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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National Institute of Polar Research
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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 |
_version_ |
1766263900981952512 |