Observation of the upper atmosphere physics at Asuka Station by the 30th Japanese Antarctic Research Expedition in 1989

This paper describes observations of the upper atmosphere physics at Asuka Station from January 1 to December 24,1989,carried out by the 30th Japanese Antarctic Research Expedition (JARE-30). In JARE-30 one research member of the upper atmosphere physics has been wintering at Asuka Station, and seve...

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Main Author: Akira Yukimatu
Format: Article in Journal/Newspaper
Language:English
Japanese
Published: National Institute of Polar Research 1992
Subjects:
Online Access:https://doi.org/10.15094/00008772
https://doaj.org/article/2bb7f3a6fe5743e690c36a4129fa70b0
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spelling ftdoajarticles:oai:doaj.org/article:2bb7f3a6fe5743e690c36a4129fa70b0 2023-05-15T13:56:24+02:00 Observation of the upper atmosphere physics at Asuka Station by the 30th Japanese Antarctic Research Expedition in 1989 Akira Yukimatu 1992-07-01T00:00:00Z https://doi.org/10.15094/00008772 https://doaj.org/article/2bb7f3a6fe5743e690c36a4129fa70b0 EN JA eng jpn National Institute of Polar Research http://doi.org/10.15094/00008772 https://doaj.org/toc/0085-7289 https://doaj.org/toc/2432-079X doi:10.15094/00008772 0085-7289 2432-079X https://doaj.org/article/2bb7f3a6fe5743e690c36a4129fa70b0 Antarctic Record, Vol 36, Iss 2, Pp 294-309 (1992) Geography (General) G1-922 article 1992 ftdoajarticles https://doi.org/10.15094/00008772 2022-12-31T11:13:46Z This paper describes observations of the upper atmosphere physics at Asuka Station from January 1 to December 24,1989,carried out by the 30th Japanese Antarctic Research Expedition (JARE-30). In JARE-30 one research member of the upper atmosphere physics has been wintering at Asuka Station, and several instruments were newly installed so as to observe auroral phenomena in conjunction with Syowa Station, Iceland observations, and scientific satellites. Characteristics of the JARE-30's observations at Asuka Station are as follows : 1) The observation of CNA with a 30-MHz riometer has been made throughout the year. 2) A fixed direction and a tracking photometers were newly installed, and spatial and temporal developments of aurora photo emissions in various wave lengths were observed. 3) An all sky camera used in JARE-28 was re-installed. 4) An all sky SIT-TV camera was newly installed so as to observe auroral motions with high time resolution. 5) A digital data recorder was installed for the auroral photometric data. 6) Z-component of a ULF induction magnetometer which had been in trouble was recovered, so we could observe the three components of both a fluxgate magnetometer and the induction magnetometer. 7) In 1989,the solar activity was very high and there were many interesting geophysical events, and auroral phenomena. Article in Journal/Newspaper Antarc* Antarctic Iceland Directory of Open Access Journals: DOAJ Articles Antarctic Syowa Station
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
Akira Yukimatu
Observation of the upper atmosphere physics at Asuka Station by the 30th Japanese Antarctic Research Expedition in 1989
topic_facet Geography (General)
G1-922
description This paper describes observations of the upper atmosphere physics at Asuka Station from January 1 to December 24,1989,carried out by the 30th Japanese Antarctic Research Expedition (JARE-30). In JARE-30 one research member of the upper atmosphere physics has been wintering at Asuka Station, and several instruments were newly installed so as to observe auroral phenomena in conjunction with Syowa Station, Iceland observations, and scientific satellites. Characteristics of the JARE-30's observations at Asuka Station are as follows : 1) The observation of CNA with a 30-MHz riometer has been made throughout the year. 2) A fixed direction and a tracking photometers were newly installed, and spatial and temporal developments of aurora photo emissions in various wave lengths were observed. 3) An all sky camera used in JARE-28 was re-installed. 4) An all sky SIT-TV camera was newly installed so as to observe auroral motions with high time resolution. 5) A digital data recorder was installed for the auroral photometric data. 6) Z-component of a ULF induction magnetometer which had been in trouble was recovered, so we could observe the three components of both a fluxgate magnetometer and the induction magnetometer. 7) In 1989,the solar activity was very high and there were many interesting geophysical events, and auroral phenomena.
format Article in Journal/Newspaper
author Akira Yukimatu
author_facet Akira Yukimatu
author_sort Akira Yukimatu
title Observation of the upper atmosphere physics at Asuka Station by the 30th Japanese Antarctic Research Expedition in 1989
title_short Observation of the upper atmosphere physics at Asuka Station by the 30th Japanese Antarctic Research Expedition in 1989
title_full Observation of the upper atmosphere physics at Asuka Station by the 30th Japanese Antarctic Research Expedition in 1989
title_fullStr Observation of the upper atmosphere physics at Asuka Station by the 30th Japanese Antarctic Research Expedition in 1989
title_full_unstemmed Observation of the upper atmosphere physics at Asuka Station by the 30th Japanese Antarctic Research Expedition in 1989
title_sort observation of the upper atmosphere physics at asuka station by the 30th japanese antarctic research expedition in 1989
publisher National Institute of Polar Research
publishDate 1992
url https://doi.org/10.15094/00008772
https://doaj.org/article/2bb7f3a6fe5743e690c36a4129fa70b0
geographic Antarctic
Syowa Station
geographic_facet Antarctic
Syowa Station
genre Antarc*
Antarctic
Iceland
genre_facet Antarc*
Antarctic
Iceland
op_source Antarctic Record, Vol 36, Iss 2, Pp 294-309 (1992)
op_relation http://doi.org/10.15094/00008772
https://doaj.org/toc/0085-7289
https://doaj.org/toc/2432-079X
doi:10.15094/00008772
0085-7289
2432-079X
https://doaj.org/article/2bb7f3a6fe5743e690c36a4129fa70b0
op_doi https://doi.org/10.15094/00008772
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