Physics
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..141..391s&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 141, no. 2, p. 391-410.
Physics
19
Convective Heat Transfer, Geomagnetism, Solar Cycles, Solar Terrestrial Interactions, Sunspots, Dipoles, Helioseismology, Solar Activity, Solar Interior
Scientific paper
Published solar data are used here to establish and discuss the temporal and spatial behaviors of the main components of a two-component cycle. Various properties of the dipole-field sources which are deep-seated in the solar interior and have a rigid rotation of about 27 days are established. Two cyclic phenomena are identified which in each hemisphere link with a 5-6 yr delay the dipole field generation at high latitudes to the bipolar field emergence at sunspot latitudes. The constraints imposed on the mechanisms of the sunspot field generation by a two-component cycle and by new observational results are examined.
Legrand Jean-Pierre
Simon P. A.
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