Study 000487:

ACRONYM: DRW001_HI_BRT_V3

HOP212: This study is a modified version of DRW001_HI_BRT_V2 

Modification: 10 pointing positions

The study is intended to be run exactly on the disk centre in Quiet Sun, plage or
equatorial Coronal hole conditions to search for rapidly evolving, cool events such
as swirls and spicules.

The study consists of a single raster, with 10 contiguous positions
of EIS's narrow slit (1"), making a narrow but tall scan with 30 second
exposures at each position.

Target:			QS
Exposures:		10
FOV:			10"X240"
Expsoure time:		30s
Raster Duration:	5m 34s
Compression:		DPCM
Volume:			18 Mbits

Target:
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QS patch at Sun centre

Instruction to planners:
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1 - Run study #378 (IUU_SLOT_488x512) as a context raster
2 - Run this study. Minimum 12 raster repeats
3 - Run study #378 (IUU_SLOT_488x512) as a context raster

It is recommended to run these studies chained.

For Hop212: The prime 1 hour interval for each day will be from 09:00 UT until 10:00 UT

Contact details: eamonms@astro.uio.no

WARNING:
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Please note the error in the raster description. It should be:

DRW_CLBRT_SCAN_10"_v3

rather than _5"_v3 (the _5" is left accidentaly from v2)