The Brightness Temperature of the Quiet Solar Chromosphere at 2.6 mm
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/article/10.1007/s11207-016-1044-5/fulltext.html
Reference34 articles.
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2. Bastian, T.S., Dulk, G.A., Leblanc, Y.: 1996, High-resolution microwave observations of the quiet solar chromosphere. Astrophys. J. 473, 539. ADS . DOI .
3. Dulk, G.A.: 1985, Radio emission from the sun and stars. Annu. Rev. Astron. Astrophys. 23, 169. ADS . DOI .
4. De Pontieu, B., Rouppe van der Voort, L., McIntosh, S., Pereira, T.M.D., Carlsson, M., Hansteen, V., et al.: 2014, On the prevalence of small-scale twist in the solar chromosphere and transition region. Science 346, 315. ADS . DOI .
5. Ewell, M.W. Jr., Zirin, H., Jensen, J.B., Bastian, T.S.: 1993, Submillimeter observations of the 1991 July 11 total solar eclipse. Astrophys. J. 403, 426. ADS . DOI .
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