Using Imaging Infrared Coronal Spectropolarimetry to Measure the Near-Sun Plasma

Details Using Imaging Infrared Coronal Spectropolarimetry to Measure the Near-Sun Plasma Using Imaging Infrared Coronal Spectropolarimetry to Measure the Near-Sun Plasma

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsh44a..08k&link_type=abstract

American Geophysical Union, Fall Meeting 2005, abstract #SH44A-08

Physics

2144 Interstellar Gas, 7509 Corona, 7524 Magnetic Fields, 7599 General Or Miscellaneous

Scientific paper

A moderate aperture ground-based coronagraph and an imaging infrared spectropolarimeter have provided our first direct longitudinal coronal magnetograms. This talk will describe the advantages and subtleties of these techniques for direct coronal magnetometry. We also summarize some of the diagnostic potential of current and likely future IR spectropolarimetric instruments (like the Advanced Technology Solar Telescope) for measuring the properties of the near-solar plasma.

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