Large-scale patterns, complexes of solar activity and ‘active longitudes’

Details Large-scale patterns, complexes of solar activity and ‘active longitudes’ Large-scale patterns, complexes of solar activity and ‘active longitudes’

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007hia....14..277a&link_type=abstract

Highlights of Astronomy, Volume 14, p. 277-278

Astronomy and Astrophysics

Astronomy

Sun, Sun: Magnetic Field, Solar Activity

Scientific paper

Typical latitude zones and longitude sectors with a dominant occurrence of newly emerging magnetic flux were systematically detected during three last activity cycles. Two long time persistent longitude sectors with the preferred occurrence of a new strong magnetic flux are characteristic for magnetic flux distribution and their rotation rate is latitude dependent in the relationship with differential rotation rate. Recent new information about the large-scale flows in convection zone relates to a concept of the expected giant cells and jets and show a new relationship with different scales of the large-scale circulation. Non-axially symmetric horizontal flow in upper part of convection zone gives a good motivation for an extension of the existing axially symmetric 2D models into new 3D concept.

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