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Investigation of Titan Aerogravity Assist for Capture into Orbit About Saturn
DOI: 10.2514/1.9274 Bibcode: 2006JSpRo..43..231L

Lyne, James; Ramsey, Philip

2006 Journal of Spacecraft and Rockets
Cassini 5
XMM-Newton Detection of the Supernova Remnant G337.2+0.1
DOI: 10.1086/510329 Bibcode: 2006ApJ...653L..41C

Albacete Colombo, Juan F.; Benaglia, Paula; Combi, Jorge A. +1 more

We report the first XMM-Newton detection of the SNR candidate G337.2+0.1 (=AX J1635.9-4719). The object shows centrally filled and diffuse X-ray emission. The emission peaks in the hard 3.0-10.0 keV band. A spatially resolved spectral study confirms that the column density of the central part of the SNR is about NH~5.9(+/-1.5)×1022…

2006 The Astrophysical Journal
XMM-Newton 5
Planetary science: Saturn's bared mini-moons
DOI: 10.1038/440614a Bibcode: 2006Natur.440..614S

Schmidt, Jürgen; Spahn, Frank

Propeller-shaped structures seem to reveal the presence of moonlets, about 100 metres in diameter, embedded in Saturn's rings. This discovery adds to our picture of how the rings formed and are evolving.

2006 Nature
Cassini 5
Neon dewar for the X-ray spectrometer onboard Suzaku
DOI: 10.1016/j.nima.2005.12.093 Bibcode: 2006NIMPA.559..648F

Mitsuda, K.; Kelley, R. L.; Fujimoto, R. +6 more

The X-ray spectrometer (XRS) onboard Suzaku is the first X-ray microcalorimeter array in orbit. The sensor array is operated at 60 mK, which is attained by an adiabatic demagnetization refrigerator and superfluid liquid helium. The neon dewar is a vacuum-insulated container for the XRS. The requirements for the XRS dewar are to maintain the detect…

2006 Nuclear Instruments and Methods in Physics Research A
Suzaku 5
Titan, Fractals, and Filtering of Cassini Altimeter Data
DOI: 10.1109/TGRS.2006.872152 Bibcode: 2006ITGRS..44.2055F

Callahan, P.; Wall, S. D.; Riccio, D. +2 more

2006 IEEE Transactions on Geoscience and Remote Sensing
Cassini 5
An ionized disc reflection component for the X-ray spectrum of NGC 4051 and IRAS13224-3809?
DOI: 10.1002/asna.200610691 Bibcode: 2006AN....327.1055P

Cappi, M.; Ponti, G.; Fabian, A. C. +2 more

A spectral variability study of the two Narrow Line Seyfert 1 galaxies NGC 4051 and IRAS13224-3809 is presented. Both sources show a high degree of flux and spectral variability. The nuclear emission, lightly absorbed by warm material, has been decomposed into a direct power law emission and an ionized disc reflection plus constant emission from d…

2006 Astronomische Nachrichten
XMM-Newton 5
Spin of Planetary Probes in Atmospheric Flight
Bibcode: 2006JBIS...59..273L

Lorenz, R. D.

Probes that enter planetary atmospheres are often spun during entry or descent for a variety of reasons. Their spin rate histories are influenced by often subtle effects. The spin requirements, control methods and flight experience from planetary and earth entry missions are reviewed. An interaction of the probe aerodynamic wake with a drogue para…

2006 Journal of the British Interplanetary Society
Huygens 5
Chemometric evaluation of time-of-flight secondary ion mass spectrometry data of minerals in the frame of futurein situ analyses of cometary material by COSIMA onboard ROSETTA
DOI: 10.1002/rcm.2448 Bibcode: 2006RCMS...20.1361E

Silén, Johan; Thirkell, Laurent; Varmuza, Kurt +5 more

2006 Rapid Communications in Mass Spectrometry
Rosetta 5
Analysis of the Interaction between Low-Frequency Waves and Ions in the High-Altitude Cusp Region Observed by Satellite Cluster
DOI: 10.1088/0256-307X/23/5/079 Bibcode: 2006ChPhL..23.1351D

Balogh, A.; Reme, H.; Cao, Jin-Bin +8 more

The energy transfer between ions (protons) and low frequency waves (LFWs) in the frequency range f1 from 0.3 to 10 Hz is observed by Cluster crossing the high-altitude polar cusp. The energy transfer between low frequency waves and ions has two means. One is that the energy is transferred from low frequency waves to ions and ions energy…

2006 Chinese Physics Letters
Cluster 5
Early Inner Solar System Impactors: Physical Properties of Comet Nuclei and Dust Particles Revisited
DOI: 10.1007/s11084-006-9032-7 Bibcode: 2006OLEB...36..507L

Lasue, J.; Levasseur-Regourd, A. C.; Desvoivres, E.

During the epoch of early bombardment, terrestrial planets have been heavily impacted by cometary nuclei and cometary dust particles progressively injected in the interplanetary medium. Stardust and Deep Impact missions confirm that the nuclei are porous, loosely consolidated objects, with densities below 1,000 kg m-3, and that they oft…

2006 Origins of Life and Evolution of the Biosphere
Giotto 5