Search Publications

RPC-MIP: the Mutual Impedance Probe of the Rosetta Plasma Consortium
DOI: 10.1007/s11214-006-9005-1 Bibcode: 2007SSRv..128..713T

Schmidt, W.; Eriksson, A.; Décréau, P. M. E. +18 more

The main objective of the Mutual Impedance Probe (MIP), part of the Rosetta Plasma Consortium (RPC), is to measure the electron density and temperature of Comet 67P/Churyumov-Gerasimenko’s coma, in particular inside the contact surface. Furthermore, MIP will determine the bulk velocity of the ionised outflowing atmosphere, define the spectral dist…

2007 Space Science Reviews
Rosetta 104
RPC-ICA: The Ion Composition Analyzer of the Rosetta Plasma Consortium
DOI: 10.1007/s11214-006-9031-z Bibcode: 2007SSRv..128..671N

Kallio, E.; Fedorov, A.; Koskinen, H. +9 more

The Ion Composition Analyzer (ICA) is part of the Rosetta Plasma Consortium (RPC). ICA is designed to measure the three-dimensional distribution function of positive ions in order to study the interaction between the solar wind and cometary particles. The instrument has a mass resolution high enough to resolve the major species such as protons, he…

2007 Space Science Reviews
Rosetta 104
The Comet Nucleus Sounding Experiment by Radiowave Transmission (CONSERT): A Short Description of the Instrument and of the Commissioning Stages
DOI: 10.1007/s11214-006-9034-9 Bibcode: 2007SSRv..128..413K

Plettemeier, D.; Picardi, G.; Elachi, C. +12 more

The primary scientific goal of the CONSERT experiment on the Rosetta space mission is to investigate the deep interior of the nucleus of comet 67/P Churyumov-Gerasimenko. This will be achieved through the use of long wavelength radio-waves, transmitted from the orbiter and returned from the lander. In this overview, a description of the instrument…

2007 Space Science Reviews
Rosetta 102
Cosac, The Cometary Sampling and Composition Experiment on Philae
DOI: 10.1007/s11214-006-9000-6 Bibcode: 2007SSRv..128..257G

Szopa, Cyril; Roll, Reinhard; Goesmann, Fred +7 more

Comets are thought to preserve the most pristine material currently present in the solar system, as they are formed by agglomeration of dust particles in the solar nebula, far from the Sun, and their interiors have remained cold. By approaching the Sun, volatile components and dust particles are released forming the cometary coma. During the phase…

2007 Space Science Reviews
Rosetta 84
A Portrait of the Nucleus of Comet 67P/Churyumov-Gerasimenko
DOI: 10.1007/s11214-007-9146-x Bibcode: 2007SSRv..128...23L

Toth, Imre; Lamy, Philippe L.; Gutiérrez, Pedro +5 more

In 2003, comet 67P/Churyumov-Gerasimenko was selected as the new target of the Rosetta mission as the most suitable alternative to the original target, comet 46P/Wirtanen, on the basis of orbital considerations even though very little was known about the physical properties of its nucleus. In a matter of a few years and based on highly focused obs…

2007 Space Science Reviews
Rosetta eHST 80
The Plasma Environment of Comet 67P/Churyumov-Gerasimenko Throughout the Rosetta Main Mission
DOI: 10.1007/s11214-006-9142-6 Bibcode: 2007SSRv..128..133H

Alexander, C.; Combi, M. R.; Gombosi, T. I. +6 more

The plasma environment of comet 67P/Churyumov-Gerasimenko, the Rosetta mission target comet, is explored over a range of heliocentric distances throughout the mission: 3.25 AU (Rosetta instruments on), 2.7 AU (Lander down), 2.0 AU, and 1.3 AU (perihelion). Because of the large range of gas production rates, we have used both a fluid-based magnetoh…

2007 Space Science Reviews
Rosetta 80
Alice: The rosetta Ultraviolet Imaging Spectrograph
DOI: 10.1007/s11214-006-9035-8 Bibcode: 2007SSRv..128..507S

Parker, Joel Wm.; Stern, S. A.; Feldman, P. D. +8 more

We describe the design, performance and scientific objectives of the NASA-funded ALICE instrument aboard the ESA Rosetta asteroid flyby/comet rendezvous mission. ALICE is a lightweight, low-power, and low-cost imaging spectrograph optimized for cometary far-ultraviolet (FUV) spectroscopy. It will be the first UV spectrograph to study a comet at cl…

2007 Space Science Reviews
IUE Rosetta 70
The Grain Impact Analyser and Dust Accumulator (GIADA) Experiment for the Rosetta Mission: Design, Performances and First Results
DOI: 10.1007/s11214-006-9038-5 Bibcode: 2007SSRv..128..803C

Fulle, M.; Rodriguez, J.; Colangeli, L. +13 more

The Grain Impact Analyser and Dust Accumulator (GIADA) onboard the ROSETTA mission to comet 67P/Churyumov-Gerasimenko is devoted to study the cometary dust environment. Thanks to the rendezvous configuration of the mission, GIADA will be plunged in the dust environment of the coma and will be able to explore dust flux evolution and grain dynamic p…

2007 Space Science Reviews
Rosetta 69
Mupus A Thermal and Mechanical Properties Probe for the Rosetta Lander Philae
DOI: 10.1007/s11214-006-9081-2 Bibcode: 2007SSRv..128..339S

Banaszkiewicz, Marek; Zarnecki, John C.; Spohn, Tilman +14 more

MUPUS, the multi purpose sensor package onboard the Rosetta lander PHILAE, will measure the energy balance and the physical parameters in the near-surface layers - up to about 30 cm depth- of the nucleus of Rosetta's target comet Churyumov-Gerasimenko. Moreover it will monitor changes in these parameters over time as the comet approaches the sun. …

2007 Space Science Reviews
Rosetta 69
The Composition of the Solar Wind in Polar Coronal Holes
DOI: 10.1007/s11214-007-9189-z Bibcode: 2007SSRv..130..139G

Gloeckler, George; Geiss, Johannes

The solar wind charge state and elemental compositions have been measured with the Solar Wind Ion Composition Spectrometers (SWICS) on Ulysses and ACE for a combined period of about 25 years. This most extensive data set includes all varieties of solar wind flows and extends over more than one solar cycle. With SWICS the abundances of all charge s…

2007 Space Science Reviews
Ulysses 63