\begin{table}%t1
\caption{\label{Tab}May~17, 2002--time line.}
%\centerline
 {\small \begin{tabular}[]{lllp{9cm}}
\hline \hline\noalign{\smallskip}
{\bf Wave band}&{\bf Figure} & {\bf Instrument/}& {\bf Description}  \\
& & {\bf observatory} & (times in UT, speeds in {\bf km~s$^{-1}$}, angles, colatitude, degrees,\\
& & & counterclockwise from North Pole) \\
 \hline
&&  & \\
WL & & LASCO-C2 & CME at 01:50~E~90$^{\circ}$ $v$ = {\bf 370}, width~=~38$^{\circ}$ \\
 & & & 04:26 E 91$^{\circ}$ $v$~=~{\bf 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--~$>$08:40~M1 \\
UVB & & CELIAS & 07:30~onwards: SEM flux increase \\
hard X-rays& & RHESSI$^{10}$& 07:32--07:36 double source, motion, 07:37 single source at E~76$^{\circ}$\\
Radio & & AOO & 07:32--~$>$08:12 3~GHz complex dm burst, main max. 08:06 \\
&3 & AOO, AIP & 07:37--07:59 1800--350~MHz drifting pulsating structures \\
EUV & 1& EIT & 07:36 first rising loop image 195~\AA{} at E~76$^{\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, $v_{\rm rise}$~=~{\bf 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}$ $v$~=~{\bf 665}, width~=~92$^{\circ}$ GO \\
& 2& & 08:06 E 61$^{\circ}$ $v$~=~{\bf 347}, width~=~95$^{\circ}$ OLZ \\
Radio& 3&AIP& 08:14--08:23~II 55--40~MHz  \\
&4 & NRH$^11$& 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.~\ref{rxo})\\
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 \\
\noalign{\smallskip}\hline\noalign{\smallskip}
\end{tabular}}
\medskip 
$^{10}$ Images to 40~keV in Karlick\'y 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. \\
{\it Abbreviations:} UVB: UV broadband, GO: \url{/cdaw.gsfc.nasa.gov/CME{\_}list}, OLZ: \url{/spaceweather.gmu.edu/seeds},
KA: \url{/lep694.gsfc.nasa.gov/waves}, AIP: Astrophysikalisches Institut
Potsdam; AOO: Astronomical Observatory Ond\v{r}ejov; NRH: Nan\c{c}ay Radio Heliograph; SVTO: San~Vito, HOLL: Holloman.
\end{table}