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Table 1:

May 17, 2002-time line.
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$^\circ $ v = 370, width = 38$^\circ $
      04:26 E 91$^\circ $ v =  123, width = 10$^\circ $
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$^\circ $
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$^\circ $
Radio 3 AIP, WIND 07:41-07:46 80-1 MHz IIIG, changing $f_{\rm start}$
EUV 1 EIT 07:48 second image of the loop, $v_{\rm rise}$ =  135
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 $\approx $08:00-08:10 CME continuum
    AOO 08:06 main 3 GHz pulse
WL 2 LASCO-C2 CME 08:06 E 61$^\circ $ v =  665, width = 92$^\circ $ GO
  2   08:06 E 61$^\circ $ v =  347, width = 95$^\circ $ OLZ
Radio 3 AIP 08:14-08:23 II 55-40 MHz
  4 NRH11 radio loop E 76$^\circ $ $h \approx 70$ Mm at 327 MHz
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$^\circ $
WL   LASCO-C3 CME 08:42 UT (cf. Footnote 1, Sect. 2.2)
EUV 5 UVCS 08:28-9:58 slitpos. E 90$^\circ $ covering postCME CS
  5   from 2.1-1.5 $R_{\odot }$ 9:13-9:58 OVI reduced, SiXII enhanced
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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