The behavior of the cosmic ray equatorial anisotropy inside fast solar wind streams ejected by coronal holes

Details The behavior of the cosmic ray equatorial anisotropy inside fast solar wind streams ejected by coronal holes The behavior of the cosmic ray equatorial anisotropy inside fast solar wind streams ejected by coronal holes

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8413130i&link_type=abstract

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Physics

Anisotropy, Coronal Loops, Solar Corona, Solar Cosmic Rays, Solar Wind, Diurnal Variations, Harmonic Analysis, Harmonic Radiation

Scientific paper

The cosmic ray equatorial anisotropy inside broad high-speed solar wind streams ejected by coronal holes, i.e, in quasistationary condition, was analyzed. From the beginning to the end of the stream the amplitude of the first and second harmonics of the anisotropy are found to decrease remarkably, by factors of 2.5 and 2.0 respectively, while the phases do not show systematic variations. The development of the stream structure in interplanetary space together with the Parker theory on the diurnal anisotropy in stationary condition explains the large variation observed in the first harmonic of the anisotropy. The behavior of the second harmonic is discussed.

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