Changes of the first Schumann resonance frequency during relativistic solar proton precipitation in the 6 November 1997 event
The variations of the first mode of Schumann resonance are analyzed using data from Kola peninsula stations during the solar proton event of 6 November 1997. On this day the intensive flux of energetic protons on GOES-8 and the 10% increase of the count rate of the neutron monitor in Apatity between...
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ftcopernicus:oai:publications.copernicus.org:angeo34478 2023-05-15T17:04:57+02:00 Changes of the first Schumann resonance frequency during relativistic solar proton precipitation in the 6 November 1997 event Roldugin, V. C. Maltsev, Ye. P. Vasiljev, A. N. Vashenyuk, E. V. 2018-09-27 application/pdf https://doi.org/10.1007/s00585-999-1293-9 https://angeo.copernicus.org/articles/17/1293/1999/ eng eng doi:10.1007/s00585-999-1293-9 https://angeo.copernicus.org/articles/17/1293/1999/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.1007/s00585-999-1293-9 2020-07-20T16:28:02Z The variations of the first mode of Schumann resonance are analyzed using data from Kola peninsula stations during the solar proton event of 6 November 1997. On this day the intensive flux of energetic protons on GOES-8 and the 10% increase of the count rate of the neutron monitor in Apatity between 1220 and 2000 UT were preceded by a solar X-ray burst at 1155 UT. This burst was accompanied by a simultaneous increase of the Schumann frequency by 3.5%, and the relativistic proton flux increase was accompanied by 1% frequency decrease. These effects are explained by changes of the height and dielectric permeability of the Earth-ionosphere cavity. Key words. Ionosphere (ionospheric disturbances; solar radiation and cosmic ray effects) · Radio science (ionospheric propagation) Text kola peninsula Copernicus Publications: E-Journals Apatity ENVELOPE(33.403,33.403,67.564,67.564) Kola Peninsula Schumann ENVELOPE(-73.691,-73.691,-71.641,-71.641) Annales Geophysicae 17 10 1293 1297 |
institution |
Open Polar |
collection |
Copernicus Publications: E-Journals |
op_collection_id |
ftcopernicus |
language |
English |
description |
The variations of the first mode of Schumann resonance are analyzed using data from Kola peninsula stations during the solar proton event of 6 November 1997. On this day the intensive flux of energetic protons on GOES-8 and the 10% increase of the count rate of the neutron monitor in Apatity between 1220 and 2000 UT were preceded by a solar X-ray burst at 1155 UT. This burst was accompanied by a simultaneous increase of the Schumann frequency by 3.5%, and the relativistic proton flux increase was accompanied by 1% frequency decrease. These effects are explained by changes of the height and dielectric permeability of the Earth-ionosphere cavity. Key words. Ionosphere (ionospheric disturbances; solar radiation and cosmic ray effects) · Radio science (ionospheric propagation) |
format |
Text |
author |
Roldugin, V. C. Maltsev, Ye. P. Vasiljev, A. N. Vashenyuk, E. V. |
spellingShingle |
Roldugin, V. C. Maltsev, Ye. P. Vasiljev, A. N. Vashenyuk, E. V. Changes of the first Schumann resonance frequency during relativistic solar proton precipitation in the 6 November 1997 event |
author_facet |
Roldugin, V. C. Maltsev, Ye. P. Vasiljev, A. N. Vashenyuk, E. V. |
author_sort |
Roldugin, V. C. |
title |
Changes of the first Schumann resonance frequency during relativistic solar proton precipitation in the 6 November 1997 event |
title_short |
Changes of the first Schumann resonance frequency during relativistic solar proton precipitation in the 6 November 1997 event |
title_full |
Changes of the first Schumann resonance frequency during relativistic solar proton precipitation in the 6 November 1997 event |
title_fullStr |
Changes of the first Schumann resonance frequency during relativistic solar proton precipitation in the 6 November 1997 event |
title_full_unstemmed |
Changes of the first Schumann resonance frequency during relativistic solar proton precipitation in the 6 November 1997 event |
title_sort |
changes of the first schumann resonance frequency during relativistic solar proton precipitation in the 6 november 1997 event |
publishDate |
2018 |
url |
https://doi.org/10.1007/s00585-999-1293-9 https://angeo.copernicus.org/articles/17/1293/1999/ |
long_lat |
ENVELOPE(33.403,33.403,67.564,67.564) ENVELOPE(-73.691,-73.691,-71.641,-71.641) |
geographic |
Apatity Kola Peninsula Schumann |
geographic_facet |
Apatity Kola Peninsula Schumann |
genre |
kola peninsula |
genre_facet |
kola peninsula |
op_source |
eISSN: 1432-0576 |
op_relation |
doi:10.1007/s00585-999-1293-9 https://angeo.copernicus.org/articles/17/1293/1999/ |
op_doi |
https://doi.org/10.1007/s00585-999-1293-9 |
container_title |
Annales Geophysicae |
container_volume |
17 |
container_issue |
10 |
container_start_page |
1293 |
op_container_end_page |
1297 |
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1766059311380824064 |