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Solar EUV flux variations near activity maxima

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Abstract

Data on solar emission variations in the extreme ultraviolet range λ<1300 Å (EUV-range) performed on board the “Prognoz” satellites and the “Phobos” spacecraft by the thermoluminescent method are presented. Flux variations from the 11-years cycle are factors of 2–2.5, and that by the 27-days cycle do not exceed 30%.

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References

  • Arkhangelskaya, V.A. and Razumova, T.K.: 1963,Optics and Spectroscopy (in Russian). Separate issue ‘Luminiscence’, 299.

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Authors and Affiliations

  1. Fedorov Institute of Applied Geophysics, Rostokinskaya, 9, 129226, Moscow, Russia

    T. V. Kazachevskaya, A. I. Lomovsky & A. A. Nusintov

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  1. T. V. Kazachevskaya
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  2. A. I. Lomovsky
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  3. A. A. Nusintov
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Kazachevskaya, T.V., Lomovsky, A.I. & Nusintov, A.A. Solar EUV flux variations near activity maxima. Sol Phys 152, 77–80 (1994). https://doi.org/10.1007/BF01473186

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  • DOI: https://doi.org/10.1007/BF01473186

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