The origin of the 28- to 29-day recurrent patterns of the solar magnetic field

Details The origin of the 28- to 29-day recurrent patterns of the solar magnetic field The origin of the 28- to 29-day recurrent patterns of the solar magnetic field

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..104..425s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 104, April 1986, p. 425-429.

Physics

16

Photosphere, Solar Cycles, Solar Magnetic Field, Line Of Sight, Magnetic Flux, Secular Variations, Simulation

Scientific paper

Numerical simulations of the Sun's mean line-of-sight magnetic field suggest an origin for the 28- to 29-day recurrent patterns of the field and its associated interplanetary phenomena. The patterns are caused by longitudinal fluctuations in the eruption of new magnetic flux, the transport of this flux to mid latitudes by supergranular diffusion and meridional flow, and the slow rotation of the resulting flux distributions at the 28- to 29-day periods characteristic of those latitudes.

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