author | huffman |
Tue, 13 Jan 2009 14:08:24 -0800 | |
changeset 29479 | be8a15ffc511 |
parent 28918 | eda3d9976ec7 |
child 29481 | 3e8420c1124a |
permissions | -rw-r--r-- |
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Important notes on Mercurial repository access for Isabelle.
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Important notes on Mercurial repository access for Isabelle |
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=========================================================== |
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Preamble |
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-------- |
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Mercurial http://www.selenic.com/mercurial belongs to a new generation |
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of source code management systems, following the paradigm of |
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"distributed version control". Compared to the old centralized model |
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of CVS or SVN, this gives considerable more power and freedom in |
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organizing the flow of changes, both between individual developers and |
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designated pull/push areas that are shared with others. |
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More power for the user also means more responsibility! Due to its |
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decentralized nature, changesets that have been published once, |
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e.g. via "push" to a shared repository that is visible on the net, |
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cannot be easily retracted from the public again. Regular Mercurial |
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operations are strictly monotonic, where changset transactions are |
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only added, but never deleted. There are special tools to manipulate |
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individual repositories via non-monotonic actions, but this does not |
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yet retrieve any changesets that have escaped into the public by |
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accident. |
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Only global operations like "pull" and "push" fall into this critical |
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category. Note that "incoming" / "outgoing" allow to inspect |
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changesets before exchanging them globally. Anything else in |
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Mercurial is local to the user's repository clone (including "commit", |
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"update", "merge" etc.) and is in fact much simpler and safer to use |
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than the corresponding operations of CVS or SVN. |
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Initial configuration |
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===================== |
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Always use Mercurial version 1.0 or later, such as 1.0.1 or 1.0.2. |
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The old 0.9.x versions do not work in a multi-user environment with |
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shared file spaces. |
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The official Isabelle repository can be cloned like this: |
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hg clone http://isabelle.in.tum.de/repos/isabelle |
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This will create a local directory "isabelle", unless an alternative |
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name is specified. The full repository meta-data and history of |
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changes is in isabelle/.hg; local configuration for this clone can be |
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added to isabelle/.hg/hgrc, but note that hgrc files are never copied |
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by another clone operation! |
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There is also $HOME/.hgrc for per-user Mercurial configuration. The |
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initial configuration should include at least an entry to identify |
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yourself. For example, something like this in /home/wenzelm/.hgrc: |
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[ui] |
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username = wenzelm |
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Of course, the user identity can be also configured in |
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isabelle/.hg/hgrc on per-repository basis. Failing to specify the |
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username correctly makes the system invent funny machine names that |
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may persist indefinitely in the public flow of changesets. |
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In principle, user names can be chosen freely, but for longterm |
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committers of the Isabelle repository the obvious choice is to keep |
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with the old CVS naming scheme. |
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There are other useful configuration to go into $HOME/.hgrc, |
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e.g. defaults for common commands: |
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[defaults] |
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log = -l 10 |
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The next example shows how to install some Mercurial extension: |
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[extensions] |
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hgext.graphlog = |
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Now the additional glog command will be available. |
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See also the fine documentation for further details, especially the |
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book http://hgbook.red-bean.com/ |
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Shared pull/push access |
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======================= |
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The entry point http://isabelle.in.tum.de/repos/isabelle is world |
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readable, both via plain web browsing and the hg client as described |
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above. Anybody can produce a clone, change it arbitrarily, and then |
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use regular mechanisms of Mercurial to report changes upstream, say |
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via e-mail to someone with write access to that file space. It is |
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also quite easy to publish changed clones again on the web, using the |
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adhoc command "hg serve -v", or the hgweb.cgi or hgwebdir.cgi scripts |
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that are included in the Mercurial distribution. |
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The downstream/upstream mode of operation is quite common in the |
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distributed version control community, and works well for occasional |
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changes produced by anybody out there. Of course, upstream |
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maintainers need to review and moderate changes being proposed, before |
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pushing anything onto the official Isabelle repository at TUM. |
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Write access to the Isabelle repository requires an account at TUM, |
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with properly configured ssh access to the local machines |
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(e.g. macbroy20, atbroy100). You also need to be a member of the |
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"isabelle" Unix group. |
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Sharing a locally modified clone then works as follows, using your |
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user name instead of "wenzelm": |
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hg out ssh://wenzelm@atbroy100//home/isabelle-repository/repos/isabelle |
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In fact, the "out" or "outgoing" command performs only a dry run: it |
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displays the changesets that would get published. An actual "push", |
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with a lasting effect on the Isabelle repository, works like this: |
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hg push ssh://wenzelm@atbroy100//home/isabelle-repository/repos/isabelle |
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Default paths for push and pull can be configure in isabelle/.hg/hgrc, |
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for example: |
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[paths] |
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default = ssh://wenzelm@atbroy100//home/isabelle-repository/repos/isabelle |
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Now "hg pull" or "hg push" will use that shared file space, unless a |
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different URL is specified explicitly. |
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When cloning a repository, the default path is set to the initial |
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source URL. So we could have cloned via that ssh URL in the first |
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place, to get exactly to the same point: |
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hg clone ssh://wenzelm@atbroy100//home/isabelle-repository/repos/isabelle |
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Content discipline |
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================== |
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Old-style centralized version control is occasionally compared to "a |
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library where everybody scribbles into the books". Or seen the other |
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way round, the centralized model discourages individual |
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experimentation (with local branches etc.), because everything is |
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forced to happen on a shared file space. With Mercurial, arbitrary |
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variations on local clones are no problem, but care is required again |
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when publishing changes eventually. |
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The following principles should be kept in mind when producing |
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changesets that might become public at some point. |
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* The author of changes should be properly identified, using |
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ui/username configuration as described above. |
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While Mercurial also provides means for signed changesets, we want |
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to keep things simple and trust that users specify their identity |
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correctly. |
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* The history of sources is an integral part of the sources |
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themselves. This means that private experiments and branches |
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should not be published, unless they are really meant to become |
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universally available. |
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Note that exchanging local experiments with some other users can |
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be done directly on peer-to-peer basis, without affecting the |
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central pull/push area. |
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* Log messages are an integral part of the history of sources. |
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Other users will have to look there eventually, to understand why |
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things have been done in a certain way at some point. |
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Mercurial provides nice web presentation of incoming changes with |
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a digest of log entries; this also includes RSS/Atom news feeds. |
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Users should be aware that others will actually read what is |
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written into log messages. |
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176 |
|
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The usual changelog presentation style for the Isabelle repository |
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admits log entries that consist of several lines, but without the |
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special headline that is used in Mercurial projects elsewhere. |
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Since some display styles strip newlines from text, it is |
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advisable to separate lines via punctuation, and not rely on |
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two-dimensional presentation too much. |
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|
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Building Isabelle from the repository version |
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============================================= |
|
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||
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Compared to a proper distribution or development snapshot, a |
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repository version of Isabelle lacks textual version identifiers in |
190 |
some sources and scripts, and various components produced by |
|
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Admin/build are missing. After applying that script with suitable |
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arguments, the regular user instructions for building and running |
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Isabelle from sources apply. |
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Needless to say, the results from the build process must not be added |
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to the repository! |
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||
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Makarius 30-Nov-2008 |