Study 000655:

ACRONYM:  DHB_007_v5

m.whillock@ucl.ac.uk: New version copied from DHB_007. Mg V replaced in line list by
Fe X 257 for coronal magnetic field measurements.

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 very large field of view 
(494"x512") in a relatively short time (70 mins) using the 2" slit and 6"
steps. The idea is to fit the raster between SAAs. 

TARGET:           Active Region
EXPOSURE TIME:    30s
RASTER:           Scanning
SLIT:             2"
FOV:              494"x512" 
RASTER DURATION:  1h8m59s 
VOLUME:           224 Mbits
RATE:             54 kbits/s
COMPRESSION:      JPEG90        

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

Pointing:
---------

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

Warning:
-------

None.