Physics – Optics
Scientific paper
Jan 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992spie.1546..402f&link_type=abstract
In: Multilayer and grazing incidence X-ray/EUV optics; Proceedings of the Meeting, San Diego, CA, July 22-24, 1991 (A93-39658 15
Physics
Optics
2
Coronagraphs, H Alpha Line, Lyman Alpha Radiation, Polarimeters, Solar Corona, Emission Spectra, Linear Polarization, Solar Atmosphere, Solar Magnetic Field
Scientific paper
The present treatment of vector magnetic field measurement in coronas by means of the Hanle effect of the Lyman-alpha line uses data from all-reflecting imaging coronagraph/polarimeters. The polarization sensitivity, bandpass, and spatial resolution of these instruments are defined through a modeling of the Hanle-effect signature in Lyman-alpha emission from coronal magnetic loops; the line-of-sight integration through an inhomogeneous coronal medium is taken into account. The use of the Hanle effect to measure solar corona vector magnetic fields is verified.
Fineschi Silvano
Hoover Richard B.
Walker Arthur B. C. Jr.
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