Satellite observation of medium-scale traveling ionospheric disturbances over Syowa Station

P(論文) From March 9,1985 to January 11,1986,428 medium-scale traveling ionospheric disturbances (TID's) were detected at Syowa Station, Antarctica, by means of differential-Doppler measurements with the 150 and 400MHz beacon waves from six NNSS satellites. It is found from statistical analysis t...

Full description

Bibliographic Details
Main Authors: Ogawa, Tadahiko, Igarashi, Kiyoshi, Aikyou, Kazuhiro, Maeno, Hideo
Language:English
Published: National Institute of Polar Research 1988
Subjects:
Online Access:https://nipr.repo.nii.ac.jp/record/4048/files/KJ00000035894.pdf
https://doi.org/10.15094/00004048
https://nipr.repo.nii.ac.jp/records/4048
_version_ 1829311558459588608
author Ogawa, Tadahiko
Igarashi, Kiyoshi
Aikyou, Kazuhiro
Maeno, Hideo
author_facet Ogawa, Tadahiko
Igarashi, Kiyoshi
Aikyou, Kazuhiro
Maeno, Hideo
author_sort Ogawa, Tadahiko
collection National Institute of Polar Research Repository, Japan
description P(論文) From March 9,1985 to January 11,1986,428 medium-scale traveling ionospheric disturbances (TID's) were detected at Syowa Station, Antarctica, by means of differential-Doppler measurements with the 150 and 400MHz beacon waves from six NNSS satellites. It is found from statistical analysis that (1) the medium-scale TID's in the polar regions appear quite often during geomagnetically quiet and moderately disturbed conditions and their occurrence seems not to increase with increasing geomagnetic activity, (2) they attain the maximum activity in winter and the minimum in summer, (3) diurnal variation shows the maximum occurrence around 1400-1600LT with a second maximum around midnight, and (4) most of the medium-scale TID's propagate from south toward the equator. These findings are compared with observations made at midlatitude to find a fairly good consistency between both results. It is pointed out that the gravity waves excited in the mesosphere rather than in the auroral ionosphere play an important role in producing most of the observed medium-scale TID's. departmental bulletin paper
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
geographic Syowa Station
geographic_facet Syowa Station
id ftnipr:oai:nipr.repo.nii.ac.jp:00004048
institution Open Polar
language English
op_collection_id ftnipr
op_doi https://doi.org/10.15094/00004048
op_relation Proceedings of the NIPR Symposium on Upper Atmosphere Physics
1
192
198
AA10756224
https://nipr.repo.nii.ac.jp/record/4048/files/KJ00000035894.pdf
https://doi.org/10.15094/00004048
https://nipr.repo.nii.ac.jp/records/4048
publishDate 1988
publisher National Institute of Polar Research
record_format openpolar
spelling ftnipr:oai:nipr.repo.nii.ac.jp:00004048 2025-04-13T14:08:17+00:00 Satellite observation of medium-scale traveling ionospheric disturbances over Syowa Station Ogawa, Tadahiko Igarashi, Kiyoshi Aikyou, Kazuhiro Maeno, Hideo 1988-02 application/pdf https://nipr.repo.nii.ac.jp/record/4048/files/KJ00000035894.pdf https://doi.org/10.15094/00004048 https://nipr.repo.nii.ac.jp/records/4048 eng eng National Institute of Polar Research Proceedings of the NIPR Symposium on Upper Atmosphere Physics 1 192 198 AA10756224 https://nipr.repo.nii.ac.jp/record/4048/files/KJ00000035894.pdf https://doi.org/10.15094/00004048 https://nipr.repo.nii.ac.jp/records/4048 1988 ftnipr https://doi.org/10.15094/00004048 2025-03-19T10:19:57Z P(論文) From March 9,1985 to January 11,1986,428 medium-scale traveling ionospheric disturbances (TID's) were detected at Syowa Station, Antarctica, by means of differential-Doppler measurements with the 150 and 400MHz beacon waves from six NNSS satellites. It is found from statistical analysis that (1) the medium-scale TID's in the polar regions appear quite often during geomagnetically quiet and moderately disturbed conditions and their occurrence seems not to increase with increasing geomagnetic activity, (2) they attain the maximum activity in winter and the minimum in summer, (3) diurnal variation shows the maximum occurrence around 1400-1600LT with a second maximum around midnight, and (4) most of the medium-scale TID's propagate from south toward the equator. These findings are compared with observations made at midlatitude to find a fairly good consistency between both results. It is pointed out that the gravity waves excited in the mesosphere rather than in the auroral ionosphere play an important role in producing most of the observed medium-scale TID's. departmental bulletin paper Other/Unknown Material Antarc* Antarctica National Institute of Polar Research Repository, Japan Syowa Station
spellingShingle Ogawa, Tadahiko
Igarashi, Kiyoshi
Aikyou, Kazuhiro
Maeno, Hideo
Satellite observation of medium-scale traveling ionospheric disturbances over Syowa Station
title Satellite observation of medium-scale traveling ionospheric disturbances over Syowa Station
title_full Satellite observation of medium-scale traveling ionospheric disturbances over Syowa Station
title_fullStr Satellite observation of medium-scale traveling ionospheric disturbances over Syowa Station
title_full_unstemmed Satellite observation of medium-scale traveling ionospheric disturbances over Syowa Station
title_short Satellite observation of medium-scale traveling ionospheric disturbances over Syowa Station
title_sort satellite observation of medium-scale traveling ionospheric disturbances over syowa station
url https://nipr.repo.nii.ac.jp/record/4048/files/KJ00000035894.pdf
https://doi.org/10.15094/00004048
https://nipr.repo.nii.ac.jp/records/4048