Physics
Scientific paper
Nov 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..136..169f&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 136, Nov. 1991, p. 169-189.
Physics
5
Earth Orbits, Interplanetary Space, Solar Magnetic Field, Solar Wind Velocity, Magnetic Field Configurations, Mariner 2 Space Probe, Solar Diameter, Solar Rotation
Scientific paper
Quantitative relationships that represent the role of the interaction of fast and slow solar wind (SW) streams in the formation of characteristic SW properties at the earth's orbit are determined from observational data. It is shown that maximum values of the magnetic field and density peaks in the neighborhood of the sector boundary (SB) at the base of the high-speed stream front are associated with solar wind characteristics such as the SW minimum velocity near the SB, the maximum velocity in the central part of the fast stream, and the slope of the magnetic field neutral line to the solar plane at 2.5 solar radii.
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