Diagnostics of Subphotospheric Sources of Solar Variability

Details Diagnostics of Subphotospheric Sources of Solar Variability Diagnostics of Subphotospheric Sources of Solar Variability

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsh13a1144k&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #SH13A-1144

Physics

7519 Flares, 7522 Helioseismology, 7537 Solar And Stellar Variability, 7544 Stellar Interiors And Dynamo Theory

Scientific paper

Local helioseismology provides new tools for studying subphotospheric processes that are related to solar variability of various spatial and temporal scales. Large-scale flow patterns beneath active regions and sunspots affect the solar energy transport in the upper convection zone. Smaller-scale shearing and twisting flows may trigger instabilities of magnetic configurations that lead to flares and CMEs. We discuss the recent progress in the local helioseismology diagnostic tools and in our understanding of the subphotospheric dynamics and sources of variability.

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