Study 000485:

ACRONYM: HH_Flare_162x152

This study is to hunt for various flow structures in solar flares.
It is (not) suitable for active regions.

Target: Flare

Type: scanning raster
Field of view: 162"x152"
Exposure time: 3.0 s
Slit: 2"
Step size: 3"
Raster Duration: 4m59s
Data volume: 7.0 Mbits (JPEG75 - default)

Lines:
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Fe VIII : response of transition region
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) Adjust the raster repeat for a maximum run-time possible,
   accounting for the TM constraint.

Warning:
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None