A method for investigating the brightness distribution near the solar limb at millimeter wavelengths
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/BF00162423.pdf
Reference6 articles.
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2. Flett, A. M., Foster, P. R., Strachan, P., and Thornton, D. C.: 1971, Solar Phys. 20, 317.
3. Gary, B., Stacey, J., and Drake, F. D.: 1965, Astrophys. J. Suppl. 12, 239.
4. Noyes, R. W., Beckers, J. M., and Low, F. J.: 1968, Solar Phys. 3, 36.
5. Simon, M., Buhl, D., Cogdell, J. R., Shimabukuro, F. I., and Zapata, C.: 1970, Nature 226, 1154.
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1. Temporal and angular variation of the solar limb brightening at 17 GHz;Astronomy & Astrophysics;2003-04
2. Probing the Solar Atmosphere Through Radiophysics;Theoretical and Observational Problems Related to Solar Eclipses;1997
3. The Quiet Sun at cm- and mm-Wavelengths;Symposium - International Astronomical Union;1980
4. The Quiet Sun at cm- and mm-Wavelengths;Radio Physics of the Sun;1980
5. Interferometer observations of the solar brightness distribution at 8.6 mm wavelength;Solar Physics;1976-01
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