Study 000512:

ACRONYM: Cor_Hole_Jet_v1

This routine is designed to monitor the evolution of jets in coronal
holes. The intention is to select a bright point in a coronal hole and
hope that it produces jets.

It is recommended to run a context raster such as PRY_slot_context_v3
before and after the study.

Parameters
Duration: 6min 31s
Slit: 2"
Step size: 4"
Raster size: 42"x168"
Exposure time: 30s
Data volume: 2.5 MB
Data rate: 6.5 kB/s
Compression: DPCM