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Changes between Initial Version and Version 1 of PSNSC_NCU


Ignore:
Timestamp:
Oct 11, 2016, 11:08:19 AM (10 years ago)
Author:
Mark Huber
Comment:

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  • PSNSC_NCU

    v1 v1  
     1PSNSC_NCU requirements and notes (draft) --
     2
     3
     4NCU observations -- processing needs to be finished by early morning for MOPS to use
     5 * obs_mode NCU (new Oct 2016) -- 8 pointings, 16 dithers for 6 hrs, 45s exptime over 4 nights?
     6  * MD-like dither (rotation) plus small offsets?
     7  * WSdiff only and published to normal MOPS datastore location
     8 * chip->warp normal stdscience pantasks as with xSS products
     9 * WSdiff runs in ~ippmops/stdscience_ws to make uncompressed WSdiffs (like FSS) -- larger volume, may need more nodes
     10
     11
     12Processing products -- czar needs to make sure all faults and issues are cleared daily (early morning) for NCU.* products
     13 * chip-cam-warp -- NCU.nightlyscience -- nightly
     14 * warp-stack diffims -- NCU.WS.nightlyscience -- nightly
     15 * publishing of WSdiffs -- -- nightly
     16 * nightly stack -- NCU.nightlyscience -- nightly
     17 * stack-stack diffims -- NCU.SS.nightlyscience -- nightly
     18 * stamps -- TBD
     19
     20
     21Cleanup --
     22 * chip -- 1 days
     23 * warp -- 2 days (no specific requirement?)
     24 * WSdiff -- 1 days -- if disk space issue, can reduce this to 2 days as long as warps uncleaned the update time is minimal
     25 * publishing WSdiff catalog bundles -- Bill has script doing?
     26 * pstamp -- manual cleanup like other ps_ud_%
     27
     28
     29Tasks to do --
     30 * verify w-band stacks okay along ecliptic for opposition around October
     31 * check processing rate/nodes for WSdiffs
     32 * MOPS interested in SSdiff --
     33 * publishing location for WSdiff -- IPP-MOPS-TEST or IPP-MOPS-WS