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copies-rust: start recording overwrite as they happens...
copies-rust: start recording overwrite as they happens If a revision has information overwriting data from another revision, the overwriting revision is a descendant of the overwritten one. So we could warm the Oracle cache with such information to avoid potential future `is_ancestors` call. This provide us with a large speedup in the most expensive cases: Repo Case Source-Rev Dest-Rev # of revisions old time new time Difference Factor time per rev --------------------------------------------------------------------------------------------------------------------------------------------------------------- mozilla-try x00000_revs_x00000_added_x0000_copies 1b661134e2ca 1ae03d022d6d : 228985 revs, 41.113063 s, 36.001255 s, -5.111808 s, × 0.8757, 157 µs/rev mozilla-try x00000_revs_x00000_added_x000_copies 9b2a99adc05e 8e29777b48e6 : 382065 revs, 27.891612 s, 14.340641 s, -13.550971 s, × 0.5142, 37 µs/rev Full comparison below: Repo Case Source-Rev Dest-Rev # of revisions old time new time Difference Factor time per rev --------------------------------------------------------------------------------------------------------------------------------------------------------------- mercurial x_revs_x_added_0_copies ad6b123de1c7 39cfcef4f463 : 1 revs, 0.000042 s, 0.000042 s, +0.000000 s, × 1.0000, 42 µs/rev mercurial x_revs_x_added_x_copies 2b1c78674230 0c1d10351869 : 6 revs, 0.000114 s, 0.000109 s, -0.000005 s, × 0.9561, 18 µs/rev mercurial x000_revs_x000_added_x_copies 81f8ff2a9bf2 dd3267698d84 : 1032 revs, 0.004934 s, 0.004953 s, +0.000019 s, × 1.0039, 4 µs/rev pypy x_revs_x_added_0_copies aed021ee8ae8 099ed31b181b : 9 revs, 0.000195 s, 0.000237 s, +0.000042 s, × 1.2154, 26 µs/rev pypy x_revs_x000_added_0_copies 4aa4e1f8e19a 359343b9ac0e : 1 revs, 0.000050 s, 0.000050 s, +0.000000 s, × 1.0000, 50 µs/rev pypy x_revs_x_added_x_copies ac52eb7bbbb0 72e022663155 : 7 revs, 0.000113 s, 0.000113 s, +0.000000 s, × 1.0000, 16 µs/rev pypy x_revs_x00_added_x_copies c3b14617fbd7 ace7255d9a26 : 1 revs, 0.6f1f4a s, 0.6f1f4a s, +0.000000 s, × 1.0000, 322 µs/rev pypy x_revs_x000_added_x000_copies df6f7a526b60 a83dc6a2d56f : 6 revs, 0.010788 s, 0.010702 s, -0.000086 s, × 0.9920, 1783 µs/rev pypy x000_revs_xx00_added_0_copies 89a76aede314 2f22446ff07e : 4785 revs, 0.050880 s, 0.050504 s, -0.000376 s, × 0.9926, 10 µs/rev pypy x000_revs_x000_added_x_copies 8a3b5bfd266e 2c68e87c3efe : 6780 revs, 0.081760 s, 0.080159 s, -0.001601 s, × 0.9804, 11 µs/rev pypy x000_revs_x000_added_x000_copies 89a76aede314 7b3dda341c84 : 5441 revs, 0.061382 s, 0.060058 s, -0.001324 s, × 0.9784, 11 µs/rev pypy x0000_revs_x_added_0_copies d1defd0dc478 c9cb1334cc78 : 43645 revs, 0.585802 s, 0.536950 s, -0.048852 s, × 0.9166, 12 µs/rev pypy x0000_revs_xx000_added_0_copies bf2c629d0071 4ffed77c095c : 2 revs, 0.012803 s, 0.012868 s, +0.000065 s, × 1.0051, 6434 µs/rev pypy x0000_revs_xx000_added_x000_copies 08ea3258278e d9fa043f30c0 : 11316 revs, 0.113558 s, 0.112806 s, -0.000752 s, × 0.9934, 9 µs/rev netbeans x_revs_x_added_0_copies fb0955ffcbcd