Study 000287:

ACRONYM: LT_CH_1_510x256_1

Intended to study the morphology and flows in the boundary region between
coronal holes and quiet Sun.

The study is a sparse-raster of a large area with the 2" slit and step size
4" (128 pointing positions),  for 6 spectral windows.

Spectral windows are selected to include
He II (blend) 256.2, O V 192.9, Fe VIII 186.6, Fe X 184.5, Fe XI (blend) 192.8,
Fe XII 186.8, 195.1, Fe XIV 264.7, i.e. with a good temperature coverage
for coronal holes/quiet Sun.

TARGET        : Coronal Hole/Quiet Sun boundary
EXPOSURE TIME : 40s
RASTER        : Scanning
SLIT          : 2"
STEP_SIZE     : 4"
FOV           : 512"x256"
SPECTRAL WIND.: 6
DATA COMP.    : DCPM
VOLUME	      : 32.5 Mbits
RASTER DURATON: 1h 34m

POINTING:

On-disc coronal hole boundary. If possible repeat with 2-3 different
pointings.

INSTRUCTION TO PLANNERS:

There should be ample coverage in each exposure of at least a
part of Quiet Sun. This is to ensure proper wavelength calibration
using the Quiet Sun as a reference.

WARNING:

This study is not suitable for active regions since some of the strong
lines might saturate.