Physics
Scientific paper
Sep 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..117n&link_type=abstract
SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 117-1
Physics
Particle Emission, Solar Wind, Interplanetary Magnetic Fields, Solar Wind Plasma, Sources Of Solar Wind
Scientific paper
The magnetic fields of interplanetary objects that were ejected as coronal mass ejections (CMEs) from the limb of the Sun were observed by the NOZOMI spacecraft at 1.38 AU above the east limb of the Sun. The solar wind magnetic field whose launch time coincided with ejection of the limb CME was different from that estimated from ACE observations near the Earth, suggesting that NOZOMI encountered transient magnetic structures, or that the heliospheric magnetic field re-structured after ejection of the CMEs. The corresponding interplanetary magnetic field showed non-spiral magnetic field, enhancements of magnetic field, or magnetic discontinuities, but no common structure was yet found.
Matsuoka Ayako
Nakagawa Takao
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