Study: 000670

ACRONYM:  CMAP_002


This study is another version of CMAP_001. 

This study uses a 16 arcsec sparse EIS raster to observe the Sun with fewer slit positions than the standard full raster. The goal is to test whether this faster, lower-telemetry observing strategy still captures enough spatial information for reliable full-Sun calibration. It covers a very large field of view (480"x512") in a relatively short time (18 mins) using the 2" slit and 16" steps. The idea is to fit the raster between SAAs. 

TARGET:           Active Region
EXPOSURE TIME:    30s
RASTER:           Scanning
SLIT:             2"
FOV:              480"x512" 
RASTER DURATION:  17 min 40 sec 
VOLUME:           55 Mbits
RATE:             52 kbits/s
COMPRESSION:      JPEG90        

The line-list is unchanged.

Pointing:
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As in HOP 130 for a full Sun scan, or any large active region, or AR/CH complex.

Warning:
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None.