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The Beagle 2 environmental sensors: science goals and instrument description
DOI: 10.1016/j.pss.2004.07.015 Bibcode: 2004P&SS...52.1141T

Patel, M. R.; Zarnecki, J. C.; Wilson, C. F. +12 more

A suite of instruments on the Beagle 2 Mars lander was designed and built in order to investigate the environmental conditions at the landing site. The sensor suite was capable of measuring air temperature at two heights, surface level pressure, wind speed and direction, saltated particle momentum, UV flux (diffuse and direct at five wavelengths),…

2004 Planetary and Space Science
MEx 16
A stratospheric balloon experiment to test the Huygens atmospheric structure instrument (HASI)
DOI: 10.1016/j.pss.2004.02.009 Bibcode: 2004P&SS...52..867F

Patel, M. R.; Fulchignoni, M.; Hathi, B. +15 more

We developed a series of balloon experiments parachuting a 1:1 scale mock-up of the Huygens probe from an altitude just over 30 km to simulate at planetary scale the final part of the descent of the probe through Titan's lower atmosphere. The terrestrial atmosphere represents a natural laboratory where most of the physical parameters meet quite we…

2004 Planetary and Space Science
Huygens 12
Scientific objectives and selection of targets for the SMART-1 Infrared Spectrometer (SIR)
DOI: 10.1016/j.pss.2004.09.002 Bibcode: 2004P&SS...52.1261B

Keller, H. U.; Hiesinger, H.; Mall, U. +3 more

The European SMART-1 mission to the Moon, primarily a testbed for innovative technologies, was launched in September 2003 and will reach the Moon in 2005. On board are several scientific instruments, including the point-spectrometer SMART-1 Infrared Spectrometer (SIR). Taking into account the capabilities of the SMART-1 mission and the SIR instrum…

2004 Planetary and Space Science
SMART-1 11
The far-infrared spectra of Jupiter and Saturn
DOI: 10.1016/j.pss.2003.07.004 Bibcode: 2004P&SS...52..379B

Lellouch, E.; Encrenaz, T.; Orton, G. S. +4 more

We present far-infrared, disk-averaged spectra of Jupiter and Saturn that were measured with the Long Wavelength Spectrometer aboard the Infrared Space Observatory. The Long Wavelength Spectrometer covered the wavelength region between 43 and 197 µm and achieved in grating mode a resolving power of 150-300.

The spectra observed in the f…

2004 Planetary and Space Science
ISO 11
Rotational dynamics of subsolar sublimating triaxial comets
DOI: 10.1016/j.pss.2004.04.001 Bibcode: 2004P&SS...52..897M

Mysen, Eirik

A model with subsolar water sublimation on a triaxial, ellipsoidal comet nucleus is presented for the calculation of reactive torques. The resulting differential equations describing the comet's rotation are then Hamiltonian, and gravity-gradients are trivial to include. While effects derived from a weak perturbing function are neither able to cha…

2004 Planetary and Space Science
Rosetta 10
Martian northern polar cap: Layering and possible implications for radar sounding
DOI: 10.1016/j.pss.2004.08.002 Bibcode: 2004P&SS...52.1195I

Ilyushin, Yaroslaw A.

The propagation of electromagnetic waves in the northern polar ice sheet of Mars is considered. It is shown that the dispersion and attenuation of radio waves in the polar sheet are regulated by two groups of factors: the physical and chemical composition of the ice, and the geometrical parameters of the layered structure of polar sheet. Both anal…

2004 Planetary and Space Science
MEx 9
Comet Hyakutake (C/1996 B2): Spectacular disconnection event and the latitudinal structure of the solar wind
DOI: 10.1016/j.pss.2003.10.001 Bibcode: 2004P&SS...52..313S

Brandt, J. C.; Snow, M.; Mikuz, H. +2 more

Images of comet Hyakutake (C/1996 B2) are analyzed in conjunction with solar wind data from spacecraft to determine the relationship between solar wind conditions and plasma tail morphology. The disconnection event (DE) on March 25, 1996 is analyzed with the aid of data from the IMP-8 and WIND Earth-orbiting spacecraft and the DE is found to be co…

2004 Planetary and Space Science
Ulysses 8
On a systematic spectral variation of energetic ions in the Jovian outer magnetosphere: HI-SCALE/Ulysses observations
DOI: 10.1016/j.pss.2003.07.006 Bibcode: 2004P&SS...52..561M

Sarris, E. T.; Anagnostopoulos, G. C.; Marhavilas, P. K.

An important finding of Ulysses flyby of Jupiter is the discovery of a large-scale energetic particle layer adjacent to the magnetopause. Previous studies discussed the particle flux and the anisotropy characteristics of this layer. This study examines the spectral characteristics of the large-scale magnetopause boundary layer of energetic particl…

2004 Planetary and Space Science
Ulysses 6
Simulation and analysis of the revised Huygens probe entry and descent trajectory and radio link modelling
DOI: 10.1016/j.pss.2004.03.008 Bibcode: 2004P&SS...52..799K

Lebreton, J. -P.; Kazeminejad, B.; Pérez-Ayúcar, M. +7 more

The Cassini spacecraft will arrive at Saturn in 2004 carrying the Huygens probe. The beginning of the Cassini tour at Saturn has been redesigned to achieve a different relative orbiter/probe geometry in order to compensate for the probe relay receiver design flaw that was discovered during tests in February 2000. This paper presents a numerical si…

2004 Planetary and Space Science
Huygens 6
Visualization and topographical analysis of the Mars surface
DOI: 10.1016/j.pss.2003.08.017 Bibcode: 2004P&SS...52..249D

Dorninger, P.; Jansa, J.; Briese, Ch.

The Institute of Photogrammetry and Remote Sensing has more than 30 years of experience in computation, visualization and analysis of digital terrain data. Most of the developed methods and algorithms are implemented in the software application SCOP++ and tested on Earth datasets. Due to the institute's involvement into Mars Express, these methods…

2004 Planetary and Space Science
MEx 5