'Campaign' refers to a concerted, focused effort on one or more event periods or topics, usually taking place over a limited time period with the goal of a final report or papers devoted to the results of the campaign. Since coronal mass ejections (CMEs) are the primary transient phenomena that cause the largest interplanetary disturbances, driving shock waves that in turn accelerate particles and cause the largest geomagnetic storms, it was decided that the SHINE Campaigns should focus on a few carefully selected CME Events occurring since 1996. The chosen events should have reasonably complete data on both its solar source regions and its propagation through the low corona into the heliosphere. It is desirable but not essential to include Earth-directed events so that their in-situ and geoeffective characteristics can be studied.

Superposition of GOES proton flux, CME height-time plots, GOES X-ray plots for each event.

Click to access various data sources directly.

The SEP time in UTC.

The CME time in UTC.

The CME speed in km/sec.

The width of the CME from LASCO

NOAA region number and the flares heliographic position

GOES X-ray class and start time.

5-min X-rays from GOES

NOAA SEC Event List and the Solar Region Summary.

MDI and MWO map.

Daily MPEG movies from LASCO, EIT 19.5 nm, and Yohkoh/SXT.

Movies from LASCO, EIT 19.5 nm, and TRACE. RD = running difference. LASCO, TRACE1, and TRACE2 movies were created by M. Andrews, D. Alexander, and N. Nitta, respectively.

WIND/WAVES high- and low-resolution and Culgoora spectrograms. The HiRAS plots are high frequency (>20 MHz) spectra mostly from Hiraiso and WIND/RAD 2.

GOES and ACE data were provided by their websites. Wind/LEMT data were contributed by D.V. Reames. Plots from Tylka et al. (2004, submitted to ApJ).

EPAM data from ACE website

Wind/SWE data from NSSDC, courtesy of K. Ogilvie.

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