Diagnosing the Prominence-Cavity Connection

Details Diagnosing the Prominence-Cavity Connection Diagnosing the Prominence-Cavity Connection

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsh43b1947s&link_type=abstract

American Geophysical Union, Fall Meeting 2011, abstract #SH43B-1947

Astronomy and Astrophysics

Astrophysics

[7524] Solar Physics, Astrophysics, And Astronomy / Magnetic Fields, [7549] Solar Physics, Astrophysics, And Astronomy / Ultraviolet Emissions

Scientific paper

The magnetic field is thought to play a central role in both the support of prominence plasma as well as the thermodynamic isolation of the surrounding cavity. We use the statistical goldmine of the SDO/AIA dataset to probe for the first time the dynamical link between these related structures. These observations are compared to the 3D magnetic geometries predicted by MHD models. The dynamic features are explained within the context of 1D field-aligned momentum and energy imbalance.

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