Spatial Structures of Polar Magnetic Field During the Last Solar Cycle

Details Spatial Structures of Polar Magnetic Field During the Last Solar Cycle Spatial Structures of Polar Magnetic Field During the Last Solar Cycle

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.1103s&link_type=abstract

American Astronomical Society, SPD meeting #40, #11.03; Bulletin of the American Astronomical Society, Vol. 41, p.825

Astronomy and Astrophysics

Astronomy

Scientific paper

The Sun's polar field is closely related to the large scale coronal structure. It is important for coronal modeling and greatly affects the result. However, the polar field is not well observed because the ecliptic lies near the Sun's equator. In this study, we make use of the data from various observatories (MDI/WSO/MWO/Hinode) to study its spatial structures during the last solar cycle. The result is useful to improve the polar field extrapolation schemes.

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