Mathematics
Scientific paper
May 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7634107d&link_type=abstract
Unknown
Mathematics
Interplanetary Magnetic Fields, Latitude, Mathematical Models, Satellite Observation, Solar Wind, Comet Tails, Cosmic Rays, Geomagnetism, Plasma-Particle Interactions, Scintillation, Solar Corona, Solar Orbits, Three Dimensional Models
Scientific paper
The experimental information on latitude effects in the solar wind plasma, obtained from both direct measurements and, indirectly, from observations of comet tails and radio scintillations, is reviewed. Magnetic field observations, notably of the polar magnetic field and of the semiannual variation of the geomagnetic activity, are reported. Theoretical models of latitudinal effects in the solar wind are outlined; three-dimensional solar wind models and studies of gas-magnetic field interactions are considered. The results of such models are reported in detail for different types of coronal boundary conditions, both uniform and non-uniform. The predictions of the theoretical models are compared with the available experimental knowledge on latitudinal structures of the solar wind plasma and the interplanetary magnetic field.
Dobrowolny Marino
Moreno Giovani
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