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Proceedings Paper

Hydrogen Lyman α coronagraph/polarimeter
Author(s): Silvano Fineschi; Richard B. Hoover; Arthur B. C. Walker
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Paper Abstract

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.

Paper Details

Date Published: 1 January 1992
PDF: 12 pages
Proc. SPIE 1546, Multilayer and Grazing Incidence X-Ray/EUV Optics, (1 January 1992); doi: 10.1117/12.51238
Show Author Affiliations
Silvano Fineschi, NASA/Marshall Space Flight Ctr. (United States)
Richard B. Hoover, NASA/Marshall Space Flight Ctr. (United States)
Arthur B. C. Walker, Stanford Univ. (United States)

Published in SPIE Proceedings Vol. 1546:
Multilayer and Grazing Incidence X-Ray/EUV Optics
Richard B. Hoover, Editor(s)

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