Proposed SOOP Coordinators
A. Giunta, C. Owen, J. Hirzberger, D. Berghmans
Description
This SOOP is designed to let the high-resolution RS observations cover a wider area than normal, in particular the SPICE FOV. This SOOP is to be used in particular with a mosaic of pointings, though it does not necessarily need to be. Alternatively it could be used when we point for a limited amount of time (few hours typically) to the most likely connectivity point, within a mainly sun-disk-centred observation.
Default SOOP duration: 3 hours
Pointing requirements: mosaic of offpointing
Triggers: only IS triggers enabled
See SOOP 4a defined for SOWG8 planning exercise.
Instrument | Mode | Comment |
---|---|---|
SPICE (leads) | SPICE Composition Mapping (30mins per map)
|
Lines for SPICE Composition Mapping (from 1.1.2.2 Does slow and intermediate solar wind originate from coronal loops outside of coronal holes?) : – 15 lines (2 profiles+ 13 intensities)
N.B. This line list for SPICE Composition Mapping is similar to that of L_BOTH_HRES_LCAD_CH-Boundary-Expansion, except for O VI 1037 (removed) and Si II 992 (added). |
PHI | PHI_magnetograph_FDT/HRT_2 with HRT, 15 mins cadence | 2 PHI/HRT datasets per SPICE map |
EUI | EUV & LYA Coronal hole modes (C) with HRI, 10-15 mins cadence FSI Synoptic mode (S) with FSI | 2-3 HRI images per SPICE map |
SoloHI | SoloHI Synoptic program modelled as HI_SYN_NEAR | cadences adapted to applicable sun distance and TM corridor |
STIX | STIX Normal Mode | |
Metis | will generally be SAFE+door closed, due to off-pointing mosaic. IF far enough from Sun: METIS standard modes for context for connection | |
EPD | Normal Mode | |
MAG | Normal Mode | |
RPW | Detection Mode | Burst Triggers Active |
SWA | Normal Mode |
SAP objective | Target | Duration | Opportunity (e.g., orbital requirements, solar cycle phase, quadrature ...) | Operational constraints | Additional comments |
---|---|---|---|---|---|
1.1.2.7 Trace streamer blobs and other structures through the outer corona and the heliosphere. | N-S mosaic centred on most likely connection point | 3 hrs + slews for mosaic of 6 positions (30mins dwell time) |
|
| radial or quadrature alignment with SPP is a plus |
1.1.2.2 Does slow and intermediate solar wind originate from coronal loops outside of coronal holes? | coronal loops outside of coronal holes | few days |
|
| radial alignment with SPP is a plus |
1.1.3.2.3 How does the heliospheric magnetic field disconnect from the Sun? | |||||
2 Comments
Andrew Walsh
Could also run PHI_PDF_MOSIAC during this assuming the timing makes sense.
Anik De Groof
SOOP ID in SOOP Kitchen = LS4