Reflection of the structure of the chromosphere and corona in the solar wind and interplanetary magnetic field

Details Reflection of the structure of the chromosphere and corona in the solar wind and interplanetary magnetic field Reflection of the structure of the chromosphere and corona in the solar wind and interplanetary magnetic field

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..780l&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, July-Aug. 1985, p. 780-789) Soviet Astronomy (ISSN 0038-5301), vol. 29, July-Aug. 1985, p. 4

Astronomy and Astrophysics

Astronomy

9

Chromosphere, Interplanetary Magnetic Fields, Solar Corona, Solar Wind Velocity, Stellar Structure, Coronal Loops, Magnetic Flux, Plasma Density, Solar Activity, Stellar Models

Scientific paper

New features in the structure of the low-velocity solar wind are found and additional indications of the sources of the solar wind are obtained by the method of concrete comparison of data on the solar wind and the interplanetary magnetic field with solar data. These regularities were discovered in data for April 1968 and were confirmed for other intervals. It is shown that: (1) the low-velocity solar wind corresponds to sections of the quiet solar chromosphere between groups of active regions; (2) the low-velocity solar wind carries off the weak large-scale solar magnetic field, the sign of which corresponds to the sign of the weak interplanetary magnetic field; (3) doublet pulses of density, which correspond to the minimum value of the magnetic field strength, are observed at the line of reversal of the sign of the interplanetary magnetic field. The hypothesis is advanced that coronal-loop plasma structures transported by the solar wind to 1 AU are observed. A phenomenological model of the phenomenon is proposed.

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