Wed, 12 Sep 2018 09:58:23 -0700 exchangev2: start to implement pull with wire protocol v2
Gregory Szorc <gregory.szorc@gmail.com> [Wed, 12 Sep 2018 09:58:23 -0700] rev 39629
exchangev2: start to implement pull with wire protocol v2 Wire protocol version 2 will take a substantially different approach to exchange than version 1 (at least as far as pulling is concerned). This commit establishes a new exchangev2 module for holding code related to exchange using wire protocol v2. I could have added things to the existing exchange module. But it is already quite big. And doing things inline isn't in question because the existing code is already littered with conditional code for various states of support for the existing wire protocol as it evolved over 10+ years. A new module gives us a chance to make a clean break. This approach does mean we'll end up writing some duplicate code. And there's a significant chance we'll miss functionality as code is ported. The plan is to eventually add #testcase's to existing tests so the new wire protocol is tested side-by-side with the existing one. This will hopefully tease out any features that weren't ported properly. But before we get there, we need to build up support for the new exchange methods. Our journey towards implementing a new exchange begins with pulling. And pulling begins with discovery. The discovery code added to exchangev2 is heavily drawn from the following functions: * exchange._pulldiscoverychangegroup * discovery.findcommonincoming For now, we build on top of existing discovery mechanisms. The new wire protocol should be capable of doing things more efficiently. But I'd rather defer on this problem. To foster the transition, we invent a fake capability on the HTTPv2 peer and have the main pull code in exchange.py call into exchangev2 when the new wire protocol is being used. Differential Revision: https://phab.mercurial-scm.org/D4480
Tue, 21 Aug 2018 15:33:11 -0700 httppeer: expose capabilities for each command
Gregory Szorc <gregory.szorc@gmail.com> [Tue, 21 Aug 2018 15:33:11 -0700] rev 39628
httppeer: expose capabilities for each command This will help code using peers to sniff out exactly what servers support. Differential Revision: https://phab.mercurial-scm.org/D4436
Thu, 13 Sep 2018 22:48:27 -0700 narrow: intersect provided matcher with narrowmatcher in `hg diff`
spectral <spectral@google.com> [Thu, 13 Sep 2018 22:48:27 -0700] rev 39627
narrow: intersect provided matcher with narrowmatcher in `hg diff` This provides significant speedups when running diff, and no change in behavior that I'm aware of (or that the tests found). I tested with a repo that I started using narrow in after it was created and attempted to run `hg diff -c .` and similar commands in it on a commit that had files not in the narrowspec. Timing numbers below, using a similar setup as my previous commits. before=9db85644, m-u is mozilla-unified at eb39298e432d (flatmanifest) and 0553b7f29eaf (treemanifest). l-d-r is a repo simulating a situation I've encountered where there's one directory with 30k+ subdirectories. N means narrow, T means treemanifest. The narrowspec is pretty small when in use, and importantly the narrowspec is applied *after* doing the initial checkout (without narrowing), so all of these files exist in the filesystem, which is not normally the case if someone