Proposed SOOP Coordinators
A. Giunta, S. Parenti, D. Berghmans, D. Spadaro, A. Fludra, L. Harra, D. Baker
Description
Mapping the abundance of minor ions as a function of height in the corona to distinguish between slow and fast wind. This will be targeted at the boundary of a streamer, or at an active region on the limb. SPICE-led.
Default SOOP duration: 3 hrs
POinting requirements: off-pointing close-in / disk-centre farther out
Triggers: disabled
Instrument | Mode | Comment |
---|---|---|
EUI | HRI observations, e.g. in EUV & LYA Active Region modes (A). Cadence TBD (currently modelled with 360s cadence, i.e. 20.2 kbps) | Context and also higher (than SPICE) cadence observations in order to interpret the SPICE composition map |
Metis | One of METIS standard modes before main observations, get coronal context, but will not participate at limb pointing (unless s/c at large heliocentric distance): mode TBD Currently modelled as WIND | Context especially important for streamers |
PHI | FDT synoptic data: 1024 x 1024 pixels, at 6 hr cadence Ic, B, γ, φ | PHI is needed for context magnetic field, but mainly before or after the SPICE observations as the target will be on the limb! |
SPICE |
| Lines for SPICE Composition Mapping: – 15 lines (2 profiles+ 13 intensities)
( L_BOTH_HRES_LCAD_CH-Boundary-Expansion assumed to be default.) |
.
SAP objective | Target | Duration | Opportunity (e.g., orbital requirements, solar cycle phase, quadrature ...) | Operational constraints | Additional comments |
---|---|---|---|---|---|
1.1.2.3 Abundance of minor ions as a function of height in the corona as indicator of slow or fast wind | Limb active region (incl the edges), or streamer boundary at limb | 3.2 hours, twice | Any RSW is okay, but perihelion preferred for the AR case, and >0.55AU is preferred for the streamer case (requires Metis compatibility) | put EUI in at least twice the cadence of SPICE to interpret composition map (and possible aliasing in time) |
1 Comment
Anik De Groof
SOOP ID in SOOP Kitchen = RS7