Solar Active Longitude recurring every 28-29 days acting differently in low and higher latitudes

Details Solar Active Longitude recurring every 28-29 days acting differently in low and higher latitudes Solar Active Longitude recurring every 28-29 days acting differently in low and higher latitudes

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991baicz..42..381b&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 42, Nov. 1991, p. 381-385.

Astronomy and Astrophysics

Astronomy

2

Magnetic Field Configurations, Solar Activity, Solar Magnetic Field, Interplanetary Magnetic Fields, Latitude, Photosphere

Scientific paper

The existence of Active Longitudes (ALs) recurring every 28-29 days is
briefly discussed. These Als develop at higher heliophysical latitudes
in the same way as the 27-day ALs in the equatorial belt, but in this
equatorial belt the slowly rotating ALs acts as a trigger mechanism of
greater activity, especially when it crosses the 27-day AL.

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