a01e9239f9e7 : 2 revs, 0.000085 s, 0.000084 s, -0.000001 s, × 0.9882, 42 µs/rev netbeans x_revs_x000_added_0_copies 6f360122949f 20eb231cc7d0 : 2 revs, 0.000106 s, 0.000106 s, +0.000000 s, × 1.0000, 53 µs/rev netbeans x_revs_x_added_x_copies 1ada3faf6fb6 5a39d12eecf4 : 3 revs, 0.000175 s, 0.000174 s, -0.000001 s, × 0.9943, 58 µs/rev netbeans x_revs_x00_added_x_copies 35be93ba1e2c 9eec5e90c05f : 9 revs, 0.000721 s, 0.000726 s, +0.000005 s, × 1.0069, 80 µs/rev netbeans x000_revs_xx00_added_0_copies eac3045b4fdd 51d4ae7f1290 : 1421 revs, 0.010127 s, 0.010105 s, -0.000022 s, × 0.9978, 7 µs/rev netbeans x000_revs_x000_added_x_copies e2063d266acd 6081d72689dc : 1533 revs, 0.015616 s, 0.015748 s, +0.000132 s, × 1.0085, 10 µs/rev netbeans x000_revs_x000_added_x000_copies ff453e9fee32 411350406ec2 : 5750 revs, 0.061341 s, 0.060357 s, -0.000984 s, × 0.9840, 10 µs/rev netbeans x0000_revs_xx000_added_x000_copies 588c2d1ced70 1aad62e59ddd : 66949 revs, 0.542214 s, 0.499356 s, -0.042858 s, × 0.9210, 7 µs/rev mozilla-central x_revs_x_added_0_copies 3697f962bb7b 7015fcdd43a2 : 2 revs, 0.000089 s, 0.000092 s, +0.000003 s, × 1.0337, 46 µs/rev mozilla-central x_revs_x000_added_0_copies dd390860c6c9 40d0c5bed75d : 8 revs, 0.000279 s, 0.000279 s, +0.000000 s, × 1.0000, 34 µs/rev mozilla-central x_revs_x_added_x_copies 8d198483ae3b 14207ffc2b2f : 9 revs, 0.000184 s, 0.000186 s, +0.000002 s, × 1.0109, 20 µs/rev mozilla-central x_revs_x00_added_x_copies 98cbc58cc6bc 446a150332c3 : 7 revs, 0.000661 s, 0.000660 s, -0.000001 s, × 0.9985, 94 µs/rev mozilla-central x_revs_x000_added_x000_copies 3c684b4b8f68 0a5e72d1b479 : 3 revs, 0.003377 s, 0.003372 s, -0.000005 s, × 0.9985, 1124 µs/rev mozilla-central x_revs_x0000_added_x0000_copies effb563bb7e5 c07a39dc4e80 : 6 revs, 0.070508 s, 0.070294 s, -0.000214 s, × 0.9970, 11715 µs/rev mozilla-central x000_revs_xx00_added_0_copies 6100d773079a 04a55431795e : 1593 revs, 0.006576 s, 0.006545 s, -0.000031 s, × 0.9953, 4 µs/rev mozilla-central x000_revs_x000_added_x_copies 9f17a6fc04f9 2d37b966abed : 41 revs, 0.004809 s, 0.004998 s, +0.000189 s, × 1.0393, 121 µs/rev mozilla-central x000_revs_x000_added_x000_copies 7c97034feb78 4407bd0c6330 : 7839 revs, 0.064872 s, 0.063348 s, -0.001524 s, × 0.9765, 8 µs/rev mozilla-central x0000_revs_xx000_added_0_copies 9eec5917337d 67118cc6dcad : 615 revs, 0.026142 s, 0.026154 s, +0.000012 s, × 1.0005, 42 µs/rev mozilla-central x0000_revs_xx000_added_x000_copies f78c615a656c 96a38b690156 : 30263 revs, 0.203956 s, 0.199063 s, -0.004893 s, × 0.9760, 6 µs/rev mozilla-central x00000_revs_x0000_added_x0000_copies 6832ae71433c 4c222a1d9a00 : 153721 revs, 1.763853 s, 1.277320 s, -0.486533 s, × 0.7242, 8 µs/rev mozilla-central x00000_revs_x00000_added_x000_copies 76caed42cf7c 1daa622bbe42 : 204976 revs, 2.609761 s, 1.698794 s, -0.910967 s, × 0.6509, 8 µs/rev mozilla-try x_revs_x_added_0_copies aaf6dde0deb8 9790f499805a : 2 revs, 0.000847 s, 0.000842 s, -0.000005 s, × 0.9941, 421 µs/rev mozilla-try x_revs_x000_added_0_copies d8d0222927b4 5bb8ce8c7450 : 2 revs, 0.000867 s, 0.000865 s, -0.000002 s, × 0.9977, 432 µs/rev mozilla-try x_revs_x_added_x_copies 092fcca11bdb 