Project of the Large Solar Telescope with mirror 3 m in diameter

Project of the Large Solar Telescope with mirror 3 m in diameter

One of the most important problems of modern solar physics is the observation of the small-scale structure of the solar atmosphere at various heights (including the chromosphere and corona) in different spectral lines. Such observations can be made only with large solar telescopes whose main mirror...

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Bibliographic Details
Main Authors: Grigoryev V.M., Demidov M.L., Kolobov D.Yu., Pulyaev V.A., Skomorovsky V.I., Chuprakov S.A.
Format: Article
Language:English
Published: INFRA-M 2020-06-01
Series:Solar-Terrestrial Physics
Subjects:
sun
corona
telescope
spatial resolution
magnetic fields
polarization
spectrograph
spectral lines
Online Access:https://naukaru.ru/en/nauka/article/38135/view

Internet

https://naukaru.ru/en/nauka/article/38135/view

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