The Coronal Spectrum
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Publisher
Springer Netherlands
Link
http://link.springer.com/content/pdf/10.1007/978-94-010-3587-3_16
Reference43 articles.
1. Aly, M. K., Evans, J. W., and Orrall, F. Q.: 1963, ‘A Photometric Study of the Continuum and Seventeen Emission Lines in the Inner Solar Corona’, Astrophys. J. 136, 956.
2. Billings, D. E.: 1957, ‘Profile of the Yellow Coronal Line’, Astrophys. J. 125, 817.
3. Billings, D. E.: 1959, ‘Velocity Fields in a Coronal Region with a Possible Hydromagnetic Interpretation’, Astrophys. J. 130, 215.
4. Billings, D. E.: 1963, ‘Spectroscopic Limitation on Coronal Heating Mechanisms’, Astrophys. J. 137, 592.
5. Billings, D. E. and Lehman, R. C.: 1962, ‘Line-Width Temperatures of Distinct Coronal Features’, Astrophys. J. 136, 258.
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1. Using Fe X 6374 Å and Fe XIV 5303 Å Spectral line intensities to study the effect of line of sight integration on coronal temperature inferences;Journal of Geophysical Research;1995
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