Study 000626:

ACRONYM: HH_Flare+AR_180x152v2

Updated	by M. Whillock,	MSSL, 20220708.
Copied from study id 0000461, increased	exposure time by 50%.

This study is to hunt for various flow structures in solar flares.
It can also be used as a study for active regions.

Target: Active region / Flare

Type: scanning raster
Field of view: 180"x152"
Exposure time: 14.0 s
Slit: 2"
Step size: 6"
Raster Duration: 8m42s
Data volume: 3.6 Mbits (JPEG75 - default), 4.4 Mbits (JPEG85)
             See note in instruction to planners section

Lines:
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O V     : detection of TR response at the impulsive phase
Fe X    : hunting of reconnection inflow
Fe XII  : hunting of reconnection inflow
Fe XIV  : study of normal coronal loops with density sensitive pairs
Fe XV   : study of flare loops in a cooling phase
Fe XVI  : study of flare loops in a cooling phase
Fe XVII : study of flare-loop heating and reconnection outflow
Ca XVII : study of reconnection outflow
Fe XXIII: study of loop-top hot region and reconnection outflow
Fe XXIV : study of loop-top hot region and reconnection outflow

The non-thermal velocity component in solar flares is studied by
combinations of Fe XXIII ad Fe XXIV.

Pointing:
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Active region including those with the potential for flaring

Instruction to planners:
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1) Center the raster on an expected site in an active region.
2) When flare hunting, adjust the raster repeat for a maximum
  run-time possible, accounting for the TM constraint.

** Note** : The default compression is JPEG75. For a short time scale runs, the
compression parameter should be changed to JPEG85.

Warning:
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None