Proposed SOOP Coordinators
D. Berghmans, A. Giunta, A. Zhukov
Description
High resolution observations of ARs or other solar features to discover the finest scales. SOOP with low cadence observations as we do not aim at analysing dynamics here. Perihelion preferred.
Pointing requirements: may be run at disk centre or offpointed (without metis)
Default SOOP duration: 12 hours (TBC)
Triggers: disabled
| Instrument | Mode | Comment |
|---|---|---|
| EUI | HRI in highest resolution, e.g. in EUV & LYA Quiet Sun modes (Q) or EUV & LYA Active Region modes (A) - LOW CADENCE: 10mins | best at perihelion. Model AR mode, 10 mins cadence |
PHI | HRT in highest resolution, e.g PHI_vector_HRT1 with cadence 10mins (or PHI_nominal_FDT/HRT_0 with much lower cadence)-> best mode TBD by PHI team | PHI need depending on science goal |
| SPICE | one of the high res modes, depends on science goal. Model as SPICE Dynamics (highest resolution mode). | may be needed for waves and/or temperature structure discrimination, depending on science goal |
| Metis | in one of METIS standard modes, e.g. MAGTOP with 10mins cadence (=default) | may be part of this SOOP for off-limb observations (close to perihelion only) like plumes |
| SAP objective | Target | Duration | Opportunity (e.g., orbital requirements, solar cycle phase, quadrature ...) | Operational constraints | Additional comments |
|---|---|---|---|---|---|
| 1.2.1.6 Resolve the geometry of fine elemental loop strands | |||||
1 Comment
Anik De Groof
SOOP ID in SOOP Kitchen = RS8