Proposed SOOP Coordinators
D. Spadaro, A. Vourlidas, A. Giunta, D. Williams
Description
This SOOP is designed to be used as a whole- or half-orbit Synoptic campaign that scans the Sun from one high latitude to the other (therefore mainly to be used later in the NMP at min inclination of 15º, i.e. orbit 3 or later). Close to the higher latitude windows, we get a radial sweep at nearly constant latitude for in-situ.
This SOOP resembles very much the L_FULL_LRES_MCAD_Coronal-Synoptic but this time SPICE is necessary as well.
We could possibly schedule this SOOP after every Venus GAM.
Default SOOP duration: 10 days
Pointing requirements: mainly disk centre
Triggers: only IS triggers active
Instrument | Mode | Comment |
---|---|---|
EUI | FSI Synoptic mode (S) with FSI | 10 min cadence |
Metis | One of METIS standard modes to observe large scale coronal structures: GLOBAL or LT-CONFIG Model: LTCONFIG (cadence 20mins) and 3 x 1 hour CMEOBS | CME Watch On could do a slight offpoint without switching metis off, e.g. to poles during RSW1+3 |
PHI | FDT in general though HRT could be high resolution, medium cadence (TBC) | at higher latitudes, point to the poles for polar magnetic field observations. |
SoloHI | SoloHI synoptic Operations Currently modelled as HI_SYN_NEAR | |
SPICE | SPICE Composition Mapping raster followed by multiple instances of SPICE CME Watch | SPICE scans many latitudes during the SOOP : large swath around the sun magnetic field spiral less curved at higher latitudes: Use observation called SPICE_CME_COMP in modelling. |
STIX | N/A | |
EPD | Normal + Burst Mode | |
MAG | Normal + Burst Mode | |
RPW | Detection Mode | Burst Triggers Active |
SWA | Normal + Burst Mode |
SAP objective | Target | Duration | Opportunity (e.g., orbital requirements, solar cycle phase, quadrature ...) | Operational constraints | Additional comments |
---|---|---|---|---|---|
2.2.1 How do CMEs contribute to the global evolution of magnetic flux in the heliosphere? | |||||
2.2.2 What is the role of ICMEs in the Sun’s magnetic cycle? | |||||
2.1.1.3 CME evolution | |||||
1.1.3.2 How does the Sun's magnetic field link into space? | |||||
4.2 What are the properties of the magnetic field at high solar latitudes? | |||||
2 Comments
Vincenzo Andretta
Anik De Groof
SOOP ID in SOOP Kitchen = LB2