936255a0384a : 4 revs, 0.000161 s, 0.000160 s, -0.000001 s, × 0.9938, 40 µs/rev mozilla-try x_revs_x00_added_x_copies b53d2fadbdb5 017afae788ec : 2 revs, 0.001131 s, 0.001122 s, -0.000009 s, × 0.9920, 561 µs/rev mozilla-try x_revs_x000_added_x000_copies 20408ad61ce5 6f0ee96e21ad : 1 revs, 0.033114 s, 0.032743 s, -0.000371 s, × 0.9888, 32743 µs/rev mozilla-try x_revs_x0000_added_x0000_copies effb563bb7e5 c07a39dc4e80 : 6 revs, 0.071092 s, 0.071529 s, +0.000437 s, × 1.0061, 11921 µs/rev mozilla-try x000_revs_xx00_added_0_copies 6100d773079a 04a55431795e : 1593 revs, 0.006554 s, 0.006593 s, +0.000039 s, × 1.0060, 4 µs/rev mozilla-try x000_revs_x000_added_x_copies 9f17a6fc04f9 2d37b966abed : 41 revs, 0.005160 s, 0.005311 s, +0.000151 s, × 1.0293, 129 µs/rev mozilla-try x000_revs_x000_added_x000_copies 1346fd0130e4 4c65cbdabc1f : 6657 revs, 0.065063 s, 0.063063 s, -0.002000 s, × 0.9693, 9 µs/rev mozilla-try x0000_revs_x_added_0_copies 63519bfd42ee a36a2a865d92 : 40314 revs, 0.297118 s, 0.312363 s, +0.015245 s, × 1.0513, 7 µs/rev mozilla-try x0000_revs_x_added_x_copies 9fe69ff0762d bcabf2a78927 : 38690 revs, 0.284002 s, 0.283106 s, -0.000896 s, × 0.9968, 7 µs/rev mozilla-try x0000_revs_xx000_added_x_copies 156f6e2674f2 4d0f2c178e66 : 8598 revs, 0.086311 s, 0.083817 s, -0.002494 s, × 0.9711, 9 µs/rev mozilla-try x0000_revs_xx000_added_0_copies 9eec5917337d 67118cc6dcad : 615 revs, 0.026738 s, 0.026516 s, -0.000222 s, × 0.9917, 43 µs/rev mozilla-try x0000_revs_xx000_added_x000_copies 89294cd501d9 7ccb2fc7ccb5 : 97052 revs, 1.514270 s, 1.304865 s, -0.209405 s, × 0.8617, 13 µs/rev mozilla-try x0000_revs_x0000_added_x0000_copies e928c65095ed e951f4ad123a : 52031 revs, 0.735875 s, 0.681088 s, -0.054787 s, × 0.9255, 13 µs/rev mozilla-try x00000_revs_x_added_0_copies 6a320851d377 1ebb79acd503 : 363753 revs, 4.843329 s, 4.454320 s, -0.389009 s, × 0.9197, 12 µs/rev mozilla-try x00000_revs_x00000_added_0_copies dc8a3ca7010e d16fde900c9c : 34414 revs, 0.591752 s, 0.567913 s, -0.023839 s, × 0.9597, 16 µs/rev mozilla-try x00000_revs_x_added_x_copies 5173c4b6f97c 95d83ee7242d : 362229 revs, 4.760563 s, 4.547043 s, -0.213520 s, × 0.9551, 12 µs/rev mozilla-try x00000_revs_x000_added_x_copies 9126823d0e9c ca82787bb23c : 359344 revs, 4.751942 s, 4.378579 s, -0.373363 s, × 0.9214, 12 µs/rev mozilla-try x00000_revs_x0000_added_x0000_copies 8d3fafa80d4b eb884023b810 : 192665 revs, 2.605014 s, 1.703622 s, -0.901392 s, × 0.6540, 8 µs/rev mozilla-try x00000_revs_x00000_added_x0000_copies 1b661134e2ca 1ae03d022d6d : 228985 revs, 41.113063 s, 36.001255 s, -5.111808 s, × 0.8757, 157 µs/rev mozilla-try x00000_revs_x00000_added_x000_copies 9b2a99adc05e 8e29777b48e6 : 382065 revs, 27.891612 s, 14.340641 s, -13.550971 s, × 0.5142, 37 µs/rev Differential Revision: https://phab.mercurial-scm.org/D9497

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README.rst
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Gregory Szorc
automation: perform tasks on remote machines...
r42191 ====================
Mercurial Automation
====================
This directory contains code and utilities for building and testing Mercurial
on remote machines.
