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Quasi-periodic emissions (15- 80 min) from the poles of Jupiter as a principal source of the large-scale high-latitude magnetopause boundary layer of energetic particle
DOI: 10.1016/j.pss.2003.10.002 Bibcode: 2004P&SS...52..543K

Preka-Papadema, P.; Anagnostopoulos, G. C.; Karanikola, I. +2 more

In this study, we concentrate on the examination of the quasi-periodic behavior of 0.5-1.6 MeV(∼40-400 keV) protons (electrons) and of relativistic (>16 MeV) electrons, observed at Jupiter by two different experiments onboard Ulysses, the HI-SCALE and COSPIN, respectively, within the large-scale south duskside magnetopause boundary layer (MPBL)…

2004 Planetary and Space Science
Ulysses 19
Visible and infrared spectroscopy of minerals and mixtures with the OMEGA/MARS-EXPRESS instrument
DOI: 10.1016/j.pss.2003.08.014 Bibcode: 2004P&SS...52..133B

Gendrin, Aline; Bibring, Jean-Pierre; Langevin, Yves +4 more

We present the reflectance measurements made with OMEGA during ground calibration on a selection of minerals and mixtures considered as candidates for constituents of the Mars surface. OMEGA is the visible and infrared mapping spectrometer designed to fly on-board the ESA/MARS-EXPRESS probe. These measurements allow to evaluate the instrument perf…

2004 Planetary and Space Science
MEx 18
The microscope for Beagle 2
DOI: 10.1016/j.pss.2004.02.008 Bibcode: 2004P&SS...52..853T

Keller, H. U.; Hviid, S. F.; Thomas, N. +13 more

The microscope for the Beagle 2 lander, which was launched as part of the European Space Agency's Mars Express mission on 2 June 2003, will provide images of the Martian surface at around 6 µm resolution. It will provide optical images of the surface of Mars at a resolution 5 times higher than any other experiment currently planned. The devi…

2004 Planetary and Space Science
MEx 17
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