Computer Science
Scientific paper
Sep 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535....3b&link_type=abstract
In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2
Computer Science
2
Solar Magnetic Fields
Scientific paper
Grouping tendency in the magnetic flux emergence in the solar photosphere; single local magnetic fields and complexes of activity. Relation of the local and background large-scale magnetic fields (global fields), dynamics of their evolution. Longitudinal distribution and sector structure in the solar magnetic fields. Magnetic field as a coupling factor of all layers of the solar atmosphere with the convective zone. Reflection of the solar magnetic field changes in the heliosphere. Regularities in the solar activity appearance. Local and global magnetic fields during different phases of the solar activity cycle, and variations in their longitudinal and latitudinal distribution with time. Characteristics of such changes, quasi-biennial oscillations, shorter-term periodicities in magnetic flux formation and solar rotation rate variations. Reflection of the solar magnetic field cyclic and short-term changes in the corona, in the heliospheric magnetic field distribution and in the variation of the solar wind characteristics.
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