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Radio Emission of Rydberg Atoms in the Upper Atmosphere Modified by High-Power HF Radio Waves

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dc.contributor.author Troitskii A.V.
dc.contributor.author Frolov V.L.
dc.contributor.author Vostokov A.V.
dc.contributor.author Rakut’ I.V.
dc.date.accessioned 2021-02-24T20:33:31Z
dc.date.available 2021-02-24T20:33:31Z
dc.date.issued 2020
dc.identifier.issn 0033-8443
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/160892
dc.description.abstract © 2020, Springer Science+Business Media, LLC, part of Springer Nature. We report on the results of studying the radio emission of the Rydberg states of atoms and molecules in the Earth’s upper atmosphere at ionospheric altitudes when the ionosphere is modified by high-power HF radio waves radiated by the Sura heating facility. Radio emission from the upper atmosphere, caused by the emission of highly excited Rydberg atoms and molecules with the principal quantum number n = 163–169 and n = 225 (decimeter wavelength range) and two spectral features that coincide with the frequencies of transitions between Rydberg states m = 169 → n = 168 with the transition frequency νn = 1375.35 MHz and m = 166 → n = 165 with νn = 1451.5 MHz were detected. Characteristic altitudes of the Rydberg radiation generation region were 150–250 km. The radio emission intensity corresponds to 10–45 K, which is comparable with the intensity of the radio emission generated during solar flares.
dc.relation.ispartofseries Radiophysics and Quantum Electronics
dc.title Radio Emission of Rydberg Atoms in the Upper Atmosphere Modified by High-Power HF Radio Waves
dc.type Article
dc.relation.ispartofseries-issue 10
dc.relation.ispartofseries-volume 62
dc.collection Публикации сотрудников КФУ
dc.relation.startpage 677
dc.source.id SCOPUS00338443-2020-62-10-SID85086086633


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  • Публикации сотрудников КФУ Scopus [24551]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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