Seasonal variation in the latitude of geomagnetically conjugate points observed with imaging riometers in the auroral zone

Seasonal variation in the latitude of geomagnetically conjugate point was obtained statistically using the imaging riometers at Syowa-Tjornes conjugate pair stations. The conjugate point was evaluated experimentally from the relative location of band-type CNA (Cosmic Noise Absorption) appearing at t...

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Main Authors: Yuiti Fujita, Hisao Yamagishi, Natsuo Sato
Format: Article in Journal/Newspaper
Language:English
Japanese
Published: National Institute of Polar Research 1998
Subjects:
Online Access:https://doi.org/10.15094/00009026
https://doaj.org/article/6f9ff90c2c7c4c71ac109ac44ada4224
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spelling ftdoajarticles:oai:doaj.org/article:6f9ff90c2c7c4c71ac109ac44ada4224 2023-05-15T16:50:45+02:00 Seasonal variation in the latitude of geomagnetically conjugate points observed with imaging riometers in the auroral zone Yuiti Fujita Hisao Yamagishi Natsuo Sato 1998-03-01T00:00:00Z https://doi.org/10.15094/00009026 https://doaj.org/article/6f9ff90c2c7c4c71ac109ac44ada4224 EN JA eng jpn National Institute of Polar Research http://doi.org/10.15094/00009026 https://doaj.org/toc/0085-7289 https://doaj.org/toc/2432-079X doi:10.15094/00009026 0085-7289 2432-079X https://doaj.org/article/6f9ff90c2c7c4c71ac109ac44ada4224 Antarctic Record, Vol 42, Iss 1, Pp 1-19 (1998) Geography (General) G1-922 article 1998 ftdoajarticles https://doi.org/10.15094/00009026 2022-12-31T04:12:48Z Seasonal variation in the latitude of geomagnetically conjugate point was obtained statistically using the imaging riometers at Syowa-Tjornes conjugate pair stations. The conjugate point was evaluated experimentally from the relative location of band-type CNA (Cosmic Noise Absorption) appearing at the conjugate stations, associated with auroral breakups in premidnight hours. The statistical analyses were made for poleward moving CNA-bands observed during February 1992 to December 1993. Following characteristics are obtained. (1) The poleward expanding speed of the CNA-bands differs significantly between the two hemispheres : it is faster at Syowa than Tjornes in Iceland by 15% on average. This difference may be attributable to an interhemispherical asymmetry of the magnetic flux tube radii mapped to the ionospheres, which is caused by the differences in the geomagnetic field strength and dip angles between the both stations. (2) The conjugate point of Syowa mapped to the northern hemisphere moves most equatorward in June and most poleward in December from Tjornes. The latitudinal range of the seasonal displacement is about 200km for the average geomagnetic activities of Kp=4. (3) The seasonal displacement agrees well with the calculations of the conjugate points using the combination of IGRF 1995 and Tsyganenko 1989 geomagnetic field models. Article in Journal/Newspaper Iceland Directory of Open Access Journals: DOAJ Articles
institution Open Polar
collection Directory of Open Access Journals: DOAJ Articles
op_collection_id ftdoajarticles
language English
Japanese
topic Geography (General)
G1-922
spellingShingle Geography (General)
G1-922
Yuiti Fujita
Hisao Yamagishi
Natsuo Sato
Seasonal variation in the latitude of geomagnetically conjugate points observed with imaging riometers in the auroral zone
topic_facet Geography (General)
G1-922
description Seasonal variation in the latitude of geomagnetically conjugate point was obtained statistically using the imaging riometers at Syowa-Tjornes conjugate pair stations. The conjugate point was evaluated experimentally from the relative location of band-type CNA (Cosmic Noise Absorption) appearing at the conjugate stations, associated with auroral breakups in premidnight hours. The statistical analyses were made for poleward moving CNA-bands observed during February 1992 to December 1993. Following characteristics are obtained. (1) The poleward expanding speed of the CNA-bands differs significantly between the two hemispheres : it is faster at Syowa than Tjornes in Iceland by 15% on average. This difference may be attributable to an interhemispherical asymmetry of the magnetic flux tube radii mapped to the ionospheres, which is caused by the differences in the geomagnetic field strength and dip angles between the both stations. (2) The conjugate point of Syowa mapped to the northern hemisphere moves most equatorward in June and most poleward in December from Tjornes. The latitudinal range of the seasonal displacement is about 200km for the average geomagnetic activities of Kp=4. (3) The seasonal displacement agrees well with the calculations of the conjugate points using the combination of IGRF 1995 and Tsyganenko 1989 geomagnetic field models.
format Article in Journal/Newspaper
author Yuiti Fujita
Hisao Yamagishi
Natsuo Sato
author_facet Yuiti Fujita
Hisao Yamagishi
Natsuo Sato
author_sort Yuiti Fujita
title Seasonal variation in the latitude of geomagnetically conjugate points observed with imaging riometers in the auroral zone
title_short Seasonal variation in the latitude of geomagnetically conjugate points observed with imaging riometers in the auroral zone
title_full Seasonal variation in the latitude of geomagnetically conjugate points observed with imaging riometers in the auroral zone
title_fullStr Seasonal variation in the latitude of geomagnetically conjugate points observed with imaging riometers in the auroral zone
title_full_unstemmed Seasonal variation in the latitude of geomagnetically conjugate points observed with imaging riometers in the auroral zone
title_sort seasonal variation in the latitude of geomagnetically conjugate points observed with imaging riometers in the auroral zone
publisher National Institute of Polar Research
publishDate 1998
url https://doi.org/10.15094/00009026
https://doaj.org/article/6f9ff90c2c7c4c71ac109ac44ada4224
genre Iceland
genre_facet Iceland
op_source Antarctic Record, Vol 42, Iss 1, Pp 1-19 (1998)
op_relation http://doi.org/10.15094/00009026
https://doaj.org/toc/0085-7289
https://doaj.org/toc/2432-079X
doi:10.15094/00009026
0085-7289
2432-079X
https://doaj.org/article/6f9ff90c2c7c4c71ac109ac44ada4224
op_doi https://doi.org/10.15094/00009026
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