| Version 2 (modified by , 10 years ago) ( diff ) |
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PSNSC_NCU requirements and notes (draft) --
NCU observations -- processing needs to be finished by early morning for MOPS to use
- obs_mode NCU (new end Oct 2016 possibly) -- 8 fields/targets (chunks?), 8 dithers for 6 hrs (64 exposures per field?), 45s exptime over 4 nights? (not sure right yet)
- offset only dither (no rotation like MD)
- WSdiff and published to normal MOPS datastore location
- chip->warp normal stdscience pantasks as with xSS products
- WSdiff runs in ~ippmops/stdscience_ws to make uncompressed WSdiffs (like FSS) -- larger volume, may need more nodes -- must be uncompressed for MOPS stamps since large data volume
- comment string -- needs to be worked on
Processing products -- czar needs to make sure all faults and issues are cleared daily (early morning) for NCU.* products
- chip-cam-warp -- NCU.nightlyscience -- nightly
- warp-stack diffims -- NCU.WS.nightlyscience -- nightly
- publishing of WSdiffs -- (need datastore location to use from MOPS) -- nightly
- nightly stack -- NCU.nightlyscience -- nightly, manually done to avoid any poor images
- stack-stack diffims -- NCU.SS.nightlyscience -- nightly, likely automatic possible once manual stacks made
- stamps -- TBD
Cleanup --
- chip -- 1 day?
- warp -- 2 days (no specific requirement?)
- WSdiff -- 1 day? uncompressed so likely will need to limit and just do updates for stamps
- publishing WSdiff catalog bundles --
- pstamp -- manual cleanup like other ps_ud_%
Tasks to do --
- verify w-band stacks okay along ecliptic for opposition end October
- check processing rate/nodes for WSdiffs
- MOPS interested in SSdiff?
- publishing location for WSdiff by MOPS preference -- IPP-MOPS-TEST or IPP-MOPS-WS -- unique set so likely normal location
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