- Photospheric reconnection (Borrero et al., 2010; Martínez Pillet et al., 2011; Borrero et al., 2013; Requerey et al., 2015).
Operational requirements table:
Requirement | YES / NO / Not required / MAYBE / GOOD TO HAVE / NUMBERS | Remarks |
|---|---|---|
| Duration of the observations | ? | |
| Perihelion | Yes | |
| RS window | Yes | RS only |
| High latitude | Good to have | Low and high latitude |
| Solar cycle dependence | Good to have | |
| Radial dependence | No | |
| Linkage science | No | The related linkage science should already be included in the solar wind sub-objectives. |
| Multiple orbits | Good to have | |
| Far side observations | No | |
| Earth observations | Good to have | |
| EMC Quiet | No | |
| SPP | No | Unless they need for their planning. |
| Instruments | SoloHI, PHI, METIS, SPICE? | RS only |
Required observations:
- SoloHI: Contribute (mode: synoptic+shock+turbulence), no min. obs time, all distances.
- SPICE: No
PHI,
FDT medium-high resolution data
Requirement
FOV [pixels]
1024 x 1024 – 2048 x 2048
Parameters
Ic, B, γ, φ
duration
10 days
cadence
1/(10 min)
N orbits
4
solar distance
entire orbit
PHI operating mode
2
co-ordination
?
HRT high resolution data
Requirement
FOV [pixels]
2048 x 2048
Parameters
Ic, vLOS, B, γ, φ (interlaced with raw data)
duration
5 hours
cadence
1/(1 min)
N orbits
2
solar distance
perihelion, polar passage
PHI operating mode
0
co-ordination
?
- METIS: Measurement of the electron density through the polarised brightness in VL (580-640 nm) in the field of view 1.5-2.9 degrees to derive the evolution of the magnetic field topology from the global corona evolution in different time-scales.
- Products:
- Global maps of the electron density in corona/coronal configuration.
- Modes:
- MAGTOP (min. obs time 2 hr, data volume ≤ 480 Mb)
- GLOBAL (min. obs time 2 hr, data volume ≤ 300 Mb)
Repeated each half a day in one observation window.
- Other instruments: PHI, EUI, SoloHI, MAG, SWA.
- Products:
Duration:
Other constraints: