A detection of the $2^{2}P_{3/2}-2^{2}S_{1/2}$ fine-structure transition of hydrogen in the radio spectrum of the Sun?
Author:
Funder
Magnus Ehrnroothin Säätiö
Publisher
Springer Science and Business Media LLC
Link
https://link.springer.com/content/pdf/10.1007/s10509-024-04349-9.pdf
Reference21 articles.
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4. Ayres, T.R., Plymate, C., Keller, C.U.: Solar carbon monoxide, thermal profiling, and the abundances of C, O, and their isotopes. Astrophys. J. Suppl. Ser. 165(2), 618–651 (2006). https://doi.org/10.1086/504847. arXiv:astro-ph/0606153 [astro-ph]
5. Carlsson, M., Stein, R.F.: Does a nonmagnetic solar chromosphere exist? Astrophys. J. Lett. 440, L29 (1995). https://doi.org/10.1086/187753. arXiv:astro-ph/9411036 [astro-ph]
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