Description
This mode uses HRI telescopes targeting a full coronal hole, a CH boundary or polar plumes.
The mode can be commanded on HRI_EUV and HRI_Lya telescopes independently.
Parameters
cadence, compression TBC
Resource usage
| Observing mode | Target | Instrument | Channel | Cadence | Rebinning | Compression | Calculated TM | #Images/h | Data Rate | Data Rate | Max time | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (nm) | (s) | or subfield | rate | (bits/image) | (Gibits/h) | (bits/s) | per orbit | |||||
| EUV Coronal hole (C) | Full CH + boundary | HRI_EUV | 17,4 | 30 | 1 | 6.25 | 10066329.6 | 120 | 1,5 | 447392.4 | 30 h | |
| LYA Coronal hole (C) | + plumes | HRI_Lyalpha | Ly alpha | 30 | 1 | 18.75 | 3355443.2 | 120 |
Maximum time in this mode
restricted to 30 hours per orbit = 90% of allocation (if both telescopes are used), if all resulting TM gets downlinked!
SOOP kitchen observations:
EUV_CH
LYA_CH