Characteristics of Radio Aurora Occurrences Observed at Syowa Station in Antarctica
Radio aurora occurrences on 112 MHz observed for nearly one year from April 1970 till February 1971 at Syowa Station the Antarctic were analized. Results obtained are summarized as follows: 1) The diurnal variation in the frequency of the radio echo occurrence correlates well with the magnetic Q-ind...
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Format: | Article in Journal/Newspaper |
Language: | English |
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National Institute of Polar Research
1973
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Subjects: | |
Online Access: | https://doi.org/10.15094/00007717 https://doaj.org/article/ab99f751f40e45e7844e362dbfcccaf5 |
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author | Isao SHIRO Toshirou SAKAMOTO |
author_facet | Isao SHIRO Toshirou SAKAMOTO |
author_sort | Isao SHIRO |
collection | Unknown |
description | Radio aurora occurrences on 112 MHz observed for nearly one year from April 1970 till February 1971 at Syowa Station the Antarctic were analized. Results obtained are summarized as follows: 1) The diurnal variation in the frequency of the radio echo occurrence correlates well with the magnetic Q-index. 2) The frequency of their occurrence in the morning sequence correlates comparatively well with absorption of the cosmic radio noise recorded by the riometer, but no definite relation is found in the evening sequence. 3) Most echoes in the dark winter have discrete structures, while those in the sunlit summer are characterized by diffuse ones. 4) The reflected echoes are generally weaker in the winter than in the summer. 5) The echoes in the winter are confined within the range from 300 to 400 km, while the range of those in the summer extends from 300 to 1100 km. 6) Radio auroras move northward in the morning and southward in the evening, at a speed of 500~600 m/s. |
format | Article in Journal/Newspaper |
genre | Antarc* Antarctic Antarctica |
genre_facet | Antarc* Antarctic Antarctica |
geographic | Antarctic The Antarctic Syowa Station |
geographic_facet | Antarctic The Antarctic Syowa Station |
id | fttriple:oai:gotriple.eu:oai:doaj.org/article:ab99f751f40e45e7844e362dbfcccaf5 |
institution | Open Polar |
language | English |
op_collection_id | fttriple |
op_doi | https://doi.org/10.15094/00007717 |
op_relation | doi:10.15094/00007717 0085-7289 2432-079X https://doaj.org/article/ab99f751f40e45e7844e362dbfcccaf5 |
op_rights | undefined |
op_source | Antarctic Record, Iss 47, Pp 46-61 (1973) |
publishDate | 1973 |
publisher | National Institute of Polar Research |
record_format | openpolar |
spelling | fttriple:oai:gotriple.eu:oai:doaj.org/article:ab99f751f40e45e7844e362dbfcccaf5 2025-01-16T19:21:06+00:00 Characteristics of Radio Aurora Occurrences Observed at Syowa Station in Antarctica Isao SHIRO Toshirou SAKAMOTO 1973-09-01 https://doi.org/10.15094/00007717 https://doaj.org/article/ab99f751f40e45e7844e362dbfcccaf5 en other eng National Institute of Polar Research doi:10.15094/00007717 0085-7289 2432-079X https://doaj.org/article/ab99f751f40e45e7844e362dbfcccaf5 undefined Antarctic Record, Iss 47, Pp 46-61 (1973) geo Journal Article https://vocabularies.coar-repositories.org/resource_types/c_6501/ 1973 fttriple https://doi.org/10.15094/00007717 2023-01-22T18:48:00Z Radio aurora occurrences on 112 MHz observed for nearly one year from April 1970 till February 1971 at Syowa Station the Antarctic were analized. Results obtained are summarized as follows: 1) The diurnal variation in the frequency of the radio echo occurrence correlates well with the magnetic Q-index. 2) The frequency of their occurrence in the morning sequence correlates comparatively well with absorption of the cosmic radio noise recorded by the riometer, but no definite relation is found in the evening sequence. 3) Most echoes in the dark winter have discrete structures, while those in the sunlit summer are characterized by diffuse ones. 4) The reflected echoes are generally weaker in the winter than in the summer. 5) The echoes in the winter are confined within the range from 300 to 400 km, while the range of those in the summer extends from 300 to 1100 km. 6) Radio auroras move northward in the morning and southward in the evening, at a speed of 500~600 m/s. Article in Journal/Newspaper Antarc* Antarctic Antarctica Unknown Antarctic The Antarctic Syowa Station |
spellingShingle | geo Isao SHIRO Toshirou SAKAMOTO Characteristics of Radio Aurora Occurrences Observed at Syowa Station in Antarctica |
title | Characteristics of Radio Aurora Occurrences Observed at Syowa Station in Antarctica |
title_full | Characteristics of Radio Aurora Occurrences Observed at Syowa Station in Antarctica |
title_fullStr | Characteristics of Radio Aurora Occurrences Observed at Syowa Station in Antarctica |
title_full_unstemmed | Characteristics of Radio Aurora Occurrences Observed at Syowa Station in Antarctica |
title_short | Characteristics of Radio Aurora Occurrences Observed at Syowa Station in Antarctica |
title_sort | characteristics of radio aurora occurrences observed at syowa station in antarctica |
topic | geo |
topic_facet | geo |
url | https://doi.org/10.15094/00007717 https://doaj.org/article/ab99f751f40e45e7844e362dbfcccaf5 |