Study 000563:

ACRONYM: AN_ALMA_EIS_S01V01

A study developed for coordinated ALMA-EIS observations scheduled by
Alexander Nidos for March 2017. These observations will study the
center-to-limb variations of the quiet solar atmosphere.

The study was designed to match the ALMA observing cadence of about
600s followed by 180s of calibration and a ~50"x50" field of
view. This limits the EIS exposure time to about 36s, which is short
for quiet sun observations. Spatial averaging will be needed for many
of the weaker lines.

The line list is taken from the HPW021 series and this study can be
used for active region observations.

TARGET:           Quiet Sun/Active Region
EXPOSURE TIME:    36s
RASTER:           Scanning
SLIT:             2"
STEP:		  3"
FOV:              43"x256"
RASTER DURATION:  9m56s
VOLUME:           22 Mbits
RATE:             36.6 kbits/s
COMP:		  DPCM

Pointing:
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To be determined

Instruction to planners:
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The ALMA observations will call for a repoint after each raster. ALMA and Hinode will both observe for
about 10 minutes. Then ALMA will do 3 minutes of calibration while Hinode repoints and settles at the
next pointing position. 

Warning:
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3" steps are taken between exposures (2" Slit).