Table 7.
Overview of the operational characteristics of the remote-sensing instruments.
| Instrument | Onboard SCE | Onboard SC80 | Wavelengths | FOV (RSun) | Detector size (pix) | Pixel size (arcsec) | Observable |
|---|---|---|---|---|---|---|---|
| UV and IR coronagraph | × | × | HI Lyα (121.6 nm) | 1.1–2 | 1024 × 1024 | 5 | Magnetic field in low corona |
| HI Lyβ (102.6 nm) | |||||||
| FeXIII (1074.7 nm) | |||||||
| FeXIII (1079.8 nm) | |||||||
| HeI (1083.0 nm) | |||||||
| Visible (560 nm) | |||||||
| Multi-Magnetic Imager | × | Fe I (630.15 nm) | <1.07 | 4096 × 4096 | 0.5 | Magnetic field in photosphere and chromosphere | |
| Fe I (630.25 nm) | |||||||
| NaI (589.59 nm) | |||||||
| NaI (588.99 nm) | |||||||
| Magnetic Imager | × | Fe I (617.3 nm) | <1.07 | 4096 × 4096 | 0.5 | Magnetic field in photosphere | |
| White Light Coronagraph | × | × | 400–850 nm | 2–30 | 1024 × 1024 | 56 | Velocity of CMEs near the Sun |
| Heliospheric Imager | × | 400–1000 nm | 130–216 | 1024 × 1024 | 148 | Properties of the propagation of CMEs through interplanetary medium | |
| EUV Imager | × | × | Fe IX/X (17.4 nm) | <1.6 | 1024 × 1024 | 3.2 | Coronal structures |
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