Study 000600:

ACRONYM: DHB_007_v2

This is a new version of DHB_007 with an increased exposure time to improve the signals
in weak lines. To maintain the duration the field of view in the solar-X direction is
reduced by half.

The study itself is for multiple use, with spectral lines chosen to measure densities,
compute an emission measure distribution to obtain temperatures, and use that
distribution to compute abundances. It covers a reasonable field of view 
(246"x512") in a relatively short time (70 mins) using the 2" slit and 4"
steps. The idea is to fit the raster between SAAs. 

TARGET:           Active Region
EXPOSURE TIME:    60s
RASTER:           Scanning
SLIT:             2"
FOV:              246"x512" 
RASTER DURATION:  1h8m 
VOLUME:           114 Mbits
RATE:             28 kbits/s
COMPRESSION:      JPEG90        

The line-list is similar to #218 with Fe XXIV 255 replaced by Si X 261.

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.