Other
Scientific paper
Oct 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985sssmp..28.1081z&link_type=abstract
Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences (ISSN 0253-5831), vol. 28, Oct. 1985, p.
Other
Heliosphere, Solar Activity Effects, Solar Magnetic Field, Kinetic Energy, Solar Cycles, Solar Flares, Solar Rotation, Solar Wind Velocity
Scientific paper
The response of heliospheric quantities to solar phenomena is discussed from a statistical point of view. It is shown that the ratio of the magnetic to the thermal heliospheric magnetic parameter is one of the physical characteristics useful in determining the influence of solar activity on the heliospheric disturbance and especially for distinguishing different effects exerted by brilliant flares and normal and faint flares. The ratio is also useful for identifying the precursor in the ascending and maximum phases for postmaximum stable high-speed streams from coronal holes. The magnetic sonic speed has a rather stable heliolongitudinal distribution, and high magnetic sonic speed is a common property of both the region with magnetically strong stream in the ascending and maximum phases and with stable high-speed streams in the postmaximum phases. The other magnetic parameters also characterize all these features to some extent.
Gao Yanfang
Lu Caidian
Xu Yadong
Zhang Guobao
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