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Ionization frequencies for major thermospheric constituents as a function of solar cycle 21

Torr, Marsha R., Torr, D. G., Ong, R. A., Hinteregger, H. E.·1979·Geophysical Research Letters

Abstract

Increases in the solar ultraviolet flux (λ < 1250Å) over the past five years of rising solar activity have been larger than anticipated. This increase in UV flux dramatically affects the production of ionization of the various constituents in the thermosphere. In this paper we use measurements of the solar UV flux by the Atmosphere Explorer satellites to determine ionization frequencies for the major thermospheric species for various dates exhibiting notably different levels of solar activity. For the convenience of users of such dataa reduced set of cross section and flux data is presented for the wavelength range below 1027Åcomprising 37 wavelength intervals.

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Metadata

Authors
Torr, M. R., Torr, D. G., Ong, R. A., & Hinteregger, H. E.
Venue
Geophysical Research Letters
Published
1979-10
Volume
6
Issue
10
Pages
771-774
ISSN
  • 0094-8276 (ISSN-L)
  • 1944-8007
OpenAlex
W2012479771
Cited by
349
References
0
FWCI
21.35
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Ionization frequencies for major thermospheric constituents as a function of solar cycle 21. https://app.cochat.ai/papers/10.1029/gl006i010p00771
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Torr, M. R., Torr, D. G., Ong, R. A., & Hinteregger, H. E. (1979). Ionization frequencies for major thermospheric constituents as a function of solar cycle 21. Geophysical Research Letters. https://doi.org/10.1029/gl006i010p00771

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