Streamers study at solar minimum: combination of UV observations and numerical modeling

Details Streamers study at solar minimum: combination of UV observations and numerical modeling Streamers study at solar minimum: combination of UV observations and numerical modeling

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216..387a&link_type=abstract

TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 387-390 (2010).

Computer Science

3

Solar Wind, Magnetohydrodynamics, Solar Corona, Magnetic Field Effects, Particle Emission, Solar Wind, Magnetohydrodynamics And Plasmas, Corona, Electric And Magnetic Fields, Solar Magnetism

Scientific paper

The present study concerns a comparison between the slow solar wind plasma parameters obtained in the extended corona by the UV spectroscopic data from the Ultraviolet Coronagraph Spectrometer (UVCS) onboard SOHO during the minimum of solar activity (1996) and the results of a time-dependent 2.5 D three-fluid MHD model of coronal streamer belt. The aim of the study is to improve the knowledge of the slow solar wind acceleration mechanism and the origin of its variability.

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