has been using narrow for the entire life of the clone. Anything less than a 5% difference in performance is most likely noise. diff --git: repo | N | T | before (mean +- stdev) | after (mean +- stdev) | % of before ------+---+---+------------------------+-----------------------+------------ m-u | | | 1.292 s +- 0.009 s | 1.295 s +- 0.010 s | 100.2% m-u | | x | 1.296 s +- 0.042 s | 1.299 s +- 0.026 s | 100.2% m-u | x | | 1.292 s +- 0.010 s | 1.297 s +- 0.021 s | 100.4% m-u | x | x | 84.2 ms +- 1.2 ms | 83.6 ms +- 0.2 ms | 99.3% l-d-r | | | 188.7 ms +- 2.7 ms | 188.8 ms +- 2.0 ms | 100.1% l-d-r | | x | 189.9 ms +- 1.5 ms | 189.4 ms +- 1.2 ms | 99.7% l-d-r | x | | 97.1 ms +- 1.0 ms | 87.1 ms +- 1.0 ms | 89.7% <-- l-d-r | x | x | 96.9 ms +- 0.8 ms | 87.2 ms +- 0.7 ms | 90.0% <-- diff -c . --git: repo | N | T | before (mean +- stdev) | after (mean +- stdev) | % of before ------+---+---+------------------------+-----------------------+------------ m-u | | | 231.6 ms +- 3.1 ms | 228.9 ms +- 1.6 ms | 98.8% m-u | | x | 150.5 ms +- 1.7 ms | 150.7 ms +- 1.4 ms | 100.1% m-u | x | | 233.7 ms +- 2.4 ms | 232.2 ms +- 1.9 ms | 99.4% m-u | x | x | 126.1 ms +- 1.2 ms | 126.8 ms +- 1.2 ms | 100.6% l-d-r | | | 82.1 ms +- 2.0 ms | 81.8 ms +- 1.4 ms | 99.6% l-d-r | | x | 3.732 s +- 0.020 s | 3.746 s +- 0.027 s | 100.4% l-d-r | x | | 83.1 ms +- 0.8 ms | 107.6 ms +- 2.4 ms | 129.5% <-- l-d-r | x | x | 758.2 ms +- 38.8 ms | 188.5 ms +- 1.8 ms | 24.9% <-- rebase -r . --keep -d .^^: repo | N | T | before (mean +- stdev) | after (mean +- stdev) | % of before ------+---+---+------------------------+-----------------------+------------ m-u | | | 5.532 s +- 0.087 s | 5.496 s +- 0.016 s | 99.3% m-u | | x | 5.554 s +- 0.061 s | 5.532 s +- 0.013 s | 99.6% m-u | x | | 5.602 s +- 0.134 s | 5.508 s +- 0.035 s | 98.3% m-u | x | x | 582.2 ms +- 15.2 ms | 572.9 ms +- 12.0 ms | 98.4% l-d-r | | | 629.5 ms +- 12.3 ms | 622.5 ms +- 7.3 ms | 98.9% l-d-r | | x | 6.173 s +- 0.062 s | 6.185 s +- 0.076 s | 100.2% l-d-r | x | | 274.5 ms +- 10.0 ms | 272.1 ms +- 6.2 ms | 99.1% l-d-r | x | x | 4.835 s +- 0.056 s | 4.826 s +- 0.034 s | 99.8% status --change . --copies: repo | N | T | before (mean +- stdev) | after (mean +- stdev) | % of before ------+---+---+------------------------+-----------------------+------------ m-u | | | 214.4 ms +- 1.4 ms | 212.2 ms +- 1.7 ms | 99.0% m-u | | x | 130.9 ms +- 1.2 ms | 131.7 ms +- 1.1 ms | 100.6% m-u | x | | 215.0 ms +- 2.1 ms | 214.9 ms +- 2.7 ms | 100.0% m-u | x | x | 109.5 ms +- 2.3 ms | 107.8 ms +- 0.9 ms | 98.4% l-d-r | | | 79.6 ms +- 0.9 ms | 79.8 ms +- 1.6 ms | 100.3% l-d-r | | x | 3.799 s +- 0.037 s | 3.928 s +- 0.021 s | 103.4% <--? l-d-r | x | | 82.7 ms +- 0.7 ms | 83.2 ms +- 1.0 ms | 100.6% l-d-r | x | x | 746.8 ms +- 6.1 ms | 739.0 ms +- 4.2 ms | 99.0% status --copies: repo | N | T | before (mean +- stdev) | after (mean +- stdev) | % of before ------+---+---+------------------------+-----------------------+------------ m-u | | | 1.884 s +- 0.012 s | 1.885 s +- 0.013 s | 100.1% m-u | | x | 1.897 s +- 0.027 s | 1.909 s +- 0.077 s | 100.6% m-u | x | | 1.886 s +- 0.021 s | 1.891 s +- 0.030 s | 100.3% m-u | x | x | 92.0 ms +- 0.7 ms | 92.4 ms +- 0.4 ms | 100.4% l-d-r | | | 570.3 ms +- 18.7 ms | 552.2 ms +- 4.5 ms | 96.8% l-d-r | | x | 568.9 ms +- 16.1 ms | 567.2 ms +- 11.9 ms | 99.7% l-d-r | x | | 171.1 ms +- 