{"title":"角冈磁观测站的历史","authors":"I. Fujii, S. Nagamachi","doi":"10.5194/hgss-13-147-2022","DOIUrl":null,"url":null,"abstract":"Abstract. Kakioka Magnetic Observatory (KMO) was founded in 1913 by\nthe Central Meteorological Observatory (CMO, later the Japan Meteorological Agency) as a successor to Tokyo Magnetic Observatory. Kakioka was a village 70 km north of Tokyo and was selected to escape from tram noise in Tokyo. At first, it was an unstaffed observatory only for geomagnetic field observation. Then, the Great Kanto Earthquake in 1923 changed the fate of\nKMO because the earthquake severely damaged the CMO in Tokyo, and recording papers of KMO were lost. KMO was staffed in 1924 and was redesigned as an institute for geophysics rather than geomagnetism. KMO operated a variety of\nobservations, such as the atmospheric electric field, the geoelectric field, the seismicity, the air temperature, the wind velocity, the sunspot and\nsolar prominence as well as the geomagnetic field, by the 1940s. In addition, research activity flourished with the leadership of the first director, Shuichi Imamichi. After World War II was over in 1945, KMO formed a\nnetwork of observatories in Japan by founding several branch observatories\noriginally for geoelectric field observation. Two branch observatories at Memambetsu and Kanoya survived, with geomagnetic field observation added in the International Geophysical Year project (1957–1958). Efforts in development of instruments for geomagnetic absolute measurement and systems of high-sampling recordings in the 1950s to 1970s resulted in the development of the Kakioka Automatic Standard Magnetometer (KASMMER) system in\n1972. KASMMER measured the geomagnetic field every 3 s at the highest standard in the world in digital form, giving 1 min digital values of the geomagnetic field available. This system has been updated, and\nthe high-sampling technology was applied to geoelectric field observation and atmospheric electric field observation. Later, adding\ngeomagnetic field observation at Chichijima in 1971, KMO established a unique electric and magnetic observation network at Kakioka, Memambetsu,\nKanoya and Chichijima and provided precise and high-speed sampling data\n(1 min, 1 and 0.1 s values) by 2001. On the other hand, KMO gradually\nterminated or automated their observations and reduced their staff in the last several decades following the government's reform policy. The two branch\nobservatories at Memambetsu and Kanoya were unstaffed in 2011, and the atmospheric electric field at Memambetsu was terminated at that time. The\ngeoelectric field observations at Kakioka, Memambetsu and Kanoya were\nterminated in 2021 as well as the atmospheric electric field at Kakioka. KMO\nfocuses on geomagnetic observation for now and puts efforts into total force observation at volcanoes and the digitization of historic analog\ndata.\n","PeriodicalId":48918,"journal":{"name":"History of Geo- and Space Sciences","volume":" ","pages":""},"PeriodicalIF":0.5000,"publicationDate":"2022-08-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"History of Kakioka Magnetic Observatory\",\"authors\":\"I. Fujii, S. Nagamachi\",\"doi\":\"10.5194/hgss-13-147-2022\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Abstract. Kakioka Magnetic Observatory (KMO) was founded in 1913 by\\nthe Central Meteorological Observatory (CMO, later the Japan Meteorological Agency) as a successor to Tokyo Magnetic Observatory. Kakioka was a village 70 km north of Tokyo and was selected to escape from tram noise in Tokyo. At first, it was an unstaffed observatory only for geomagnetic field observation. Then, the Great Kanto Earthquake in 1923 changed the fate of\\nKMO because the earthquake severely damaged the CMO in Tokyo, and recording papers of KMO were lost. KMO was staffed in 1924 and was redesigned as an institute for geophysics rather than geomagnetism. KMO operated a variety of\\nobservations, such as the atmospheric electric field, the geoelectric field, the seismicity, the air temperature, the wind velocity, the sunspot and\\nsolar prominence as well as the geomagnetic field, by the 1940s. In addition, research activity flourished with the leadership of the first director, Shuichi Imamichi. After World War II was over in 1945, KMO formed a\\nnetwork of observatories in Japan by founding several branch observatories\\noriginally for geoelectric field observation. Two branch observatories at Memambetsu and Kanoya survived, with geomagnetic field observation added in the International Geophysical Year project (1957–1958). Efforts in development of instruments for geomagnetic absolute measurement and systems of high-sampling recordings in the 1950s to 1970s resulted in the development of the Kakioka Automatic Standard Magnetometer (KASMMER) system in\\n1972. KASMMER measured the geomagnetic field every 3 s at the highest standard in the world in digital form, giving 1 min digital values of the geomagnetic field available. This system has been updated, and\\nthe high-sampling technology was applied to geoelectric field observation and atmospheric electric field