Proposed SOOP Coordinators
Thomas Wiegelmann, J. Hirzberger, D. Berghmans, D. Spadaro
Description
High spatial resolution synoptic operations with full disk RS instruments, Metis and insitu instruments. Low cadence (1/hour to 1/day). Most relevant for windows or parts of windows with very restricted TM and for out of window synoptic campaigns if these are possible.
Default SOOP duration: 1 day
Pointing requirements: disk centre
Triggers: only IS triggers active
| Instrument | Mode | Comment |
|---|---|---|
| PHI | PHI_synoptic_FDT_4: FDT at highest spatial resolution (2Kx2K), cadence at least 1 per day (PHI mode to be refined, synoptics typically have 1Kx1K resolution) | model cadence as twice per day |
EUI | FSI Reference Synoptic mode (R), highest spatial resolution (3Kx3K), low cadence (hrs to 1/day): | Configure instrument to enhance off-limb structures model cadence as 1/day |
| Metis | synoptic programme for magnetic field structure (METIS standard modes: GLOBAL and/or LT-CONFIG) | no reaction to CMEs needed |
| EPD | normal | |
| MAG | normal | |
| SWA | normal | |
| RPW | normal |
| SAP objective | Target | Duration | Opportunity (e.g., orbital requirements, solar cycle phase, quadrature ...) | Operational constraints | Additional comments |
|---|---|---|---|---|---|
| 1.1.3.2.1 How does the Sun's magnetic field change over time? | Full disk, photosphere and corona | long-term observations (RS synoptics in between RSW?) |
| RSW placement if no synoptics allowed EMC quiet for linkage science | |
| 1.1.3.2.2 How is the heliospheric current sheet (HCS) related to coronal structure? | |||||
1 Comment
Anik De Groof
SOOP ID in SOOP Kitchen = LF3