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The four Cluster spacecraft form a nearly regular tetrahedron with the configuration index (Q_{rm G}) close 3 (Robert et al. 2001; von Stein et al. 1992).
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The four Cluster spacecraft formed a nearly regular tetrahedron with a spacecraft separation of about 1000 km.
The mission orbits of the 3 spacecraft forming a nearly equilateral triangular array are chosen to be near the Sun-Earth Lagrange points L3, L4 and L5.
The interplanetary orbits of three pairs of spacecraft, forming three laser interferometers, are designed such that their separations, i.e. the lengths of the interferometer arms, remain nearly constant.
This task proved to be difficult, as a large cloud of debris around the spacecraft formed by the venting S-IVB made it hard to distinguish the stars.
It seems to be natural that the waves hardly steepen since their narrowband spectra in the spacecraft frame can be formed from waves in the plasma frame with a broader frequency band and smaller amplitudes than those of observed waves.
The objective is to drive follower spacecraft to form a prescribed shape around a leader, while collision avoidance is achieved among different spacecraft.
Its spacecraft orbits form a triangular array close to an equilateral triangle in the vicinity of the solar-terrestrial Lagrangian points L3, L4 and L5.
An existing superfluid helium dewar, containing the four differential accelerometers, will be used along with a small, semi-production spacecraft to form the drag free satellite.
Results are presented for the Solar Array in the SPP spacecraft in the form of design particle size and impact speed for various PNI levels.
The primary contribution of this paper resides on the application of a distributed coordination architecture, which provides an autonomous and robust ability to dynamically form spacecraft teams once the target has been detected, and to dynamically build a processing network for the orbit determination of space debris.
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