observation. Later, adding\\ngeomagnetic field observation at Chichijima in 1971, KMO established a unique electric and magnetic observation network at Kakioka, Memambetsu,\\nKanoya and Chichijima and provided precise and high-speed sampling data\\n(1 min, 1 and 0.1 s values) by 2001. On the other hand, KMO gradually\\nterminated or automated their observations and reduced their staff in the last several decades following the government's reform policy. The two branch\\nobservatories at Memambetsu and Kanoya were unstaffed in 2011, and the atmospheric electric field at Memambetsu was terminated at that time. The\\ngeoelectric field observations at Kakioka, Memambetsu and Kanoya were\\nterminated in 2021 as well as the atmospheric electric field at Kakioka. KMO\\nfocuses on geomagnetic observation for now and puts efforts into total force observation at volcanoes and the digitization of historic analog\\ndata.\\n\",\"PeriodicalId\":48918,\"journal\":{\"name\":\"History of Geo- and Space Sciences\",\"volume\":\" \",\"pages\":\"\"},\"PeriodicalIF\":0.5000,\"publicationDate\":\"2022-08-26\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"History of Geo- and Space Sciences\",\"FirstCategoryId\":\"98\",\"ListUrlMain\":\"https://doi.org/10.5194/hgss-13-147-2022\",\"RegionNum\":4,\"RegionCategory\":\"哲学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"GEOSCIENCES, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"History of Geo- and Space Sciences","FirstCategoryId":"98","ListUrlMain":"https://doi.org/10.5194/hgss-13-147-2022","RegionNum":4,"RegionCategory":"哲学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"GEOSCIENCES, MULTIDISCIPLINARY","Score":null,"Total":0}
Abstract. Kakioka Magnetic Observatory (KMO) was founded in 1913 by
the Central Meteorological Observatory (CMO, later the Japan Meteorological Agency) as a successor to Tokyo Magnetic Observatory. Kakioka was a village 70 km north of Tokyo and was selected to escape from tram noise in Tokyo. At first, it was an unstaffed observatory only for geomagnetic field observation. Then, the Great Kanto Earthquake in 1923 changed the fate of
KMO because the earthquake severely damaged the CMO in Tokyo, and recording papers of KMO were lost. KMO was staffed in 1924 and was redesigned as an institute for geophysics rather than geomagnetism. KMO operated a variety of
observations, such as the atmospheric electric field, the geoelectric field, the seismicity, the air temperature, the wind velocity, the sunspot and
solar prominence as well as the geomagnetic field, by the 1940s. In addition, research activity flourished with the leadership of the first director, Shuichi Imamichi. After World War II was over in 1945, KMO formed a
network of observatories in Japan by founding several branch observatories
originally for geoelectric field observation. Two branch observatories at Memambetsu and Kanoya survived, with geomagnetic field observation added in the International Geophysical Year project (1957–1958). Efforts in development of instruments for geomagnetic absolute measurement and systems of high-sampling recordings in the 1950s to 1970s resulted in the development of the Kakioka Automatic Standard Magnetometer (KASMMER) system in
1972. KASMMER measured the geomagnetic field every 3 s at the highest standard in the world in digital form, giving 1 min digital values of the geomagnetic field available. This system has been updated, and
the high-sampling technology was applied to geoelectric field observation and atmospheric electric field observation. Later, adding
geomagnetic field observation at Chichijima in 1971, KMO established a unique electric and magnetic observation network at Kakioka, Memambetsu,
Kanoya and Chichijima and provided precise and high-speed sampling data
(1 min, 1 and 0.1 s values) by 2001. On the other hand, KMO gradually
terminated or automated their observations and reduced their staff in the last several decades following the government's reform policy. The two branch
observatories at Memambetsu and Kanoya were unstaffed in 2011, and the atmospheric electric field at Memambetsu was terminated at that time. The
geoelectric field observations at Kakioka, Memambetsu and Kanoya were
terminated in 2021 as well as the atmospheric electric field at Kakioka. KMO
focuses on geomagnetic observation for now and puts efforts into total force observation at volcanoes and the digitization of historic analog
data.
期刊介绍:
The scope of History of Geo- and Space Sciences (HGSS) is to document historical facts and knowledge and to improve awareness of the history of geoscience. The knowledge of the development of geosciences and their experimental methods and theories in the past can improve our current understanding and may stimulate current research. It is encouraging for young scientists to read biographical material of historical figures in their research area. It is important as well to learn that history of science is an integrated part of the ongoing research in their research area. Another important aim of the journal is the association of historical retrospective and current research.