Study 000486:

ACRONYM: HH_Flare_162x152_R

This study is intended to be used as XRT flare trigger Response (Hence _R). See the WARNING below.

Target: Flare

Type: scanning raster
Field of view: 162"x152"
Exposure time: 3.0 s
Slit: 2"
Step size: 3"
Raster Duration: 4m 59s
Raster repeat: 6
Study duration: 28m
Compression: JPEG85
Total Data volume: 55.0 Mbits

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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Autonomous

Instruction to planners:
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This study to be used as an XRT FT response study. It runs with a fixed
number of rasters repeat (6) and JPEG98. Total study run time is 28m and
produces 55 Mbits (volume).

Warning:
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Only to be used when XRT flare trigger is tested. Consult Khalid, David Brooks or Harry Warren
before use.