Coordinated Ground-Satellite Observations of VLF Hiss Emissions at Syowa Station : Relationships between Hiss and Aurora
ISIS VLF data were received at Syowa Station, Antarctica in 1976. These data were compared with VLF and auroral data simultaneously observed on the around. In general, hiss and saucer emissions were succesively observed on ISIS 2, when ISIS 2 moved from the polar cap towards the low latitude. It is...
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National Institute of Polar Research
1979
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fttriple:oai:gotriple.eu:oai:doaj.org/article:b9f61c0276884da29c9d091e602ea789 2023-05-15T13:32:28+02:00 Coordinated Ground-Satellite Observations of VLF Hiss Emissions at Syowa Station : Relationships between Hiss and Aurora Kazuo MAKITA Hiroshi FUKUNISHI Takeo YOSHINO 1979-02-01 https://doi.org/10.15094/00008031 https://doaj.org/article/b9f61c0276884da29c9d091e602ea789 en other eng National Institute of Polar Research doi:10.15094/00008031 0085-7289 https://doaj.org/article/b9f61c0276884da29c9d091e602ea789 undefined Antarctic Record, Iss 64, Pp 57-71 (1979) geo Journal Article https://vocabularies.coar-repositories.org/resource_types/c_6501/ 1979 fttriple https://doi.org/10.15094/00008031 2023-01-22T19:29:46Z ISIS VLF data were received at Syowa Station, Antarctica in 1976. These data were compared with VLF and auroral data simultaneously observed on the around. In general, hiss and saucer emissions were succesively observed on ISIS 2, when ISIS 2 moved from the polar cap towards the low latitude. It is found that the geomagnetic field lines through a northernmost auroral arc are located between the occurrence regions of hiss and saucer emissions. It is also found that spectra of hiss emissions observed on the ground (Syowa) are not similar to those of VLF emissions observed in the region connected with field line at the satel-lite altitude, but are similar to those of VLF emissions observed near the same geomagnetlc latitude as that of Syowa Station. The result suggests that auroral hiss emissions do not propagate along the geomagnetic field lines from the statellite height (~1400 km) to the ground. The calculation by means of the ray theory suggests that hiss emissions propagate along a non-ducted path from the satellite height to the ground Article in Journal/Newspaper Antarc* Antarctica Unknown Syowa Station |
institution |
Open Polar |
collection |
Unknown |
op_collection_id |
fttriple |
language |
English |
topic |
geo |
spellingShingle |
geo Kazuo MAKITA Hiroshi FUKUNISHI Takeo YOSHINO Coordinated Ground-Satellite Observations of VLF Hiss Emissions at Syowa Station : Relationships between Hiss and Aurora |
topic_facet |
geo |
description |
ISIS VLF data were received at Syowa Station, Antarctica in 1976. These data were compared with VLF and auroral data simultaneously observed on the around. In general, hiss and saucer emissions were succesively observed on ISIS 2, when ISIS 2 moved from the polar cap towards the low latitude. It is found that the geomagnetic field lines through a northernmost auroral arc are located between the occurrence regions of hiss and saucer emissions. It is also found that spectra of hiss emissions observed on the ground (Syowa) are not similar to those of VLF emissions observed in the region connected with field line at the satel-lite altitude, but are similar to those of VLF emissions observed near the same geomagnetlc latitude as that of Syowa Station. The result suggests that auroral hiss emissions do not propagate along the geomagnetic field lines from the statellite height (~1400 km) to the ground. The calculation by means of the ray theory suggests that hiss emissions propagate along a non-ducted path from the satellite height to the ground |
format |
Article in Journal/Newspaper |
author |
Kazuo MAKITA Hiroshi FUKUNISHI Takeo YOSHINO |
author_facet |
Kazuo MAKITA Hiroshi FUKUNISHI Takeo YOSHINO |
author_sort |
Kazuo MAKITA |
title |
Coordinated Ground-Satellite Observations of VLF Hiss Emissions at Syowa Station : Relationships between Hiss and Aurora |
title_short |
Coordinated Ground-Satellite Observations of VLF Hiss Emissions at Syowa Station : Relationships between Hiss and Aurora |
title_full |
Coordinated Ground-Satellite Observations of VLF Hiss Emissions at Syowa Station : Relationships between Hiss and Aurora |
title_fullStr |
Coordinated Ground-Satellite Observations of VLF Hiss Emissions at Syowa Station : Relationships between Hiss and Aurora |
title_full_unstemmed |
Coordinated Ground-Satellite Observations of VLF Hiss Emissions at Syowa Station : Relationships between Hiss and Aurora |
title_sort |
coordinated ground-satellite observations of vlf hiss emissions at syowa station : relationships between hiss and aurora |
publisher |
National Institute of Polar Research |
publishDate |
1979 |
url |
https://doi.org/10.15094/00008031 https://doaj.org/article/b9f61c0276884da29c9d091e602ea789 |
geographic |
Syowa Station |
geographic_facet |
Syowa Station |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_source |
Antarctic Record, Iss 64, Pp 57-71 (1979) |
op_relation |
doi:10.15094/00008031 0085-7289 https://doaj.org/article/b9f61c0276884da29c9d091e602ea789 |
op_rights |
undefined |
op_doi |
https://doi.org/10.15094/00008031 |
_version_ |
1766027273671016448 |