Javascript must be enabled to continue!
History of Kakioka Magnetic Observatory
View through CrossRef
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.
Title: History of Kakioka Magnetic Observatory
Description:
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.
Related Results
History of Kakioka Magnetic Observatory
History of Kakioka Magnetic Observatory
Abstract. Kakioka Magnetic Observatory (KMO) was founded in 1913 by Central Meteorological Observatory (CMO, later Japan Meteorological Agency) as a successor of Tokyo Magnetic Obs...
Magnetic cloak made of NdFeB permanent magnetic material
Magnetic cloak made of NdFeB permanent magnetic material
In the past few years, the concept of an electromagnetic invisibility cloak has received much attention. Based on the pioneering theoretical work, invisibility cloaks have been gre...
Astronomical research in Kharkiv at the end of the 19th century – the first half of the 20th century
Astronomical research in Kharkiv at the end of the 19th century – the first half of the 20th century
The main milestones of the formation and development of astronomical science in Kharkiv during 1883–1945 are reconstructed on the example of the activities of the astronomical obse...
Analysis of magnetohydrodynamic drag character for hypersonic vehicles
Analysis of magnetohydrodynamic drag character for hypersonic vehicles
In hypersonic flight, a very high temperature area can form ahead of the nose of aerocraft due to the shock aerodynamic heating, which leads to air weakly ionized. Many researchers...
Fieldwork teaching on Mars using a Large-Scale Visualisation System
Fieldwork teaching on Mars using a Large-Scale Visualisation System
Recent orbital and rover images of the surface of Mars provide exceptional high-resolution views of the martian landscapes and its surface geology. These extensive datasets provide...
Een passie voor precisie: Frederik Kaiser en het instrumentarium van de Leidse Sterrewacht
Een passie voor precisie: Frederik Kaiser en het instrumentarium van de Leidse Sterrewacht
Passion for precision. Frederik Kaiser and the instrumentation of Leiden ObservatoryFrederik Kaiser (1808-1872) was one of the most inspiring directors of the Leiden astronomical o...
OMERE: A Long-Term Observatory of Soil and Water Resources, in Interaction with Agricultural and Land Management in Mediterranean Hilly Catchments
OMERE: A Long-Term Observatory of Soil and Water Resources, in Interaction with Agricultural and Land Management in Mediterranean Hilly Catchments
<p class="western"><span lang="en-US">This communication is dedicated to the Mediterranean agro-hydrological observa...
The Earth's magnetic field variations at the Algerian magnetic observatory of Tamanrasset from 1932 to 2020.
The Earth's magnetic field variations at the Algerian magnetic observatory of Tamanrasset from 1932 to 2020.
<p>In order to understand the spatial and temporal behavior of the Earth's magnetic field, scientists, following C.F. Gauss initiative in 1838 have established observ...

