Study 000515:

ACRONYM: eis_tornadoes_scan_n

This context study is intended to take a 2D raster (FOV = 100"x256") of the area above the
WEST solar limb (or on the solar disk if filaments are observed) with a potential solar
tornado in order to get the general overview of the observed structure.	     	
	 	     
observing mode: scanning
slit: 2"
step size: 2"
number of steps: 49 (total number of exposures: 50)
final FoV; 100"x256"
compression: DCPM
exposure time: 50.0s
duration: 45m33s
data rate: 8.5 kbits/s
Data volume: 23 Mbits
number of lines: 9

Pointing: 
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preferably: prominences above the WEST solar limb, or filaments on disk

Instruction to planners:
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The context raster should be taken before and after the main sit-and-stare observing sequence.

See study ID #516 for details 

Warning:
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None