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Operating Systems Solaris problem in finding a hardware problem Post 302232863 by avronius on Friday 5th of September 2008 10:39:50 AM
Old 09-05-2008
When I run into a hardware problem that I've not experienced before, I generally run SUN vts, then Explorer, then check sunsolve and google. If the host is still under a service contract, I call SUN.

Install VTS - see what it says. Be prepared to let it run (impact system performance - so don't serve anything during testing) for a few hours. Don't be surprised if it doesn't find a problem - this can run for a couple of days before it hits on anything.

If you have the ability to monitor the power that is coming into the host - something that shows spikes (+/-) in power - that's a likely cause of this sort of error.

Then, on a separate host:

- start a terminal session.
- type: script /somewhere/date.problem_hostname.capture
- telnet into the console on the problem host

Ideally, you'll write a small shell script to run prtdiag -v and dmesg every 3 minutes or so. If you have utilities that you like, include them in the script. The next time that the server crashes, let it complete it's power cycle and then see if any new and interesting errors arise. Compare your prtdiag outputs over the course of the hours prior to the crash. See if there are drastic changes in temperature, etc.

Good luck!
 

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mlib_VideoColorUYV444int_to_ARGBint(3MLIB)		    mediaLib Library Functions			mlib_VideoColorUYV444int_to_ARGBint(3MLIB)

NAME
mlib_VideoColorUYV444int_to_ARGBint - color convert UYV interleaved to ARGB interleaved SYNOPSIS
cc [ flag... ] file... -lmlib [ library... ] #include <mlib.h> void mlib_VideoColorUYV444int_to_ARGBint(mlib_u32 *ARGB, const mlib_u8 *UYV, const mlib_u8 *A_array, mlib_u8 A_const, mlib_s32 w, mlib_s32 h, mlib_s32 dlb, mlib_s32 slb, mlib_s32 alb); DESCRIPTION
The UYV pixel stream is converted into an ARGB pixel stream. All pixel components are 8-bit unsigned integers. All buffers have dimensions w and h. The alpha values for this function work in the following fashion: o If A_array pointer is not NULL, the values are taken from there. It has to have the same dimensions as the Y buffer. o If A_array pointer is NULL, the alpha values for every pixel are set to A_const. The following equation is used: |R| |1.1644 0.0000 1.5966| [|Y| | 16.0000|] |G| = |1.1644 -0.3920 -0.8132| * [|U| - |128.0000|] |B| |1.1644 2.0184 0.0000| [|V| |128.0000|] PARAMETERS
The function takes the following arguments: ARGB Pointer to output buffer. UYV Pointer to input buffer. A_array Array of alpha values. A_const Constant alpha value. w Image width in pixels. h Image height in lines. dlb Linebytes for output buffer. slb Linebytes for input buffer. alb Linebytes for alpha buffer. RETURN VALUES
None. ATTRIBUTES
See attributes(5) for descriptions of the following attributes: +-----------------------------+-----------------------------+ | ATTRIBUTE TYPE | ATTRIBUTE VALUE | +-----------------------------+-----------------------------+ |Interface Stability |Evolving | +-----------------------------+-----------------------------+ |MT-Level |MT-Safe | +-----------------------------+-----------------------------+ SEE ALSO
mlib_VideoColorYUV420seq_to_ARGBint(3MLIB), mlib_VideoColorYUV411seq_to_ARGBint(3MLIB), mlib_VideoColorYUV422seq_to_ARGBint(3MLIB), mlib_VideoColorYUV444seq_to_ARGBint(3MLIB), mlib_VideoColorYUV420seq_to_ABGRint(3MLIB), mlib_VideoColorYUV411seq_to_ABGRint(3MLIB), mlib_VideoColorYUV422seq_to_ABGRint(3MLIB), mlib_VideoColorYUV444seq_to_ABGRint(3MLIB), mlib_VideoColorYUYV422int_to_ARGBint(3MLIB), mlib_VideoColorYUV444int_to_ARGBint(3MLIB), mlib_VideoColorYUYV422int_to_ABGRint(3MLIB), mlib_VideoColorYUV444int_to_ABGRint(3MLIB), mlib_VideoColorUYVY422int_to_ARGBint(3MLIB), mlib_VideoColorUYVY422int_to_ABGRint(3MLIB), mlib_VideoColorUYV444int_to_ABGRint(3MLIB), attributes(5) SunOS 5.10 10 Nov 2004 mlib_VideoColorUYV444int_to_ARGBint(3MLIB)
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