A Possible Solar Cycle Dependence to the Hemispheric Pattern of Filaments?

Details A Possible Solar Cycle Dependence to the Hemispheric Pattern of Filaments? A Possible Solar Cycle Dependence to the Hemispheric Pattern of Filaments?

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003csss...12..595m&link_type=abstract

The Future of Cool-Star Astrophysics: 12th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (2001 July 30 - August

Astronomy and Astrophysics

Astrophysics

1

Sun, Filament, 3-D Simulations

Scientific paper

The origin of the hemispheric pattern of filaments is considered for both the rising and declining phases of the solar cycle. This is carried out by using a magnetic flux transport model which considers how bipoles interact with surrounding polar fields. For the rising phase of the cycle a range of initial twists and tilt angles of the bipoles consistent with observations can be found which reproduces the observed hemispheric pattern. For the declining phase no such range can be found. To determine whether there is a cycle variation to the hemispheric pattern new detailed observations are required.

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