Study 000467:

ACRONYM: hh_flare_sas

This study is to investigate the time variability of various flow
structures in solar flares.
It can also be used for studies of active regions.

Target: Active region / Flare
Type: sit and stare
Field of view: 2"x152"
Exposure time: 9.0 s
Slit: 2"
Step size: 0
Raster Duration: 49m5s
Data volume: 35.8Mbits

Lines:
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 and 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 slit on an expected site in an active region.
2) When flare hunting, repeat the sequence for a maximum run-time
possible, accounting for the telemetry constraint.

Note:

The default compression is JPEG85. For a short-time run, the compression
parameter should be changed to JPEG95.

Warning:
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None