Multiresolution Analysis of Synoptic Solar Magnetic Fields

Details Multiresolution Analysis of Synoptic Solar Magnetic Fields Multiresolution Analysis of Synoptic Solar Magnetic Fields

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsh11a0243l&link_type=abstract

American Geophysical Union, Fall Meeting 2005, abstract #SH11A-0243

Physics

3280 Wavelet Transform (3255, 4455), 7524 Magnetic Fields, 7529 Photosphere, 7536 Solar Activity Cycle (2162)

Scientific paper

Solar synoptic maps provide an important visualization of global patterns. Maps are available of sub-surface flows, photospheric and coronal magnetic fields. We have carried out a multiresolution analysis of averaged synoptic magnetograms. Every synoptic map was averaged in longitude resulting in a column of 180 latitude values for each Carrington Rotation. The study covered Carrington rotations 1625 through 2030 or the period 1975 up to 2005. We performed a multilevel wavelet decomposition of the solar magnetic field signal for each latitude. Trends, periods and transients in the decomposed signal are discussed.

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