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+ <H1>[Mageia-discuss] Suggestions for the ISO</H1>
+ <B>Olivier Thauvin</B>
+ <A HREF="mailto:mageia-discuss%40mageia.org?Subject=Re%3A%20%5BMageia-discuss%5D%20Suggestions%20for%20the%20ISO&In-Reply-To=%3C20101105110504.GK7479%40virgo.home.nanardon.zarb.org%3E"
+ TITLE="[Mageia-discuss] Suggestions for the ISO">nanardon at nanardon.zarb.org
+ </A><BR>
+ <I>Fri Nov 5 12:05:05 CET 2010</I>
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+<PRE>* andre999 (<A HREF="https://www.mageia.org/mailman/listinfo/mageia-discuss">andr55 at laposte.net</A>) wrote:
+&gt;&gt;<i>
+</I>&gt;&gt;<i> * andre999 (<A HREF="https://www.mageia.org/mailman/listinfo/mageia-discuss">andr55 at laposte.net</A>) wrote:
+</I>&gt;&gt;<i>
+</I>&gt;&gt;&gt;<i> Donald Stewart a &#233;crit :
+</I>&gt;&gt;&gt;<i>
+</I>&gt;&gt;<i> The problem of delta rpm is the work need to generated alls delta and
+</I>&gt;&gt;<i> the space need on mirrors to host everything.
+</I>&gt;&gt;<i> We must provide delta for each version to the next one:
+</I>&gt;&gt;<i>
+</I>&gt;&gt;<i> - main foo-1
+</I>&gt;&gt;<i> - upd foo-2 D: 1-&gt;2
+</I>&gt;&gt;<i> foo-3 D: 2-&gt;3 and 1-&gt;3 ?
+</I>&gt;&gt;<i> foo-4 D: 3-&gt;4 and 1-&gt;4, 2-&gt;4 ?
+</I>&gt;&gt;<i>
+</I>&gt;<i> I would make all delta updates relative to the distro release, i.e.
+</I>&gt;<i> - main = foo-1
+</I>&gt;<i> - upd_full = foo-2, foo-3, foo-4, etc
+</I>&gt;<i> - upd_delta = foo-1&gt;2, foo-1&gt;3, foo-1&gt;4, etc
+</I>&gt;<i> without foo 2&gt;3, 2&gt;4, 3&gt;4
+</I>&gt;<i> (so half as many, with 3 updates.)
+</I>&gt;<i>
+</I>&gt;<i> Note that the idea is to retain full update packages, the delta updates
+</I>&gt;<i> being a file-by-file diff of contained files (probably in their own
+</I>&gt;<i> repository).
+</I>
+That mean people udapting frequently their distribution will not profit
+of delta rpm, then downloading the full rpm as soon they made one
+update.
+
+Delta rpm will become not so usefull then, except for new install.
+
+&gt;&gt;<i> etc...
+</I>&gt;&gt;<i> What if delta 1-&gt;4 is bigger than the package itself ? and for 2-&gt;4 ?
+</I>&gt;&gt;<i>
+</I>&gt;<i> Highly improbable, as I conceive it.
+</I>&gt;<i> If foo-1.rpm contains files fooa foob fooc food, and only foob changes
+</I>&gt;<i> to foob',
+</I>&gt;<i> then full foo-2.rpm contains files fooa foob' fooc food
+</I>&gt;<i> and delta foo-2d.rpm contains only file foob', with the info that this
+</I>&gt;<i> replaces foob.
+</I>&gt;<i> And of course with this model, there is no 2-&gt;4.
+</I>
+Changes between 1-&gt;4 will probably be bigger than 2-&gt;4 as there is more
+changes between them.
+
+&gt;&gt;<i> Delta rpm is hard to manage (any volunteer to write the tools to manage
+</I>&gt;&gt;<i> this ?) and as bonus, I am not sure it is still compatible with our
+</I>&gt;&gt;<i> current rpm...
+</I>&gt;&gt;<i>
+</I>&gt;<i> To create a delta rpm, one only needs the new full version (or the
+</I>&gt;<i> proposed contents), and a script which automatically includes the new
+</I>&gt;<i> files with the references to those replaced.
+</I>&gt;<i> I'm not trying to say it is simple to write - especially since I
+</I>&gt;<i> understand that the current tools are written in Perl - which has a
+</I>&gt;<i> syntax which I barely understand.
+</I>&gt;<i> But I'd be interested in contributing to my ability.
+</I>
+Nothing deny you to start to work on this and then submit you code. It's
+what I did for the mirrors tools :)
+
+We'll see when BS and SVN will be ready to merge it if it works.
+
+&gt;&gt;<i> Just think we don't have an infinite space on mirror. Even the sound
+</I>&gt;&gt;<i> good, please try to estimated the cost it can be per release.
+</I>&gt;&gt;<i>
+</I>&gt;<i> I agree it would take more space on mirrors, but as full updates take
+</I>&gt;<i> much less space than the release,
+</I>&gt;<i> delta updates would take considerably less space the full updates.
+</I>&gt;<i> Also, the lower bandwidth to download for users would also benefit the
+</I>&gt;<i> mirrors.
+</I>
+You know, most of our rpms are less than 10MB, but du -sh is clear, the
+distribution is around 35GB per arch.
+
+Nothing is really big on mirrors, but the results is.
+
+--
+
+Olivier Thauvin
+CNRS - LATMOS
+&#9814; &#9816; &#9815; &#9813; &#9812; &#9815; &#9816; &#9814;
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