Multi-wavelength Comparison of Prominence Cavities

Details Multi-wavelength Comparison of Prominence Cavities Multi-wavelength Comparison of Prominence Cavities

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsp43b..04s&link_type=abstract

American Geophysical Union, Spring Meeting 2008, abstract #SP43B-04

Physics

7509 Corona

Scientific paper

Recent observational campaigns have brought together a wealth of data specifically designed to explore the physical properties and dynamics of prominence cavities. In particular, STEREO and Hinode data have provided new perspectives on these structures. In order to effectively analyze the data in a cohesive manner, we produce overlays of several distinct and complimentary datasets including SOHO UVCS, CDS, and EIT, Hinode SOT and EIS, STEREO SECCHI, TRACE, and Nancay Radioheliograph data as well as new observations of coronal magnetic fields in cavities from the Coronal Multichannel Polarimeter. We are thus able to investigate how sensitive morphology is to the wavelength observed which details the nature of the plasma in the cavity.

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