Study 000304:

ACRONYM: SK_CH_DIAG_320x384

This study performes a large scan for coronal holes
with low temperature lines (log T < 6.2). 
It is designed for polar monitoring campaign with
SOT/SP measurement of magnetic fields.

TARGET        : Coronal hole
EXPOSURE TIME : 50s
RASTER        : Scanning
SLIT          : 1"
STEP_SIZE     : 1"
FOV           : 320"x384"
SPECTRAL WIND.: 12
DATA COMP.    : JPEG90
RASTER DURATON: 4h50m
DATA VOLUME   : 150 Mbits
LINES         : Fe VIII, Fe X, Fe XI, Fe XII, Fe XIII,
                He II, O V, Mg VI, Mg VII, Si VII, Si X

POINTING: 

Polar coronal hole with fixed pointing.
Make sure to cover SOT FOV and the solar limb.

INSTRUCTION TO PLANNERS:

Start this study at the beginning of SAA free period (roughly 10-15UT)
The later part may coincide with a short SAA.

WARNING:

Large data volume (150 Mbits), duration 4h 50m. Avoid SAAs as much
as possible (SAA degrade data compression factors and mutilate the data)