Characterizing and Modeling Magnetic Flux Transport in the Sun's Photosphere and Determining Its Impact on the Sunspot Cycle
Characterization and modeling magnetic flux transport within the surface layers of the Sun are vital to explaining the 11 year sunspot cycle. I have characterized the differential rotation (DR) and meridional flow (MF) and their variations since 1996 using a cross-correlation technique on magnetogra...
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| Format: | Others |
| Language: | en |
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VANDERBILT
2014
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| Online Access: | http://etd.library.vanderbilt.edu/available/etd-03212014-134603/ |