Study 000333:

ACRONYM: blinker_cr

Study description: 

The purpose of this study is to understand the driving mechanism(s) of quiet
Sun brightenings in the solar atmosphere and their coronal responses. 

Acronym				: blinker_cr
Target				: Quiet Sun 
Raster				: scanning
Slit				: 2”
FOV				: 70”x248”
Raster duration			: 26m1s
Raster Data Volume		: 17.5 Mbits

Pointing:
--------

quiet Sun at the disk center 

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

*** Requires raster repeat ****

To be run minimum 2 days, around 3 hours per day of continuous observations
i.e., around ** 7 raster repeat ** .

Solar rotational compensation is needed i.e., tracking the same region on
the Sun.

As it is a coordinated observation with SoHO, it is essential to have the
same FOV observed. If there is an offset between CDS/SoHO and EIS/Hinode,
it has to be taken into account. 

It is essential to have simultaneous H-alpha and FGIV magnetograms / SOT
and Al Poly / XRT observations.

If/when the HOP run, please contact:

Maria Madjarska at
madjarska@mps.mpg.de
tel. +49 2406 303 5295 

Warning:

None