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Selected Problems in Collisionless-Shock Physics
DOI: 10.1023/B:SPAC.0000023372.12232.b7 Bibcode: 2004SSRv..110..161L

Krasnoselskikh, V.; Kucharek, H.; Scholer, M. +6 more

The physics of collisionless shocks is a very broad topic, which has been well studied for many decades. However, there are a number of important issues which remain unresolved. Moreover, there have been new findings, which cast doubt on well-established ideas. The purpose of this review is to address a subset of unresolved problems in collisionle…

2004 Space Science Reviews
Cluster 149
Radar: The Cassini Titan Radar Mapper
DOI: 10.1007/s11214-004-1438-9 Bibcode: 2004SSRv..115...71E

Lorenz, R. D.; Soderblom, L. A.; Ostro, S. J. +19 more

The Cassini RADAR instrument is a multimode 13.8 GHz multiple-beam sensor that can operate as a synthetic-aperture radar (SAR) imager, altimeter, scatterometer, and radiometer. The principal objective of the RADAR is to map the surface of Titan. This will be done in the imaging, scatterometer, and radiometer modes. The RADAR altimeter data will pr…

2004 Space Science Reviews
Cassini 139
Cassini Radio Science
DOI: 10.1007/s11214-004-1436-y Bibcode: 2004SSRv..115....1K

French, R. G.; Flasar, F. M.; Asmar, S. W. +10 more

Cassini radio science investigations will be conducted both during the cruise (gravitational wave and conjunction experiments) and the Saturnian tour of the mission (atmospheric and ionospheric occultations, ring occultations, determinations of masses and gravity fields). New technologies in the construction of the instrument, which consists of a …

2004 Space Science Reviews
Cassini 67
Observations of the Sun at Vacuum- Ultraviolet Wavelengths from Space. Part I: Concepts and Instrumentation
DOI: 10.1023/B:SPAC.0000032695.27525.54 Bibcode: 2004SSRv..111..415W

Wilhelm, Klaus; Marsch, Eckart; Dwivedi, Bhola N. +1 more

Studies of the high-temperature solar atmosphere are to a large extent based on spectroscopic observations of emission lines and continuum radiation in the vacuum-ultraviolet (VUV) wavelength range of the electromagnetic spectrum. In addition, important contributions stem from soft X-ray measurements. Most of the VUV radiation is produced by trans…

2004 Space Science Reviews
SOHO 27
Mars Express and MARSIS
DOI: 10.1023/B:SPAC.0000032712.05204.5e Bibcode: 2004SSRv..111..245N

Nielsen, Erling

The Mars Express mission to be launched in 2003 will provide high resolution measurements of the Martian atmosphere and ionosphere. The neutral density, temperature, and composition will be measured, and MARSIS, a low frequency radar experiment, will probe the Martian plasma environment for electron densities in the range from 100 to 3 × 105<…

2004 Space Science Reviews
MEx 19
The Impact of Space Experiments on our Knowledge of the Physics of the Universe
DOI: 10.1023/B:SPAC.0000032807.99883.09 Bibcode: 2004SSRv..112....1G

Giovannelli, Franco; Sabau-Graziati, Lola

With the advent of space experiments it was demonstrated that cosmic sources emit energy practically across all the electromagnetic spectrum via different physical processes. Several physical quantities give witness to these processes which usually are not stationary; those physical observable quantities are then generally variable. Therefore simu…

2004 Space Science Reviews
INTEGRAL 13
The Magnetostatic Cleanliness Program for the Cassini Spacecraft
DOI: 10.1007/s11214-004-1433-1 Bibcode: 2004SSRv..114..385N

Narvaez, P.

The Cassini spacecraft, launched in October 1997 and expected to reach Saturn in 2004, carries two magnetometer experiments on a 10-m boom, one at the mid-section of the boom and the other situated at the end of the boom. In order to gather valid scientific magnetic field data and avoid electromagnetic interference, the spacecraft had to comply wi…

2004 Space Science Reviews
Cassini 10