pretty large area of work that touches a lot of overlapping elements (and history) in the Linux kernel. The short version is: C is bad at noticing when it uses an array index beyond the bounds of the declared array, and we need to fix that. For example, don t do this:
int foo[5];
...
foo[8] = bar;
The long version gets complicated by the evolution of flexible array structure members, so we ll pause for a moment and skim the surface of this topic. While things like CONFIG_FORTIFY_SOURCE try to catch these kinds of cases in the memcpy() and strcpy() family of functions, it doesn t catch it in open-coded array indexing, as seen in the code above. GCC has a warning (-Warray-bounds) for these cases, but it was disabled by Linus because of all the false positives seen due to fake flexible array members. Before flexible arrays were standardized, GNU C supported zero sized array members. And before that, C code would use a 1-element array. These were all designed so that some structure could be the header in front of some data blob that could be addressable through the last structure member:
/* 1-element array */
struct foo  
    ...
    char contents[1];
 ;
/* GNU C extension: 0-element array */
struct foo  
    ...
    char contents[0];
 ;
/* C standard: flexible array */
struct foo  
    ...
    char contents[];
 ;
instance = kmalloc(sizeof(struct foo) + content_size);
Converting all the zero- and one-element array members to flexible arrays is one of Gustavo A. R. Silva s goals, and hundreds of these changes started landing. Once fixed, -Warray-bounds can be re-enabled. Much more detail can be found in the kernel s deprecation docs. However, that will only catch the visible at compile time cases. For runtime checking, the Undefined Behavior Sanitizer has an option for adding runtime array bounds checking for catching things like this where the compiler cannot perform a static analysis of the index values:
int foo[5];
...
for (i = 0; i < some_argument; i++)  
    ...
    foo[i] = bar;
    ...
 
It was, however, not separate (via kernel Kconfig) until Elena Petrova and I split it out into CONFIG_UBSAN_BOUNDS, which is fast enough for production kernel use. With this enabled, it's now possible to instrument the kernel to catch these conditions, which seem to come up with some regularity in Wi-Fi and Bluetooth drivers for some reason. Since UBSAN (and the other Sanitizers) only WARN() by default, system owners need to set panic_on_warn=1 too if they want to defend against attacks targeting these kinds of flaws. Because of this, and to avoid bloating the kernel image with all the warning messages, I introduced CONFIG_UBSAN_TRAP which effectively turns these conditions into a BUG() without needing additional sysctl settings. Fixing "additive" snprintf() usage
A common idiom in C for building up strings is to use sprintf()'s return value to increment a pointer into a string, and build a string with more sprintf() calls:
/* safe if strlen(foo) + 1 < sizeof(string) */
wrote  = sprintf(string, "Foo: %s\n", foo);
/* overflows if strlen(foo) + strlen(bar) > sizeof(string) */
wrote += sprintf(string + wrote, "Bar: %s\n", bar);
/* writing way beyond the end of "string" now ... */
wrote += sprintf(string + wrote, "Baz: %s\n", baz);
The risk is that if these calls eventually walk off the end of the string buffer, it will start writing into other memory and create some bad situations. Switching these to snprintf() does not, however, make anything safer, since snprintf() returns how much it would have written:
/* safe, assuming available <= sizeof(string), and for this example
 * assume strlen(foo) < sizeof(string) */
wrote  = snprintf(string, available, "Foo: %s\n", foo);
/* if (strlen(bar) > available - wrote), this is still safe since the
 * write into "string" will be truncated, but now "wrote" has been
 * incremented by how much snprintf() *would* have written, so "wrote"
 * is now larger than "available". */
wrote += snprintf(string + wrote, available - wrote, "Bar: %s\n", bar);
/* string + wrote is beyond the end of string, and availabe - wrote wraps
 * around to a giant positive value, making the write effectively 
 * unbounded. */
wrote += snprintf(string + wrote, available - wrote, "Baz: %s\n", baz);
So while the first overflowing call would be safe, the next one would be targeting beyond the end of the array and the size calculation will have wrapped around to a giant limit. Replacing this idiom with scnprintf() solves the issue because it only reports what was actually written. To this end, Takashi Iwai has been landing a bunch scnprintf() fixes. That's it for now! Let me know if there is anything else you think I should mention here. Next up: Linux v5.8.

