Active Region Dynamics |
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Authors: | A G Kosovichev T L Duvall Jr |
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Institution: | (1) Stanford University, Stanford, CA 94305, USA;(2) Laboratory for Astronomy and Solar Physics, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA |
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Abstract: | New methods of local helioseismology and uninterrupted time series of solar oscillation data from the Solar and Heliospheric
Observatory (SOHO) have led to a major advance in our understanding of the structure and dynamics of active regions in the
subsurface layers. The initial results show that large active regions are formed by repeated magnetic flux emergence from
the deep interior, and that their roots are at least 50 Mm deep. The active regions change the temperature structure and flow
dynamics of the upper convection zone, forming large circulation cells of converging flows. The helioseismic observations
also indicate that the processes of magnetic energy release, flares and coronal mass ejections, might be associated with strong
(1–2 km/s) shearing flows, 4–6 Mm below the surface. |
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Keywords: | Sun: activity Sun: heliseismology Sun: interior Sun: magnetic field sunspots |
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