Tracing the magnetic topology of coronal mass ejection events by Ulysses/HI-SCALE energetic particle observations in and out of the ecliptic
Source: Space Science Reviews, Volume 97, Numbers 1-4, 2001 , pp. 263-268(6)
Abstract:In January 2000, the Ulysses spacecraft observed an ICME event at 43° S heliographic latitude and ∼ 4.1 AU. We use electron (E_e>38 keV) observations to trace the topology of the IMF embedded within the ICME. The still controversial issue of whether ICMEs have been detached from the solar corona or are still magnetically anchored to it when they arrive at the spacecraft is tackled. An in ecliptic ICME event is also presented.
Document Type: Regular Paper
Affiliations: 1: Demokritos University of Thrace, Xanthi, 67100, Greece 2: Bell Laboratories, Lucent Technologies, U.S.A. 3: Observatoire de Paris, DASOP, F-92195 Meudon Principal Cedex, France 4: National Observatory of Athens, ISARS, GR-15236 P. Penteli, Greece
Publication date: January 1, 2001