Multi-Instrument Solar Flare Observations II: A SC24 retrospective
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Contents |
Introduction
Using the search capabilities outlines in a previous nugget, we can now do a retrospective analysis to see how successful - or otherwise - our coordinated observations have been during Solar Cycle 24.
Statists
Instrument | C-class | M-class | X-class | Total | Success Rate | |
RHESSI | 3,673 | 370 | 23 | 4,066 | 58% | |
SDO/EVE MEGS-A | 302.9-304.9 | 3.4x1029 | ||||
SDO/EVE MEGS-B | 1600-1740 | 2.6x1029 | ||||
Hinode/EIS | 1464-1609 | 1.7x1029 | ||||
Hinode/SOT | 504-912 | 1.8x1029 | ||||
Hinode/XRT | 3967-3970 | 5.5x1028 | ||||
IRIS | 370-504 | 3x1028 |
UpSetR plots
Biographical Note
Ryan Milligan is currently an Ernest Rutherford Fellow at the University of Glasgow.
References
[1] "Performance of Major Flare Watches from the Max Millennium Program (2001 - 2010)"