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Overview

International Cooperation

Reflecting that space is the common frontier of humanity, space science missions are almost always conducted as multi-national collaborations. In Japan, too, international cooperation has an important meaning in the field of space missions.

By floating balloons or launching rockets in Antarctica or the equatorial belt, for example, we can conduct observations impossible in the Japan area. In addition, by gathering together mutual technologies and experiences, we can conduct more fruitful observations.

By sharing tasks, it is possible to implement large-scale programs which would be difficult for single nations. For example, through simultaneous observations by several satellites and observatories or the ground, we have been able to observe the dynamic nature of the universe.

The following tables show research implemented under cooperation between foreign and Japanese research groups. (Names of country, place, etc., are those of the time of cooperation.)

Observation By Rocket

Purpose Cooperation Partner, etc. Year
X-ray star India: Thumba 1968,69
Universe seen in X-rays USA: Hawaii 1971, 72, 74, 76
Atmosphere over equator India: Thumba 1972-73
Stratosphere USA: New Mexico 1974
Ionosphere Canada: Perry Cape 1974, 77
Ionosphere Peru 1975
Aurora belt ionosphere Denmark: Greenland 1974, 76
Ozone observation USA: Wallops 1979
Parent-child rocket experiment Uchinora, Kagoshima 1980, 81
Parent-child rocket experiment USA: White Sands and Alaska 1983, 85, 92
Thermal energy balance of ionosphere West Germany 1984
Observation of middle atmosphere Uchinoura, Kagoshima  1980, 90
Aurora observation Norway: Andoya 1990
Ion outflow mechanism Norway: Spitsbergen 2000
Ionosphere irregularities USA: NASA, Clemson Univ. and Texas Univ. 2002
Observation of aurora Norway: Andoya 2004

Observation by Balloon

Purpose Cooperation Partner, etc. Year
X-ray star of the Scorpion India: Hyderabad 1970-1975
X-rays from the Crab Nebula USA: Texas 1974-1978
Stratosphere USA: New Mexico 1973
Cosmic rays India: Hyderabad 1974
Aurorae USA: Alaska 1974
Aurora X-rays Canada: Tompson 1975
Cosmic rays USA: Texas 1975-1980
High-energy cosmic rays Australia 1978-1980
Universe seen in infrared Australia 1978-1980
Atmospheric electricity Australia 1980
Galaxy infrared, heavy primary cosmic-ray, atmospheric electricity Australia 1983
Solar eclipse Indonesia 1983
Galaxy far-infrared Australia 1985
Atmospheric composition, infrared, X-ray Japan → China 1986-1988
Observation of hard X-ray/gamma ray Brasil: Sao Paulo 1988-1991
Galaxy far-infrared spectrum line USA: Texas 1991-1993
High-energy cosmic particle USA → Canada: Manitoba 1993-2002
Ozone Germany → Norway: Spitsbergen 1994-1999
Cosmic rays Russia: Kamchatka 1995-1999
Observation by balloon, loading solar telescope China: National Astronomical Observatory 1998-2001
Observation of far-infrared India: Hyderabad 1998-
High-energy cosmic particle USA → The south pole: Macmart base 2004-
Observation of hard X-ray and space far-infrared Brasil: Sao Paulo 2005-

