Study 000516:

ACRONYM: eis_tornadoes_sns_n

This study is intended to take sequences of exposures with the slit crossing the solar
tornado to obtain information on the temporal evolution of its dynamical properties.

observing mode: sit-and-stare
slit: 2"x256"
compression: DCPM
exposure time: 50.0s
number of exposures: 70
duration: 1h3m33s 
data rate: 8.5 kbits/s
data volume: 32 Mbits 
number of lines: 9

Pointing: 
-------

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

Instruction to planners:
-----------------------

1) Run context study (eis_tornadoes_scan_n, ID #515). The slit should be
located in the middle part of the main sit-and-stare (this study) observation.

2) Run this study; eis_tornadoes_sns_n. The Slit to be located at the centre of the context
(as in step 1). The number of raster repetitions: 6-8 (subject to TM availability). It is
recommended that this study is "chained" to the context in step 1 so they should run
back-to-back.

3) Run context (as described in step 1). Again preferably chained with the SNS study (step 2)


Warning:
--------

None