Study 000233:

ACRONYM: Romano_v2

Note: Modified to use DPCM

This study is designed to observe wide regions of the solar disc waiting
for eruptions of active region filaments. Spectral windows are selected
to be able to retrieve a sufficient number of spectral lines with wide
temperature coverage.  The exposure time is selected in order to obtain
useful data during the quiet and  active phases of the filament life.
The goal of this observation is to study the mass motion 
in the upper layers of the solar atmosphere, to do plasma diagnostics and 
to obtain information about the emission variations related to the
activation processes. 

SLIT          : 1"
STEP SIZE     : 1"
EXPOSURE TIME : 10s
FOV           : 360"x512"
TIME REQUIRED : 1hr 14m 47s
REPEATS       : 19 times
DATA RATE     : 35 kbs

TARGET: Eruptive filaments

WARNING:

None