From: "Paweł Brodacki" <pawel.brodacki@googlemail.com>
To: linux-btrfs@vger.kernel.org
Subject: Fwd: What to do about subvolumes?
Date: Fri, 3 Dec 2010 14:47:44 +0100 [thread overview]
Message-ID: <AANLkTi=5vyGqdoFPC=c5yf-g_A8uLvi4txvWm4iq65bK@mail.gmail.com> (raw)
In-Reply-To: <AANLkTinBzpoCnci+1a=0pjXbAdQ7mzpdr2k8GOo7HUc8@mail.gmail.com>
2010/12/2 David Pottage <david@electric-spoon.com>:
>
> Therefore I think it is a bad idea if potentially different files on =
btrfs
> can have the same inode number. It will break all sorts of tools.
>
> Instead of maintaining a big complicated reference count of used inod=
e
> numbers, could btrfs use bit masks to create a the userland visible i=
node
> number from the subvolume id and the real internal inode number. Some=
thing
> like:
>
> userland_inode =3D ( volume_id << 48 ) & internal_inode;
>
> Please forgive me if this is impossible, or if that C snippet is
> syntactically incorrect. I am not a filesystem or kernel developer, a=
nd I
> have not coded in C for many years.
>
> --
> David Pottage
>
Expanding on the idea: what about a pool of IDs for subvolumes and
inode numbers inside a subvolume having the subvolume ID as a prefix?
It gives each inode a unique number, doesn't require cheating the
userland and is less costly than keeping reference count for each
inode. The obvious downside that I can see is limitation on number of
subvolumes that it would be possible to create. It also lowers the
maximum number of inodes in a filesystem (because of bits taken up by
subvolume ID). I expect there are also less-than obvious downsides.
Just an idea by a kernel and FS ignorant.
--
Pawe=C5=82 Brodacki
--
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next prev parent reply other threads:[~2010-12-03 13:47 UTC|newest]
Thread overview: 66+ messages / expand[flat|nested] mbox.gz Atom feed top
2010-12-01 14:21 What to do about subvolumes? Josef Bacik
2010-12-01 14:50 ` Mike Hommey
2010-12-01 14:51 ` C Anthony Risinger
2010-12-01 16:01 ` Chris Mason
2010-12-01 16:03 ` C Anthony Risinger
2010-12-01 16:13 ` Chris Mason
2010-12-01 16:31 ` Mike Hommey
2010-12-09 19:53 ` Martin Steigerwald
2010-12-01 16:00 ` Chris Mason
2010-12-01 16:38 ` Hugo Mills
2010-12-01 16:48 ` Gordan Bobic
2010-12-01 16:52 ` Mike Hommey
2010-12-01 16:52 ` C Anthony Risinger
2010-12-01 17:38 ` Josef Bacik
2010-12-01 19:35 ` Hugo Mills
2010-12-01 20:24 ` Freddie Cash
2010-12-01 21:28 ` Hugo Mills
2010-12-01 23:32 ` Freddie Cash
2010-12-02 4:46 ` Mike Fedyk
2010-12-01 18:33 ` Goffredo Baroncelli
2010-12-01 18:36 ` Josef Bacik
2010-12-01 18:48 ` C Anthony Risinger
2010-12-01 18:52 ` C Anthony Risinger
2010-12-01 19:08 ` Goffredo Baroncelli
2010-12-01 19:44 ` J. Bruce Fields
2010-12-01 19:54 ` Josef Bacik
2010-12-01 20:00 ` J. Bruce Fields
2010-12-01 20:09 ` Josef Bacik
2010-12-01 20:16 ` J. Bruce Fields
2010-12-02 1:52 ` Michael Vrable
2010-12-03 20:53 ` J. Bruce Fields
2010-12-01 20:03 ` Jeff Layton
2010-12-01 20:46 ` Goffredo Baroncelli
2010-12-01 21:06 ` Jeff Layton
2010-12-02 9:26 ` Arne Jansen
2010-12-02 9:49 ` Arne Jansen
2010-12-02 16:11 ` Chris Mason
2010-12-02 17:14 ` David Pottage
[not found] ` <AANLkTinBzpoCnci+1a=0pjXbAdQ7mzpdr2k8GOo7HUc8@mail.gmail.com>
2010-12-03 13:47 ` Paweł Brodacki [this message]
2010-12-03 20:56 ` J. Bruce Fields
2010-12-03 2:43 ` Phillip Susi
2011-01-31 2:40 ` Ian Kent
2010-12-03 4:25 ` Chris Ball
2010-12-03 14:00 ` Josef Bacik
2010-12-03 21:45 ` Josef Bacik
2010-12-03 22:16 ` J. Bruce Fields
2010-12-03 22:27 ` Dave Chinner
2010-12-03 22:29 ` Chris Mason
2010-12-03 22:45 ` J. Bruce Fields
2010-12-03 23:01 ` Andreas Dilger
2010-12-06 16:48 ` J. Bruce Fields
2010-12-08 6:39 ` Andreas Dilger
2010-12-08 23:07 ` Neil Brown
2010-12-09 4:41 ` Andreas Dilger
2010-12-09 15:19 ` J. Bruce Fields
2010-12-07 16:52 ` hch
2010-12-07 20:45 ` J. Bruce Fields
2010-12-07 16:51 ` Christoph Hellwig
2010-12-07 17:02 ` Trond Myklebust
2010-12-08 17:16 ` Andreas Dilger
2010-12-08 17:27 ` J. Bruce Fields
2010-12-08 21:18 ` Andreas Dilger
2010-12-04 21:58 ` Mike Fedyk
2010-12-06 14:27 ` Josef Bacik
2011-01-31 2:56 ` Ian Kent
2010-12-07 16:48 ` Christoph Hellwig
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