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Photometric intensity and polarization measurements of the solar corona.Use of a satellite photometric observatory (SPO) to measure the solar corona from Miahuatlan, Mexico during the Mar. 7, 1970, total eclipse of the sun. The SPO is equipped with a 24-in. Cassegrainian telescope, a four-channel photoelectric photometer, a Wollaston prism, and a rotating half-wave plate. Simultaneous measurements were made of the two orthogonal components of coronal light in the B and R bands of the UBVRI system. A 1-minute arc aperture was scanned from the lunar disk center out to five solar radii in a series of spirals of gradually increasing radius. For the first time, simultaneous multicolor intensity, degree, and angle of polarization profiles are computed from photoelectric measurements. Comparison of the variations of the measurements for each spiral scan yield a detailed picture of the intensity and polarization features in the K corona.
Document ID
19720045880
Document Type
Reprint (Version printed in journal)
Authors
Mcdougal, D. S. (NASA Langley Research Center Hampton, Va., United States)
Date Acquired
August 6, 2013
Publication Date
December 1, 1971
Subject Category
SPACE SCIENCES
Distribution Limits
Public
Copyright
Other