Physics – Plasma Physics
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh51d1721p&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #SH51D-1721
Physics
Plasma Physics
[7536] Solar Physics, Astrophysics, And Astronomy / Solar Activity Cycle, [7827] Space Plasma Physics / Kinetic And Mhd Theory, [7851] Space Plasma Physics / Shock Waves
Scientific paper
The propagation of waves in the solar wind plasma from 1 AU to the heliospheric boundaries is studied. First we consider the simple 1D spherically symmetric model of the solar wind interaction with the local interstellar medium to describe the wave evolution in the supersonic solar wind flow in which parameters change with heliocentric distance. The hydrodynamics solution and the influence of the interstellar H atoms on the wave structure in the solar wind is discussed. The 2D kinetic-gasdynamic model (Izmodenov et al., 2005, 2008) and 3D MHD model (Opher et al. 2009) are used to study the interaction of the different types of waves in the solar wind with the the termination shock and heliopause.
Izmodenov Vladislav V.
Opher Merav
Provornikova E. A.
Tóth Géza
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