Study 000220:

ACRONYM: SK_CH1_70x512p

Intended to study the evolution of coronal bright points with
moderate cadence. It is designed to minimize observing time
difference of EIS and SUMER by repeating 1-hour narrow scans.
Line list consists of a wide range of iron lines (Fe VIII - Fe XV)
to cover lower corona and high temperature corona.
It also includes weak transition region lines to help
co-alignement with SUMER.

TARGET:  Coronal Hole or Quiet Sun
EXPOSURE TIME: 45s
SLIT:  1"
FOV:  70"x512"
SPECTRAL WIND: 15
DATA COMP. : DPCM
POINTING: 

POINTING:

Primary target is a bright point in polar coronal holes.
The 512" slit height allows to observe coronal hole boundary
and jets on the limb at the same time.

WARNING:

None