The ``automation.py`` Script
============================
``automation.py`` is an executable Python script (requires Python 3.5+)
that serves as a driver to common automation tasks.
When executed, the script will *bootstrap* a virtualenv in
``<source-root>/build/venv-automation`` then re-execute itself using
that virtualenv. So there is no need for the caller to have a virtualenv
explicitly activated. This virtualenv will be populated with various
dependencies (as defined by the ``requirements.txt`` file).
To see what you can do with this script, simply run it::
$ ./automation.py
Local State
===========
By default, local state required to interact with remote servers is stored
in the ``~/.hgautomation`` directory.
We attempt to limit persistent state to this directory. Even when
performing tasks that may have side-effects, we try to limit those
side-effects so they don't impact the local system. e.g. when we SSH
into a remote machine, we create a temporary directory for the SSH
config so the user's known hosts file isn't updated.
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r43327 Try Server
==========
There exists a *Try Server* which allows automation to run against
an arbitrary Mercurial changeset and displays results via the web.
.. note::
The *Try Server* is still experimental infrastructure.
To use the *Try Server*::
$ ./automation.py try
With a custom AWS profile::
$ AWS_PROFILE=hg contrib/automation/automation.py try
By default, the ``.`` revision is submitted. **Any uncommitted changes
are not submitted.**
To switch which revision is used::
$ ./automation.py try -r abcdef
Access to the *Try Server* requires access to a special AWS account.
This account is currently run by Gregory Szorc. Here is the procedure
for accessing the *Try Server*:
1. Email Gregory Szorc at gregory.szorc@gmail.com and request a
username. This username will be stored in the public domain.
2. Wait for an email reply containing your temporary AWS credentials.
3. Log in at https://gregoryszorc-hg.signin.aws.amazon.com/console
and set a new, secure password.
4. Go to https://console.aws.amazon.com/iam/home?region=us-west-2#/security_credentials
5. Under ``Access keys for CLI, SDK, & API access``, click the
``Create access key`` button.
6. See the ``AWS Integration`` section for instructions on
configuring your local client to use the generated credentials.
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r42191 AWS Integration
===============
Various automation tasks integrate with AWS to provide access to
resources such as EC2 instances for generic compute.
This obviously requires an AWS account and credentials to work.
We use the ``boto3`` library for interacting with AWS APIs. We do not employ
any special functionality for telling ``boto3`` where to find AWS credentials. See
https://boto3.amazonaws.com/v1/documentation/api/latest/guide/configuration.html
for how ``boto3`` works. Once you have configured your environment such
that ``boto3`` can find credentials, interaction with AWS should *just work*.
Gregory Szorc
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r43326 To configure ``boto3``, you can use the ``aws configure`` command to
write out configuration files. (The ``aws`` command is typically provided
by an ``awscli`` package available in your package manager, including
``pip``.) Alternatively, you can write out files in ``~/.aws/`` directly.
e.g.::
# ~/.aws/config
[default]
region = us-west-2
Gregory Szorc
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r42191
Gregory Szorc
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r43326 # ~/.aws/credentials
[default]
aws_access_key_id = XXXX
aws_secret_access_key = YYYY
If you have multiple AWS accounts, you can name the profile something
different from ``default``. e.g. ``hg``. You can influence which profile
is used by ``boto3`` by setting the ``AWS_PROFILE`` environment variable.
e.g. ``AWS_PROFILE=hg``.
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r42191
Resource Management
-------------------
Depending on the task being performed, various AWS services will be accessed.
This of course requires AWS credentials with permissions to access these
services.
The following AWS services can be accessed by automation tasks:
* EC2
* IAM
* Simple Systems Manager (SSM)
Various resources will also be created as part of performing various tasks.
This also requires various permissions.
The following AWS resources can be created by automation tasks:
* EC2 key pairs
* EC2 security groups
* EC2 instances
* IAM roles and instance profiles
* SSM command invocations
When possible, we prefix resource names with ``hg-`` so they can easily
be identified as belonging to Mercurial.
.. important::
We currently assume that AWS accounts utilized by *us* are single
tenancy. Attempts to have discrete users of ``automation.py`` (including
sharing credentials across machines) using the same AWS account can result
in them interfering with each other and things breaking.