2.5 ms | 170.4 ms +- 1.2 ms | 99.6% l-d-r | x | x | 171.6 ms +- 3.4 ms | 171.5 ms +- 1.7 ms | 99.9% update $rev^; ~/src/hg/hg{hg}/hg update $rev: repo | N | T | before (mean +- stdev) | after (mean +- stdev) | % of before ------+---+---+------------------------+-----------------------+------------ m-u | | | 3.107 s +- 0.017 s | 3.116 s +- 0.012 s | 100.3% m-u | | x | 2.943 s +- 0.010 s | 2.945 s +- 0.019 s | 100.1% m-u | x | | 3.116 s +- 0.033 s | 3.118 s +- 0.027 s | 100.1% m-u | x | x | 318.5 ms +- 2.7 ms | 320.8 ms +- 4.8 ms | 100.7% l-d-r | | | 428.9 ms +- 4.4 ms | 429.5 ms +- 4.0 ms | 100.1% l-d-r | | x | 9.593 s +- 0.081 s | 9.869 s +- 0.043 s | 102.9% l-d-r | x | | 253.2 ms +- 3.6 ms | 254.0 ms +- 2.8 ms | 100.3% l-d-r | x | x | 1.613 s +- 0.009 s | 1.630 s +- 0.017 s | 101.1% Differential Revision: https://phab.mercurial-scm.org/D4587
Sat, 01 Sep 2018 12:15:02 +0900 identify: change {parents} to a list of nodes (BC)
Yuya Nishihara <yuya@tcha.org> [Sat, 01 Sep 2018 12:15:02 +0900] rev 39626
identify: change {parents} to a list of nodes (BC) This is a part of the name unification. {parents} is a list of nodes in "hg log -Tjson" output. Since {rev} can be computed from (repo, node) pair, we no longer need to put it to provide {rev} to user templates. https://www.mercurial-scm.org/wiki/GenericTemplatingPlan#Dictionary
Sat, 01 Sep 2018 12:09:22 +0900 identify: use fm.hexfunc thoroughly
Yuya Nishihara <yuya@tcha.org> [Sat, 01 Sep 2018 12:09:22 +0900] rev 39625
identify: use fm.hexfunc thoroughly This fixes the length of {id} in JSON and template outputs.
Sat, 01 Sep 2018 15:52:18 +0900 formatter: replace contexthint() with demand loading of ctx object
Yuya Nishihara <yuya@tcha.org> [Sat, 01 Sep 2018 15:52:18 +0900] rev 39624
formatter: replace contexthint() with demand loading of ctx object And pass in repo instead to resolve ctx from (repo, node) pair.
Thu, 07 Jun 2018 21:48:11 +0900 formatter: populate ctx from repo and node value
Yuya Nishihara <yuya@tcha.org> [Thu, 07 Jun 2018 21:48:11 +0900] rev 39623
formatter: populate ctx from repo and node value This will basically replace the fm.contexthint() API. I originally thought this would be too complicated, and I wrote 8399438bc7ef "formatter: provide hint of context keys required by template" because of that. However, I had to add a similar mechanism for fctx templates, and the overall machinery became way simpler than my original patch. The test output slightly changed as {author} is no longer available in the {manifest} context, which isn't the point this test targeted on.
Fri, 14 Sep 2018 18:18:46 -0400 merge with stable
Augie Fackler <augie@google.com> [Fri, 14 Sep 2018 18:18:46 -0400] rev 39622
merge with stable
Sat, 15 Sep 2018 00:37:20 +0300 py3: call hgweb.hgweb() with bytes values
Pulkit Goyal <pulkit@yandex-team.ru> [Sat, 15 Sep 2018 00:37:20 +0300] rev 39621
py3: call hgweb.hgweb() with bytes values # skip-blame because just b'' prefixes I believe this should fix some tests. Differential Revision: https://phab.mercurial-scm.org/D4594
Sat, 15 Sep 2018 00:24:05 +0300 py3: use '%d' for integers instead of '%s'
Pulkit Goyal <pulkit@yandex-team.ru> [Sat, 15 Sep 2018 00:24:05 +0300] rev 39620
py3: use '%d' for integers instead of '%s' Differential Revision: https://phab.mercurial-scm.org/D4593
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