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

Münch, G. and Neugebauer, G. and McCammon, D. (1967) Infrared Coronal Lines. II. Observation of [SI x] λ 1.43 μ and [Mg VIII] λ 3.03 μ. Astrophysical Journal, 149 . pp. 681-686. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20170303-104230736

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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.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/149297DOIArticle
http://adsabs.harvard.edu/abs/1967ApJ...149..681MADSArticle
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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NASANsG-426
Record Number:CaltechAUTHORS:20170303-104230736
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170303-104230736
Official Citation:Infrared Coronal Lines. II. Observation of [SI x] λ 1.43 μ and [Mg VIII] λ 3.03 µm Münch, G., Neugebauer, G., & McCammon, D. Astrophysical Journal, vol. 149, p.681
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:74692
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:03 Mar 2017 20:42
Last Modified:03 Mar 2017 20:42

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