Multi-Instrument Solar Flare Observations II: A SC24 retrospective
From RHESSI Wiki
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{| class="wikitable" | {| class="wikitable" | ||
|- | |- | ||
- | + | || Instrument || C-class || M-class || X-class || Total || Success Rate | |
|- | |- | ||
| RHESSI || 3,673 || 370 || 23 || 4,066 || 58% | | RHESSI || 3,673 || 370 || 23 || 4,066 || 58% | ||
|- | |- | ||
- | | SDO/EVE MEGS-A || | + | | SDO/EVE MEGS-A || 3,825 || 343 || 19 || 4,187 || 100% |
|- | |- | ||
- | | SDO/EVE MEGS-B || | + | | SDO/EVE MEGS-B || 787 || 97 || 8 || 892 || 12% |
|- | |- | ||
- | | Hinode/EIS || | + | | Hinode/EIS || 496 || 54 || 6 || 556 || 8% |
|- | |- | ||
- | | Hinode/SOT || | + | | Hinode/SOT || 1,167 || 177 || 15 || 1,359 || 20% |
|- | |- | ||
- | | Hinode/XRT || | + | | Hinode/XRT || 3,793 || 357 || 26 | 4,122 || 59% |
|- | |- | ||
- | | IRIS || | + | | IRIS || 523 (3,349) || 76 (335) || 5 (16) || 604 (3,700) || 16% |
|- | |- | ||
|} | |} |
Revision as of 16:01, 6 March 2017
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 | 3,825 | 343 | 19 | 4,187 | 100% |
SDO/EVE MEGS-B | 787 | 97 | 8 | 892 | 12% |
Hinode/EIS | 496 | 54 | 6 | 556 | 8% |
Hinode/SOT | 1,167 | 177 | 15 | 1,359 | 20% |
Hinode/XRT | 3,793 | 357 | 4,122 | 59% | |
IRIS | 523 (3,349) | 76 (335) | 5 (16) | 604 (3,700) | 16% |
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)"