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Potential IR Observations of the Solar Corona

Published online by Cambridge University Press:  03 August 2017

C. Krishna Kumar  and
Joseph Davila
C. Krishna Kumar
Affiliation:
Department of Astronomy, Howard University, Washington, DC 20059, U.S.A.
Joseph Davila
Affiliation:
Code 682, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A.

Abstract

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We examine the potential for observations of the solar corona using forbidden lines in the near infrared.

Keywords

infrared: starsSun: corona
Type
Part 1: Infrared Diagnostics of the Solar Atmosphere and Solar Activity
Information
Symposium - International Astronomical Union , Volume 154: Infrared Solar Physics , 1994 , pp. 81 - 84
Copyright
Copyright © Kluwer 1994 

References

Chocol, D., Rušin, V., Kulcar, L., and Vanysek, V.: 1983, Astrophys. and Sp. Sci. 91, 71.CrossRefGoogle Scholar
Macqueen, R.M.: 1968, Ap.J. 154, 1062.Google Scholar
Macqueen, R.M., and St. Cyr, O.C.: 1991, Icarus 90, 96.Google Scholar
Mangus, J., and Stockhausen, R.: 1966, NASA Rept. X-614-66-29.Google Scholar
Münch, G., Neugebauer, G., and McCammon, D.: 1967 Astrophys. J. 149, 681.Google Scholar
Sheeley, N.R., Howard, R.A., Koomen, M.J., and Michels, D.J.: 1982, Nature, 300, 239.Google Scholar
Newkirk, G. and Eddy, J.: 1964 J. Atmos. Phys., 21, 34.Google Scholar