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Wave band | Figure | Instrument/ | Description |
observatory | (times in UT, speeds in km s-1, angles, colatitude, degrees, | ||
counterclockwise from North Pole) | |||
WL | LASCO-C2 | CME at 01:50 E 90![]() ![]() |
|
04:26 E 91![]() ![]() |
|||
X-rays | GOES | 05:16-05:28 (AR 9957) | |
H-alpha | SVTO | 05:20-05:34 (AR 9957) | |
X-rays | 3 | GOES | 07:27-07:54- >08:40 M1 |
UVB | CELIAS | 07:30 onwards: SEM flux increase | |
hard X-rays | RHESSI10 | 07:32-07:36 double source, motion, 07:37 single source at E 76![]() |
|
Radio | AOO | 07:32- >08:12 3 GHz complex dm burst, main max. 08:06 | |
3 | AOO, AIP | 07:37-07:59 1800-350 MHz drifting pulsating structures | |
EUV | 1 | EIT | 07:36 first rising loop image 195 Å at E 76![]() |
Radio | 3 | AIP, WIND | 07:41-07:46 80-1 MHz IIIG, changing
![]() |
EUV | 1 | EIT | 07:48 second image of the loop,
![]() |
Radio | 3 | AIP, WIND | 07:52-07:59 IIIG, 07:59 sudden end of m-Dm IIIG KA |
AIP | 07:56-07:58 faint narrowband pattern in 360-420 MHz | ||
3 | AIP | ![]() |
|
AOO | 08:06 main 3 GHz pulse | ||
WL | 2 | LASCO-C2 | CME 08:06 E 61![]() ![]() |
2 | 08:06 E 61![]() ![]() |
||
Radio | 3 | AIP | 08:14-08:23 II 55-40 MHz |
4 | NRH11 | radio loop E 76![]() ![]() |
|
Optical | WROC | <08:27-12:24 Erupt. prominence at limb N15E90 | |
4 | AIP, NRH | 09:11:30-09:12:30 IIIG 500-260 MHz E 110![]() |
|
WL | LASCO-C3 | CME 08:42 UT (cf. Footnote 1, Sect. 2.2) | |
EUV | 5 | UVCS | 08:28-9:58 slitpos. E 90![]() |
5 | from 2.1-1.5 ![]() |
||
X-rays | GOES | 12:05 E 82 | |
H-alpha | SVTO | 16:11 E 83 | |
X-rays | GOES | 23:06 E 63 (AR 9957) | |
H-alpha | HOLL | 23:07 E 63 (AR 9957) | |
WL | LASCO-C2 | CME 13:50 E 89 | |
WL | LASCO-C2 | CME 16:26 E 95 | |
IP shock | CELIAS | May 20, 02:56 UT |
10 Images to 40 keV in Karlický et al. (2004); end of RHESSI (Ramaty High Energy Solar Spectroscopic Imager) obs. at 07:39 UT; 11 start of obs. at 08:27 UT.
Abbreviations: UVB: UV broadband, GO: /cdaw.gsfc.nasa.gov/CME_list, OLZ: /spaceweather.gmu.edu/seeds, KA: /lep694.gsfc.nasa.gov/waves, AIP: Astrophysikalisches Institut Potsdam; AOO: Astronomical Observatory Ondrejov; NRH: Nançay Radio Heliograph; SVTO: San Vito, HOLL: Holloman.
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