2020, Kees Cook. This work is licensed under a Creative Commons Attribution-ShareAlike 4.0 License.
CC BY-SA 4.0

Antoine Beaupr : PSA: Mailman used to harrass people

It seems that Mailman instances are being abused to harrass people with subscribe spam. If some random people complain to you that they "never wanted to subscribe to your mailing list", you may be a victim to that attack, even if you run the latest Mailman 2.

TL;DR: IKR! HOW DO I FIX THIS!? Make sure you have SUBSCRIBE_FORM_SECRET set in your mailman configuration:
SECRET=$(tr -dc 'A-Za-z0-9' < /dev/urandom   head -c 30)'
echo "SUBSCRIBE_FORM_SECRET = '$SECRET'" >> /etc/mailman/mm.cfg
This will add a magic token to all forms in the Mailman web forms that will force the attacker to at least get a token before asking for registration. There are, of course, other ways of performing the attack then, but it's more expensive than a single request for the attacker and keeps most of the junk out.

Other solutions I originally deployed a different fix, using referrer checks and an IP block list:
RewriteMap hosts-deny  txt:/etc/apache2/blocklist.txt
RewriteCond $ hosts-deny:% REMOTE_ADDR NOT-FOUND  !=NOT-FOUND [OR]
RewriteCond $ hosts-deny:% REMOTE_HOST NOT-FOUND  !=NOT-FOUND [OR]
RewriteCond % HTTP_REFERER  !^https://lists.torproject.org/$ [NC]
RewriteRule ^/cgi-bin/mailman/subscribe/ - [F]
# see also https://www.w3.org/TR/referrer-policy/#referrer-policy-origin
Header always set Referrer-Policy "origin"
I kept those restrictions in place because it keeps the spammers from even hitting the Mailman CGI, which is useful to preserve our server resources. But if "they" escalate with smarter crawlers, the block list will still be useful. You can use this query to extract the top 10 IP addresses used for subscription attempts:
awk '  print $NF  ' /var/log/mailman/subscribe   sort   uniq -c   sort -n   tail -10    awk '  print $2 " " $1  '
Note that this might include email-based registration, but in our logs those are extremely rare: only two in three weeks, out of over 73,000 requests. I also use this to keep an eye on the logs:
tail -f  /var/log/mailman/subscribe /var/log/apache2/lists.torproject.org-access.log   grep -v 'GET /pipermail/'
The server-side mitigations might also be useful if you happen to run an extremely old version of Mailman, that is pre-2.1.18, but it's now over 6 years old and part of every supported Debian release out there (all the way back to Debian 8 jessie).

Why does that attack work? Because Mailman 2 doesn't have CSRF tokens in its forms by default, anyone can send a POST request to /mailman/subscribe/LISTNAME to have Mailman send an email to the user. In the old "Internet is for nice people" universe, that wasn't a problem: all it does is ask the victim if they want to subscribe to LISTNAME. Innocuous, right? But in the brave, new, post-Eternal-September, "Internet is for stupid" universe, some assholes think it's a good idea to make a form that collects hundreds of mailing list URLs and spam them through an iframe. To see what that looks like, you can look at the rendered source code behind samedyfreeday.co.uk (not linking to avoid promoting it). That site does what is basically a distributed cross-site scripting attack against Mailman servers. Obviously, CSRF protection should be enabled by default in Mailman, but there you go. Hopefully this will help some folks... (The latest Mailman 3 release doesn't suffer from such idiotic defaults and ships with proper CSRF protection out of the box.)

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