Other
Scientific paper
Dec 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsa12a..02g&link_type=abstract
American Geophysical Union, Fall Meeting 2002, abstract #SA12A-02
Other
7513 Coronal Mass Ejections, 7514 Energetic Particles (2114), 7534 Radio Emissions, 7851 Shock Waves
Scientific paper
The Solar and Heliospheric Observatory (SOHO) detected a large number of coronal mass ejections (CMEs) during the April 14-24, 2002 period. We describe the properties of these CMEs and contrast them with those of the general population of CMEs. We explore the connection of these CMEs to the interplanetary shocks and the solar energetic particles events using Wind and GOES data, respectively. We assess the extent of preconditioning of the corona by repeated flaring and mass ejections from the active regions involved. Based on the arrival times of the interplanetary CMEs and shocks, we discuss the evolution of these disturbances as they propagated between the Sun and Earth. We compare the extended nature of the main phase of the complex geomagnetic storm to other other similar extended storm periods
Gopalswamy Nat
Gurman Joe B.
Howard Russ A.
Kaiser Michael L.
Lawrence Gareth
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