Study 000498:

ACRONYM: PRY_flare_1

This study is intended to take spectra of flare kernels that appear
during the rise phase of a flare. The parameters have been chosen
based on lessons learnt from the data-set analyzed by Young et
al. (2012, arXiv:1212.4388).

Duration: 2min
Slit: 1"
Raster size: 40"x120"
Exposure time: 10.4s
Data volume: 1.3 MB
Data rate: 7.2 kB/s

Pointing:
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The pointing should be chosen carefully. Flare kernels do not appear
in sunspots, but can appear nearby. They will be close to the neutral
line in a region that is magnetically complex.

Instruction to planner:
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A context raster (PRY_slot_context_v3) should be run before and
after the sequence of PRY_flare_1 rasters.

Use raster repeats for as long as possible (TM permitting)

Warning:
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None