Searching for Moving Magnetic Features at 1565 nm

Details Searching for Moving Magnetic Features at 1565 nm Searching for Moving Magnetic Features at 1565 nm

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp41b..01j&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SP41B-01

Physics

7524 Magnetic Fields, 7529 Photosphere

Scientific paper

Spectropolarimetric data of the active region 10663 was taken with the CSUN-NSO IR camera and the McMath-Pierce telescope on August 26, 2004 from 16:35 to 21:02 UT. Utilizing the Zeeman split Fe I line near 1565 nm, the data is processed to remove instrumental polarization and a Milne-Eddington inversion technique is applied. The results of the inversion are used to examine the physical properties and radial motions of moving magnetic features which appear to originate in the sunspot penumbra.

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