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Table 6.
Examples of SPICE observations.
Objective | Spectral lines | Slit | FOV | Exp. time | Duration | Data rate | Data volume |
---|---|---|---|---|---|---|---|
QS dynamics | C III 997.0, Ne VIII 770.3, H I 1025.7, O II 718.5*, O IV 787.7*, Ne VI 997.2*, Mg IX 749.5*, Mg VIII 772.3*, Mg VIII 782.3*, O VI 1031.9 | 2″ | 256″ × 829″ | 5 s | 12 min | 18 kb s−1 | 12 Mb |
Composition | Ar VIII 713.8, S V 786.5, Mg IX 706.1, O VI 1037.6, Mg VIII 782.3, Ne VIII 770.4, O VI 1031.9* | 6″ | 954″ × 829″ | 60 s | 2.6 h | 2.1 kb s−1 | 19.2 Mb |
Notes. The assumed compression rates are 20:1 for spectral windows (SHC) and 10:1 for intensity windows (marked with a ). In these observations, the raster step in the x direction is equal to the nominal slit width.
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