Cost of Operation
-----------------
``automation.py`` tries to be frugal with regards to utilization of remote
resources. Persistent remote resources are minimized in order to keep costs
in check. For example, EC2 instances are often ephemeral and only live as long
as the operation being performed.
Under normal operation, recurring costs are limited to:
* Storage costs for AMI / EBS snapshots. This should be just a few pennies
per month.
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r42471 When running EC2 instances, you'll be billed accordingly. Default instance
types vary by operation. We try to be respectful of your money when choosing
defaults. e.g. for Windows instances which are billed per hour, we use e.g.
``t3.medium`` instances, which cost ~$0.07 per hour. For operations that
scale well to many CPUs like running Linux tests, we may use a more powerful
instance like ``c5.9xlarge``. However, since Linux instances are billed
per second and the cost of running an e.g. ``c5.9xlarge`` for half the time
of a ``c5.4xlarge`` is roughly the same, the choice is justified.
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r42191
.. note::
When running Windows EC2 instances, AWS bills at the full hourly cost, even
if the instance doesn't run for a full hour (per-second billing doesn't
apply to Windows AMIs).
Managing Remote Resources
-------------------------
Occassionally, there may be an error purging a temporary resource. Or you
may wish to forcefully purge remote state. Commands can be invoked to manually
purge remote resources.
To terminate all EC2 instances that we manage::
$ automation.py terminate-ec2-instances
To purge all EC2 resources that we manage::
$ automation.py purge-ec2-resources
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r42471
Remote Machine Interfaces
=========================
The code that connects to a remote machine and executes things is
theoretically machine agnostic as long as the remote machine conforms to
an *interface*. In other words, to perform actions like running tests
remotely or triggering packaging, it shouldn't matter if the remote machine
is an EC2 instance, a virtual machine, etc. This section attempts to document
the interface that remote machines need to provide in order to be valid
*targets* for remote execution. These interfaces are often not ideal nor
the most flexible. Instead, they have often evolved as the requirements of
our automation code have evolved.
Linux
-----
Remote Linux machines expose an SSH server on port 22. The SSH server
must allow the ``hg`` user to authenticate using the SSH key generated by
the automation code. The ``hg`` user should be part of the ``hg`` group
and it should have ``sudo`` access without password prompting.
The SSH channel must support SFTP to facilitate transferring files from
client to server.
``/bin/bash`` must be executable and point to a bash shell executable.
The ``/hgdev`` directory must exist and all its content owned by ``hg::hg``.
The ``/hgdev/pyenv`` directory should contain an installation of
``pyenv``. Various Python distributions should be installed. The exact
versions shouldn't matter. ``pyenv global`` should have been run so
``/hgdev/pyenv/shims/`` is populated with redirector scripts that point
to the appropriate Python executable.
The ``/hgdev/venv-bootstrap`` directory must contain a virtualenv
with Mercurial installed. The ``/hgdev/venv-bootstrap/bin/hg`` executable
is referenced by various scripts and the client.
The ``/hgdev/src`` directory MUST contain a clone of the Mercurial
source code. The state of the working directory is not important.
In order to run tests, the ``/hgwork`` directory will be created.
This may require running various ``mkfs.*`` executables and ``mount``
to provision a new filesystem. This will require elevated privileges
via ``sudo``.
Various dependencies to run the Mercurial test harness are also required.
Documenting them is beyond the scope of this document. Various tests
also require other optional dependencies and missing dependencies will
be printed by the test runner when a test is skipped.
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r43177
Releasing Windows Artifacts
===========================
The `automation.py` script can be used to automate the release of Windows
artifacts::
$ ./automation.py build-all-windows-packages --revision 5.1.1
$ ./automation.py publish-windows-artifacts 5.1.1
The first command will launch an EC2 instance to build all Windows packages
and copy them into the `dist` directory relative to the repository root. The
second command will then attempt to upload these files to PyPI (via `twine`)
and to `mercurial-scm.org` (via SSH).
Uploading to PyPI requires a PyPI account with write access to the `Mercurial`
package. You can skip PyPI uploading by passing `--no-pypi`.
Uploading to `mercurial-scm.org` requires an SSH account on that server
with `windows` group membership and for the SSH key for that account to be the
default SSH key (e.g. `~/.ssh/id_rsa`) or in a running SSH agent. You can
skip `mercurial-scm.org` uploading by passing `--no-mercurial-scm-org`.