Computer Science
Scientific paper
Mar 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216..428p&link_type=abstract
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 428-431 (2010).
Computer Science
Solar Magnetism, Magnetic Field Effects, Solar Corona, Spacecraft, Solar Wind Plasma, Sources Of Solar Wind, Electric And Magnetic Fields, Solar Magnetism, Corona, Spacecraft/Atmosphere Interactions
Scientific paper
In-situ data measured by Ulysses-SWOOPS, SWICS and VHM instruments-are used for the study of magnetic field and solar wind plasma parameters for the year 2001, in an attempt of founding new ICMEs based on the combination of classical identification conditions, plasma dynamics signatures, and plasma composition signatures. Three new candidates are determined for the DOY 80.3-81.6, DOY 155.18-156.3, and DOY 161.2-162.8. We track back to the Sun these events and determine their possible solar sources.
Dumitrache Cristiana
Popescu Nedelia Antonia
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