TOP > About ISAS > International Cooperation
Overview
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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.






