General description

This SOOP describes a coordinated observation of all high resolution RS instruments, running at highest resolution and variable but high cadence, for a short period of time.

As a planning scenario, we propose to run this SOOP at every perihelion window where we have some extra TM to spare, or where the campaign would fit without sacrificing too much of the rest of the orbit.

This SOOP can be run for different targets, also at plain disk centre, as it is aimed to discover new physics and compare high cadence dynamics in all kinds of solar regions.

Ideally, we would like to observe the same active region close to the disk center and at the limb. This will probably be not possible, so two active regions (one close to the disk center, one at the limb) should be observed. The ideal duration would be 1 hour for each pointing, i.e. 2 hours of observations in total. If this is too much telemetry-wise, then we could perhaps go down to 30 minutes of continuous observations for each pointing, but 10 minutes sounds too short.

Default SOOP duration: 1 hour (can be repeated several times when it fits)

Pointing requirements: may be run at disk-centre or off-pointed

Triggers: disabled

Observations requirement (baseline)

Science objectives

Instances run / planned, differences from the baseline observations

LTP9 

2022-10-12 & 13 (SOOP Coordinators: H. Peter)

LTP11

2023-03-29 and 2023-04-06 (SOOP Coordinators: H. Peter)

Any further information to be added:

(e.g. pointing description, evolution of target, coordinated observations, ...) 

Science outcomes

Ref of paper using the SOOP data

Original SOOP proposers

D. Berghmans, S. Krucker, J. Hirzberger, L. Harra, D. Hassler, S. Parenti, A. De Groof, A. Zhukov