Hmm, I'm not sure why that original thread devolved into a flame war. Odd. FWIW, Bill's "dd" solution is a valid method of backing up a partition, but there are some important notes.
Firstly, the filesystem must be quiescant; at best umounted, otherwise mounted read-only (as per Bill's examples), worst case mounted read/write but with no activity. Any writes to a filesystem being copied in this way can result in a corrupted backup. There is an important consequence to this: your root filesystem is not a good candidate for dd backups
Secondaly, 'dd' style backups may not be as small as other types, since they copy the whole partition - even unused space - is copied.
Being aware of those two points, "dd" is a pretty simple backup solution.
To restore a dd backup, you simply need to do the reverse.
1) ensure the partition is UNMOUNTED.
2) ensure the partition is the SAME SIZE (or bigger) than the original backup
3) do the "dd" in reverse:
ssh user@host "dd if=ubda2.img" | dd of=/dev/ubda2
4) fsck /dev/ubda2 (just for safety)
5) mount the filesystem
Make sure you get the "if" and "of" options the right way round
For what it's worth, if you plan on doing 'dd' style backups, and can afford "down time" then I would create a second OS image in some spare disk space, which has access to your original partitions (but doesn't mount them). Then you can boot into this image and "dd" your data with full confidence that the filesystems are quiescent (and can also backup your root disk safely!). In the event of a catastrophe, you can boot the alternate image again, and restore your data (as described above), including the root disk.
If you can not afford down time, then I'd recommend doing "dump" backups, since these are designed to handle hot filesystems (mounted read/write).
Personally, I use 'dd' backups to generate "gold images" of a distribution that may be rolled out to a bunch of identical machines. Especially with Solaris this is a lot quicker than an fresh install! Sun finally picked up on this and did something similar with "flash archives", which are essentially a cpio with wrappers, but in Solaris 2.5 and 2.6 days the "dd" image was a great solution
Hope this helps,