Study 000643:

ACRONYM: cool_loop_network

This is a modification of cool_loop_response. Originally designed for
coordination with IRIS, particularly looking at sunspot plumes/fan
loops. Removed some coronal lines compared to
cool_loop_response and increased the exposure time to 30s (from
20s). Fe X window expanded to include the OVI 184.02 line, step size reduced to 2" and number of steps reduced to 5.These reduce duration and the data rate.


Ysize: 144"
Xsize: 12"
Slit: 2"
Step-size: 2"
Exposure time: 30s
Duration: 2min 47s
Compression: DPCM
Data volume: 2.8 MBits (DPCM)

Pointing:
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Quiet sun network.

Instruction to planners:
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Point at the network seen in the AIA 304 channel.
Use raster repeats, as TM availability permits.

Please run IUU_SLOT_104x512_Q85 (ID 248) as a context study before and after the high cadence rasters with the FOV on the central 10" of the slit raster.

Warning:
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None