Coronal Diagnostic Spectrometer at Imperial College

JOP35 - Ground Based Instrumentation and Other Spacecraft

Yohkoh
SXT full-Sun images would be useful. Their cadence can be much faster than that of EIT so any coronal changes which may influence the study can be identified.

He 10830A
these images can be obtained from Sac Peak or elsewhere.

Other
In addition, H-alpha (Big Bear, sOON) and magnetogram (Marshall, SOON) data from ground based observatories.


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Page last updated 21st September 1996.