Abstract
The observed emission of solar radio waves, X-rays, and energetic particles indicate that processes involving great energies may develop in certain parts of the sun which we identify as the corona. Although radio quanta from the sun have small energies, the circumstances under which they are emitted indicate that they are produced by processes involving great energies and — often — energetic particles.
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de Jager, C. (1965). Radio and X-Ray Emission Associated with Solar Flares. In: Ortner, J., Maseland, H. (eds) Introduction to Solar Terrestrial Relations. Astrophysics and Space Science Library, vol 2. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3590-3_6
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DOI: https://doi.org/10.1007/978-94-010-3590-3_6
Publisher Name: Springer, Dordrecht
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