Study 000627:

ACRONYM:  cam_flare_hot1_v2

Updated	by M. Whillock,	MSSL, 20220708.
Copied from study id 0000598, increased	exposure time by 50%.

This study is designed to observe small flares. It has a range of lines at
different temperatures and density diagnostics from Ca XV.

Target: Active Region core / flare
EXPOSURE TIME : 15s
SLIT          : 2"
STEP_SIZE     : 4"
FOV           : 100"x120"
DATA COMP.    : JPEG85 (default)
RASTER DURATON: 7m 45s
DATA volume   : 2.608 Mbit
DATA rate     : 5.6 kbit/s

Lines:

Ca XV lines for density diagnostics
Fe XII lines for density diagnostics
Mg VI, Fe VIII, Fe X, Fe XIII, Fe XIV to observe the
cooler plasma.
AR core lines (3 MK): Fe XVI, Ca XIV, Ca XV, Ar XIV, S XIII.
Flare lines: Fe XVII, Fe XXI,  Fe XXIII, Fe XXIV

Pointing:
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The core of a relatively small active region

Instruction to planners:
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1) Choose a young, relatively small active region likely to produce small flares, and centre the FOV in the middle.

2) Repeat the raster for a maximum possible run-time, accounting for the telemetry constraint.

Warning:
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None