Observation by Satellite

Purpose Cooperation Partner, etc. Year Mode
Space Experiment with Particle Accelerators (SEPAC) USA: NASA 1974-1992 2
TAIYO: investigation of ionosphere West Germany: AEROS-B satellite 1975-1976 5
KYOKKO: aurora observation Canada: ISIS-2 satellite 1978 5
JIKIKEN: plasma wave in magnetosphere USA: ISIS satellite,etc. 1979-1980 5
HAKUCHO: observation of light, radio of X-ray stars European Southern Observatory, etc. 1979-1981 5
HINOTORI: observation of solar activity USA: SMM satellite 1981 5
TENMA: X-ray star, X-ray galaxy Europe: ESA 1983-1984 5
SAKIGAKE: Halley's comet Europe: ESA
Soviet Union: IKI
USA: NASA
1985-1986 4, 5
SUISEI: Halley's comet Europe: ESA
Soviet Union: IKI
USA: NASA
1985-1986 4, 5
GINGA: X-ray star, X-ray galaxy, observation of gamma-ray bursts UK: Leicester Univ. 1987-1991 1, 4
USA: Los Alamos National Laboratory 1987-1998
Voyager-2 USA: NASA 1989 3
AKEBONO: observation of aurorae Canada: Canadian Space Agency (CSA) 1989- 1, 3, 4
HITEN: observation of micro cosmic dust West Germany: Technische Universität München (MTU) 1990-1993 1
YOHKOH: observation of solar activity USA: NASA
UK: Mullard Space Science Laboratory
1991-2004 1, 3, 4
GEOTAIL: research of magnetospheric tail USA: NASA,Iowa Univ.,etc. 1992- 1, 2, 3, 4
ASCA: X-ray star, X-ray galaxy, X-ray background radiation USA: NASA(Goddard Space Flight Center), MIT, etc. 1993-2001 1, 3, 4
EXPRESS: reentry to atmosphere Uchinoura,Kagoshima
Germany: DARA
1995-1996 1, 2, 3
SFU: space experiment / observation free flyer USA: NASA 1995-1996 2
Joint observation by ESA satellite ISO ESA: ISO satellite 1995-1998  
HALCA: space VLBI observation USA: NASA (Jet Propulsion Laboratory)
National Radio Astronomy Observatory (NRAO)
European VLBI Network (EVN,JIVE)
Australia: Australia Telescope National Facility (ATNF)
Canada: Dominion Radio Astrophysical Observatory,etc.
1997-2005 3, 4, 5
NOZOMI: observation of Mars' upper atmosphere USA: NASA
France: CNES
Canada: Canadian Space Agency (CSA)
Sweden: Swedish Instutute of Space Physics (SISP)
Germany: Technische Universitaet Muenchen (MTU)
1998-2003 1, 3, 4
ESA: Mars Express 2000-2003
IMAGE: imaging observation of earth's magnetosphere USA: NASA 1999-2003  
RHESSI: observation of solar activity USA: NASA 2002-  
HAYABUSA: asteroid exploration mission. Technical development and demonstration necessary for sample return USA: NASA 2003- 1, 3, 4
SUZAKU: X-ray star, X-ray galaxy, Gamma-ray bursts USA: NASA 2005- 1, 4
REIMEI: technology demonstration of small satellite Russia: FSA 2005- 2
AKARI: all-sky survey by infrared Europe: ESA
Korea: Korea Astronomy and Space Science Institute (KASI)
2006- 1, 3, 4
HINODE: observation of solar activity USA: NASA
UK: Mullard Space Science Laboratory
2006- 1, 3, 4

Modes of Cooperation:
1: International partner provides instruments on ISAS spacecraft, or vice versa.
2: International partner launches or/and recovers ISAS spacecraft, or vice versa.
3: International partner receives telemetry from ISAS spacecraft, or vice versa.
4: International participation in analysis of ISAS spacecraft data.
5: Spacecrafts or/and ground observatories of ISAS and international partner(s) conduct joint observations.

Space Science between US and Japan Based on the Japan-US Science and Technology Cooperation Agreement - Non-energy Field

In 1979, the US-Japan Permanent Executive Committee was established to promote collaboration projects between U.S. and Japan in the space field such as remote sensing and scientific observation, and to consider new collaboration projects. Following its establishment, a variety of collaboration projects have been implemented.

Inter-Agency Consultative Group for Space Science (IACG)

International cooperation on space science has been carried out under the framework called the IACG (Inter-Agency Consultative Group for Space Science), which originated in the Halley's comet exploration program in the 1980s.