Physics
Scientific paper
Jan 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29...15v&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, Jan. 1989, p. 15-19. In Russian.
Physics
Current Sheets, Heliosphere, Interplanetary Magnetic Fields, Magnetic Field Configurations, Solar Wind Velocity, Approximation, Lines Of Force, Nonuniform Plasmas, Solar Rotation, Velocity Distribution
Scientific paper
The surface shape of the heliospheric current sheet is investigated in the kinematic approximation. It is shown that this surface shape is determined by the solar rotation, the form of the magnetic-field neutral lines on the solar surface, and the inhomogeneity of the solar-wind velocity field. Attention is given to the curving and formation of three-dimensional folds on the current-sheet surface in the heliosphere.
Triskova Ludmila
Veselovskii I. S.
No associations
LandOfFree
The surface shape of the heliospheric current sheet with consideration of the solar-wind velocity inhomogeneity does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The surface shape of the heliospheric current sheet with consideration of the solar-wind velocity inhomogeneity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The surface shape of the heliospheric current sheet with consideration of the solar-wind velocity inhomogeneity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-827282