ULYSSES plasma observations of coronal mass ejections near 2.5 AU

Details ULYSSES plasma observations of coronal mass ejections near 2.5 AU ULYSSES plasma observations of coronal mass ejections near 2.5 AU

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992georl..19.1239p&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 19, no. 12, June 19, 1992, p. 1239-1242. Research supported by DOE.

Physics

23

Geomagnetism, Solar Corona, Solar Wind, Stellar Mass Ejection, Ulysses Mission, Electron Beams, Magnetic Storms, Shock Waves, Solar Activity

Scientific paper

The Ulysses solar wind plasma experiment observed a series of interplanetary shocks and coronal mass ejections (CMEs), the latter evidenced by counterstreaming electrons and a variety of ion signatures, during March and April 1991. A striking sequence was observed near 2.5 AU from March 23 through April 2, with the second of two counterstreaming events lasting 6.4 days. The plasma observations for these features are summarized suggesting that the second counterstreaming period may be two juxtaposed CMEs. The relationship between the events observed at Ulysses, about 60 deg east of earth in ecliptic longitude, and those causing a geomagnetic storm on March 24, is unclear.

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