Study 000464:

ACRONYM: QUB_HI-CAD_FLARE_2S-EXP_104"x104"

This is a fast-raster study designed to support ground-based observations from ROSA by
measuring plasma dynamics and density changes during solar flares over a broad range of
temperatures. It is also a potential candidate study to use in response to the EIS flare
trigger. 

TARGET: Flare
EXPOSURE TIME: 2s
RASTER: Scanning
SLIT: 2"
STEP SIZE 2"
FOV: 104"x104"
DURATION: 3.5 mins
LINES: He II, O V, O VI, Mg VI, Mg VII, Fe VIII, Fe X, Fe XI, Fe XII (dens. sens. pair),
Fe XIII (dens. sens. pair), Fe XIV (dens. sens. pair), Fe XV, Fe XVI, Fe XVII, Ca XV
(dens. sens. pair), Fe XXIII, Fe XXIV

VOLUME: 18 Mbits (x16 repeats = 300 Mbits per hour = 1200 Mbits for 4 hours)

POINTING:
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A flare producing active region (C-class flares or greater) as announced by the Max
Millennium Chief Observers in their daily messages. The region can be anywhere on the
solar disk.

INSTRUCTIONS TO PLANNERS:
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The scheduling of the proposed HOP is determined by the seeing conditions at Sunspot,
NM at the time of the observing campaign (currently scheduled for 9-14 July 2011,
inclusive). Typically, seeing conditions are optimal during the first few hours after
sunrise (~14:00-18:00 UT). We therefore request that EIS continuously raster over the
chosen Target of Opportunity (ToO) during this 4 hour period, whether on the disk or
at the limb.

Warning:
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High data volume