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Galileo dust data from the jovian system: 2000 to 2003
DOI: 10.1016/j.pss.2010.03.003 Bibcode: 2010P&SS...58..965K

Krüger, H.; Srama, R.; Hamilton, D. P. +17 more

The Galileo spacecraft was the first man-made satellite of Jupiter, orbiting the planet between December 1995 and September 2003. The spacecraft was equipped with a highly sensitive dust detector that monitored the jovian dust environment between approximately 2 and 370 RJ (jovian radius RJ=71 492 km). The Galileo dust detect…

2010 Planetary and Space Science
Ulysses 10
The light curve of asteroid 2867 Steins measured by VIRTIS-M during the Rosetta fly-by
DOI: 10.1016/j.pss.2010.03.019 Bibcode: 2010P&SS...58.1066T

Mottola, S.; Barucci, M. A.; Erard, S. +11 more

On 5 September 2008, the Rosetta spacecraft encountered the asteroid 2867 Steins on its way to the comet 67P/Churyumov-Gerasimenko. This was the first of two planned asteroid fly-bys performed by the probe, the second fly-by being with the much larger asteroid 21 Lutetia in July 2010. The VIRTIS imaging spectrometer (IFOV 0.250 mrad, overall spect…

2010 Planetary and Space Science
Rosetta 8
Optical properties of aerosols in Titan’s atmosphere: Large fluffy aggregates
DOI: 10.1016/j.pss.2010.08.002 Bibcode: 2010P&SS...58.1802S

Keller, H. U.; Rodin, A. V.; Skorov, Yu. V.

Scattering properties of large ( N>2000) aggregates of monomers as found in Titan's atmosphere during the descent of the Cassini/Huygens probe are numerically calculated. We extend our previous quantitative analysis of small aggregates ( N≤256) to verify the obtained conclusions. To calculate the light scattering of such big non-spherical aggre…

2010 Planetary and Space Science
Cassini 8
Evidence for surface variegation in Rosetta OSIRIS images of asteroid 2867 Šteins
DOI: 10.1016/j.pss.2010.04.020 Bibcode: 2010P&SS...58.1107S

Sierks, H.; Keller, H. U.; Hviid, S. F. +4 more

The OSIRIS camera onboard Rosetta successfully acquired images of asteroid 2867 Steins through a variety of color filters during the flyby on 5 September 2008. The best images of this 5 km diameter asteroid have a resolution of 78 m per pixel. We process the images by deconvolving with the point spread function and enlarging through the Mitchell-N…

2010 Planetary and Space Science
Rosetta 8
Attitude and angular rates of planetary probes during atmospheric descent: Implications for imaging
DOI: 10.1016/j.pss.2010.01.003 Bibcode: 2010P&SS...58..838L

Lorenz, Ralph D.

Attitude dynamics data from planetary missions are reviewed to obtain a zeroth-order expectation on the tilts and angular rates to be expected on atmospheric probes during descent: these rates are a strong driver on descent imager design. While recent Mars missions have been equipped with capable inertial measurements, attitude measurements for mi…

2010 Planetary and Space Science
Huygens 8
A new approach for estimating Titan's electron conductivity based on data from relaxation probe sensors on the Huygens experiment
DOI: 10.1016/j.pss.2010.09.014 Bibcode: 2010P&SS...58.1945M

Rodrigo, R.; Fulchignoni, M.; Ferri, F. +15 more

The Huygens Probe measured the electrical conductivity of Titan atmosphere from about 140 km down to the surface, employing relaxation and mutual impedance techniques. Previous analyses have shown some differences on the conductivity measurements obtained with two independent sensors - relaxation probe (RP) and mutual impedance probe (MIP). A 20-f…

2010 Planetary and Space Science
Huygens 8
Analysis of disturbances in the Planetary Fourier Spectrometer through numerical modeling
DOI: 10.1016/j.pss.2010.01.011 Bibcode: 2010P&SS...58..864C

Saggin, Bortolino; Comolli, Lorenzo

Fourier transform spectrometers are instruments with high sensitivity to many kinds of disturbances. This study started from the analysis of the disturbances related to mechanical vibrations on the PFS FTIR spectrometer to show how the measured spectra can differ from the actual ones. The complete study, more in general, accounts for the character…

2010 Planetary and Space Science
MEx 7
Analysis of two sections of Shalbatana Vallis’ tributary channels
DOI: 10.1016/j.pss.2010.10.001 Bibcode: 2010P&SS...58.2008K

Kereszturi, Akos

Six tributaries of Shalbatana outflow channel were analyzed based on visible imagery by THEMIS, MOC, HRSC, and HiRISE, as well as on topographic data by MOLA. Two different sections could be identified on the tributaries: the upper and the lower reaches. The upper reaches are shallow, showing U-shaped cross-sectional profiles. Their bottom level i…

2010 Planetary and Space Science
MEx 6
Reconstruction of nonmonotonic electron density profiles of the Martian topside ionosphere
DOI: 10.1016/j.pss.2010.06.011 Bibcode: 2010P&SS...58.1391Z

Wang, X. -D.; Zou, H.; Wang, J. -S. +1 more

One of the problems in reconstructing the real ionosphere from an ionogram is the occurrence of a 'valley,' where electron density decreases with altitude and make a non-monotonic profile. For the case of the Earth ionosphere, the ordinary and extraordinary ray data, accompanied with an empirical model, based on the observations, are necessary to …

2010 Planetary and Space Science
MEx 4
Trajectory and atmospheric structure from entry probes: Demonstration of a real-time reconstruction technique using a simple direct-to-Earth radio link
DOI: 10.1016/j.pss.2010.10.005 Bibcode: 2010P&SS...58.2044W

Withers, Paul

The reconstruction of the trajectory and atmospheric structure associated with an entry probe has traditionally relied upon onboard accelerometer measurements. Here we outline an equivalent reconstruction technique that uses Doppler-shifted direct-to-Earth transmissions instead. A critical assumption is that the entry probe's angle of attack is ze…

2010 Planetary and Space Science
Huygens 3