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SPACE PLASMA PHYSICS GROUP
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The MSSL Space Plasma Physics Group pages have moved to

HTTP://WWW.UCL.AC.UK/MSSL/SPACE-PLASMA-PHYSICS.

Information about the PEACE instruments on the Cluster and Double Star Missions remains up-to-date on this site. Please update your links accordingly

Double Star

The mission

The Double Star Project is China's first purely scientific space mission and its first collaboration with the European Space Agency. Double Star is designed for magnetospheric research, using two Chinese spacecraft, TC-1 and TC-2, which each have a payload consisting of both Chinese and European experiments. The TC-1 spacecraft is in a near-equatorial orbit and TC-2 in a polar orbit. The launch vehicle was a Chinese Long March 2C . TC-1 launched successfully on 27 December 2003, TC-2 on 25 July 2004. The Double Star mission was designed with collaboration with ESA's Cluster mission in mind. The mission design allows the six spacecraft together to address science questions that neither Cluster nor Double Star could address alone.

Science objectives

artists impression of double_star in orbit The Double Star mission uses two spacecraft flying in different but carefully chosen orbits to explore the Earth's magnetosphere. The magnetosphere is a huge region of space surrounding the Earth where the Earth's magnetic field can be detected. Outside the magnetosphere is a fast flowing plasma from the Sun, the solar wind. Inside the magnetosphere we find plasma from the solar wind as well as the Earth's ionosphere. Furthemore, we know that large amounts of energy are transferred from the solar wind to the magnetosphere. The energy is frequently released in dramatic processes, such as substorms, that generate energetic radiation belt particles, disturb the Earths' magnetic field at the surface and power the Northern Lights.

Some of the Double Star science goals (e.g. radiation belt studies) can be addressed with TC-1 and TC-2 alone, but the most exciting science opportunities arise when Double Star works in coordination with Cluster. The two Double Star spacecraft plus the Cluster tetrahedron provide three measurement points separated on a large scale. The clever part is that these three measurement points will be used in ways no previous triad has been used. For example, in late spring 2004 and 2005, TC-1 will search for solar wind entry points at the sunward edge of the magnetosphere, while Cluster (and in 2005, TC-2) are placed to observe any solar wind plasma that enters and reveal how it is changed as it travels towards the Earth's atmosphere. In late summer 2004,  Cluster, TC-1 and TC-2 lie at different distances downstream of the Earth in the magnetotail. Simultaneous observations in these regions will help us to answer the long-standing questions of where, when, and how a substorm begins. These remain unanswered until now because spacecraft have never been properly placed to make the key observations.

MSSL are Principal Investigator institution for the PEACE electron spectrometer team, leading an international team of scientific collaborators. MSSL carried out the work needed to produce two single sensor electron spectrometers from the two sensor Cluster II Flight Spare instrument. Additional work was needed to protect the instruments from the more severe radiation environment that Double Star will experience, and to render the instruments fully ITAR compliant. It is planned that a PEACE Operations Team at MSSL will control the instruments, process their data and carry out in-flight calibration work.

Further Information

The Double Star homepage at ESA

The Double Star PEACE homepage at MSSL


26 May 2004
Andrew Fazakerley
anf@mssl.ucl.ac.uk


Mullard Space Science Laboratory - Holmbury St. Mary - Dorking - Surrey - RH5 6NT - Telephone: +44 (0)1483 204100 - Copyright © 1999-2005 UCL


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