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Published September 1967 | Published
Journal Article Open

Infrared Coronal Lines. II. Observation of [SI x] λ 1.43 μ and [Mg VIII] λ 3.03 μ

Abstract

The wavelengths and intensities of the coronal lines of the ions Si^(9+) and Mg^(8+), resulting from the airborne observation of the November 12, 1966, total solar eclipse, are given.

Additional Information

© 1967 American Astronomical Society. Received February 28, 1967. The co-operation and help given to us by the personnel of the NASA Ames Research Center associated with the eclipse expedition are gratefully acknowledged. Our indebtedness is also due to Dr. R. Stockhausen of the NASA Goddard Space Flight Center for the loan of the CaF2 window. The preparation of the instrument package could not have been completed without the able assistance of Mr. David Vail, of the Physics Department, California Institute of Technology. This work has been in part supported by the National Aeronautics and Space Administration, under grant NsG-426 to the California Institute of Technology.

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Published - 1967ApJ___149__681M.pdf

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August 19, 2023
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October 24, 2023