|
|
Sponsored Content
Operating Systems
Solaris
Removing Disk from SVM
Post 302263329 by kumarmani on Monday 1st of December 2008 10:23:40 AM
12-01-2008
|
|
10 More Discussions You Might Find Interesting
1. Solaris
I dont even know what raid level this is, but its raid 5 mirrored from the looks of it.
I have a failed disk (t12) within this mirror. What is the best way to replace this disk? 2 things concern me, isn't there a command to prepare the disk for a hot swap? and what should i do with the... (3 Replies)
Discussion started by: BG_JrAdmin
3 Replies
2. Solaris
Hello,
Can someone advise the proper procedure for replacing a mirrored disk in SVM. I have checked the docs and various websites but the procedure seems to vary. This is what I would do...
1. Remove the db replicas from the bad disk.
2. Detach it from the mirror
3. Clear it with... (4 Replies)
Discussion started by: Actuator
4 Replies
3. Solaris
Hi all,
we have an existing system that was configured using just one of the (two) internal disks. I want to mirror the disk using SVM, but have realised there is no free slice for creating the metadb's. Is there a workaround I can use for this?
In the past we have always kept slice 7 free -... (8 Replies)
Discussion started by: badoshi
8 Replies
4. Solaris
Hi Gurus, I've got an issue here:
(1) Hardware: Sun NetraT1, (2) OS: Solaris 10, (3) SVM
metastat shows /var having 12 GB. df shows /var having 4 GB. Real space for /var is about 4 GB since I can't move a big file to it. How is 8 GB space missing? Does /var/run swap need to account? Can I... (5 Replies)
Discussion started by: aixlover
5 Replies
5. Solaris
Dear All,
Please help me to configure root mirroring using SVM in Solaris 9.
Thanks and Regards,
Lakkireddy BR (3 Replies)
Discussion started by: lbreddy
3 Replies
6. Solaris
The following is the summarry:-
1) Four disks in server ie (c1t0d0. c1t1d0, c1t2d0, c1t3d0). c1t2d0 is the disk to be replaced.
c1t0d0 and c1t2d0 are mirrors.
c1t1d0 and c1t3d0 are mirrors.
Metadb to be deleted is in c1t2d0s7
a) Mirror d35 has 2 submirrors d38 and d39
d38 is a stripe... (0 Replies)
Discussion started by: aji1729
0 Replies
7. Solaris
I tried doing rootdisk mirroring in my local host , i added a new Ide disk in my system
and copied the prtvtoc from root disk to the newly added disk, and then when i tried to add database replicas on both the disks, it was added for boot disk but for the newly added disk i gave the error, which... (6 Replies)
Discussion started by: Laxxi
6 Replies
8. UNIX for Advanced & Expert Users
We have two node cluster with OS disk mirrored under SVM. There is slight disk problem on one of the mirror disk causing cluster to panic.
Failure of one mirror disk causing VCS to panic the node. Why VCS is not able to write /var filesystem, as one of the disk is healthy.
... (1 Reply)
Discussion started by: amlanroy
1 Replies
9. Solaris
Hi All
BAsed on the below I would like to verifu two things
(1) The udnerlying mirroris for '/mnt' na dit onlcy contaisne 1 sub-mirror, with one sliceon is one disk and hence, data loss on the mount point (the mount point, '/mnt' is backed up)
(2) the Procedure for renewal
# df -kh /mnt... (2 Replies)
Discussion started by: stevie_velvet
2 Replies
10. Solaris
Hi
Please can you help me on replacing or removing a faulty disk drive on a SUN NETRA X4250server with 4 internal drives only.
the format comand show me the following:
format
Searching for disks...done
AVAILABLE DISK SELECTIONS:
0. c0t0d0 <drive type unknown>
... (9 Replies)
Discussion started by: fretagi
9 Replies
LEARN ABOUT DEBIAN
celeste_standalone
CELESTE_STANDALONE(1) HUGIN CELESTE_STANDALONE(1) NAME
celeste_standalone - Cloud identification SYNOPSIS
celeste_standalone [options] image1 image2 [..] DESCRIPTION
Celeste has been trained using Support vector machine techniques to identify clouds in photos and remove control points from these areas. celeste_standalone is a command-line tool with all the same functionality as Celeste in hugin. Simple usage is to just 'clean' an existing project file: celeste_standalone -i project.pto -o project.pto OPTIONS
-i <filename> Input Hugin PTO file. Control points over SVM threshold will be removed before being written to the output file. If -m is set to 1, images in the file will be also be masked. -o <filename> Output Hugin PTO file. Default: '<filename>_celeste.pto' -d <filename> SVM model file. Default: 'data/celeste.model' -s <int> Maximum dimension for re-sized image prior to processing. A higher value will increase the resolution of the mask but is significantly slower. Default: 800 -t <float> SVM threshold. Raise this value to remove fewer control points, lower it to remove more. Range 0 to 1. Default: 0.5 -m <1|0> Create masks when processing Hugin PTO file. Default: 0 -f <string> Mask file format. Options are PNG, JPEG, BMP, GIF and TIFF. Default: PNG -r <1|0> Filter radius. 0 = large (more accurate), 1 = small (higher resolution mask, slower, less accurate). Default: 0 -h Print usage. AUTHORS
Written by Tim Nugent. "Version: 2011.4.0" 2011-12-02 CELESTE_STANDALONE(1)