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On magnetic measurements in prominences
Published online by Cambridge University Press: 06 January 2014
Abstract
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The successes of magnetic measurements in faint objects located near very bright ones are strongly depending on the stray light in the telescope. We propose a mask with a variable transmission placed on the primary optics of a telescope. Our computations of the stray light in such a telescope indicate that the calculated coronagraphic factor of improvement, K, would increase at least by 2 orders of magnitude compared to the Lyot-type coronagraph.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 426 - 427
- Copyright
- Copyright © International Astronomical Union 2013
References
Kim, I. S., Bugaenko, O. I., & Bruevich, V. V. and Evseev, O. A., 1995, Bull. of Rus. Acad. of Sci., 59, 153.Google Scholar
Kim, I. S, Alexeeva, I. V, & Suyunova, E. Z., 2012, ASP Conference Series, Rimmele, T. R., Collados Vera, M.et al., eds, Vol. 463, 337.Google Scholar
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