Publications
403 results found
Giampieri G, Dougherty MK, Russell CT, et al., 2005, Reply to comment by M. L. Kaiser et al. on "Rotation rate of Saturn's interior from magnetic field observations'', GEOPHYSICAL RESEARCH LETTERS, Vol: 32, ISSN: 0094-8276
Blanc M, Moura D, Alibert Y, et al., 2005, Tracing the origins of the solar system, Pages: 213-224, ISSN: 0379-6566
All contemporary objects of our Solar System emerged from a solar nebula which existed 4.5 billion years ago, and whose dynamical and thermo-chemical evolution led to the condensation of solids, then to the emergence of different types of planetesimals, and finally to the accretion of solid cores and to the formation of our planets. Space exploration makes it possible today to visit the different classes of solar system objects and retrieve key information which can help us to trace back the evolutionary path of the solar system, from its origins in the Solar Nebula to its present configuration and the likely development of habitats in planetary objects. We propose three un-ordered priorities for the space programme in this perspective: 1 - access to remaining pristine material in the solar system (interplanetary dust and small bodies); 2 - in-depth exploration of the systems of giant planets; 3 - in-situ analysis of some of the physical mechanisms relevant to planetary formation in the contemporary rings and plasma environments of giant planets. This research subject, which strongly connects our solar system and its objects to exoplanets and other planetary systems, is a very promising contribution to the progressive build-up of a synthetic view of their formation and evolution scenarios. It is a central element in the build-up of a "Cosmic Vision" of our own solar system. We show how the major scientific questions related to this broad theme can be translated into specific mission targets and measurement objectives, and grouped into a "short list" of key space missions. This short list forms an ideal basis to elaborate a multi-decadal endeavour to explore the outer solar system. Most of these missions, while addressing the specific question of solar system origin, also are of major interest for comparative planetology and exo-astrobiology. While a few can be implemented in a purely European context, most of these missions can be accomplished on
Bertucci C, Achilleos N, Russell CT, et al., 2005, Bow shock and upstream waves at Jupiter and Saturn: Cassini magnetometer observations, 4th Annual IGPP International Astrophysics Conference, Publisher: AMER INST PHYSICS, Pages: 109-115, ISSN: 0094-243X
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- Citations: 2
Jackman CM, Achilleos N, Bunce EJ, et al., 2004, Interplanetary magnetic field at ∼ 9 AU during the declining phase of the solar cycle and its implications for Saturn's magnetospheric dynamics -: art. no. A11203, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 109, ISSN: 2169-9380
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- Citations: 106
Giampieri G, Dougherty MK, 2004, Rotation rate of Saturn's interior from magnetic field observations, GEOPHYSICAL RESEARCH LETTERS, Vol: 31, ISSN: 0094-8276
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- Citations: 25
Krupp N, Woch J, Lagg A, et al., 2004, Energetic particle observations in the vicinity of Jupiter: Cassini MIMI/LEMMS results, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 109, ISSN: 2169-9380
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- Citations: 32
Hanlon PG, Dougherty MK, Krupp N, et al., 2004, Dual spacecraft observations of a compression event within the Jovian magnetosphere:: Signatures of externally triggered supercorotation? -: art. no. A09S09, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 109, ISSN: 2169-9380
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- Citations: 27
Lario D, Livi S, Roelof EC, et al., 2004, Heliospheric energetic particle observations by the Cassini spacecraft: Correlation with 1 AU observations, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 109, ISSN: 2169-9380
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- Citations: 14
Achilleos N, Dougherty MK, Young DT, et al., 2004, Magnetic signatures of Jupiter's bow shock during the Cassini flyby, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 109, ISSN: 2169-9380
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- Citations: 7
Hanlon PG, Dougherty MK, Forsyth RJ, et al., 2004, On the evolution of the solar wind between 1 and 5 AU at the time of the Cassini Jupiter flyby:: Multispacecraft observations of interplanetary coronal mass ejections including the formation of a merged interaction region -: art. no. A09S03, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 109, ISSN: 2169-9380
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- Citations: 19
Tomás A, Woch J, Krupp N, et al., 2004, Changes of the energetic particles characteristics in the inner part of the Jovian magnetosphere:: a topological study, Euroconference on Jupiter after Galileo and Cassini, Publisher: PERGAMON-ELSEVIER SCIENCE LTD, Pages: 491-498, ISSN: 0032-0633
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- Citations: 20
Giampieri G, Dougherty MK, 2004, Modelling of the ring current in Saturn's magnetosphere, ANNALES GEOPHYSICAE, Vol: 22, Pages: 653-659, ISSN: 0992-7689
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- Citations: 43
Dougherty MK, Kellock S, Southwood DJ, et al., 2004, The Cassini magnetic field investigation, SPACE SCIENCE REVIEWS, Vol: 114, Pages: 331-383, ISSN: 0038-6308
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- Citations: 441
Jones GH, Balogh A, Russell CT, et al., 2003, Possible distortion of the interplanetary magnetic field by the dust trail of comet 122P/de Vico, ASTROPHYSICAL JOURNAL, Vol: 597, Pages: L61-L64, ISSN: 0004-637X
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- Citations: 10
Bogdanov AT, Glassmeier KH, Musmann G, et al., 2003, Ion cyclotron waves in the Earth's magnetotail during CASSINI's Earth swing-by, ANNALES GEOPHYSICAE, Vol: 21, Pages: 2043-2057, ISSN: 0992-7689
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- Citations: 7
Espinosa SA, Southwood DJ, Dougherty MK, 2003, How can Saturn impose its rotation period in a noncorotating magnetosphere?, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 108, ISSN: 2169-9380
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- Citations: 74
Espinosa SA, Southwood DJ, Dougherty MK, 2003, Reanalysis of Saturn's magnetospheric field data view of spin-periodic perturbations, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 108, ISSN: 2169-9380
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- Citations: 55
Szego K, Young DT, Bagdonat T, et al., 2003, A pre-shock event at Jupiter on 30 January 2001, Journal of Geophysical Research
Kellogg PJ, Dougherty MK, Forsyth RJ, et al., 2003, Electric fluctuations and ion isotropy, Melville, 10th international solar wind conference, Pisa, Italy, 17 - 21 June 2002, Publisher: American Institute of Physics, Pages: 383-388
Kellogg PJ, Gurnett DA, Hospodarsky GB, et al., 2003, Ion isotropy and ion resonant waves in the solar wind: corrected Cassini observations (Article no. 1045), Journal of Geophysical Research.Space Physics, Vol: 108, ISSN: 0148-0227
Kellogg PJ, Dougherty MK, Forsyth RJ, et al., 2003, Electric fluctuations and ion isotropy, Melville, 10th international solar wind conference, Pisa, Italy, 17 - 21 June 2002, Publisher: American Institute of Physics, Pages: 383-388
Szego K, Young DT, Barraclough BL, et al., 2003, Cassini Plasma Spectrometer measurements of Jovian bow shock structure, Journal of Geophysical Research.Space Physics, Vol: 109, Pages: 1287-1, ISSN: 0148-0227
André N, Erdös G, Dougherty M, 2002, Overview of mirror mode fluctuations in the jovian dusk magnetosheath:: Cassini magnetometer observations -: art. no. 1980, GEOPHYSICAL RESEARCH LETTERS, Vol: 29, ISSN: 0094-8276
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- Citations: 11
Bhardwaj A, Gladstone GR, Elsner RF, et al., 2002, Soft x-ray emissions from planets, moons, and comets, Pages: 215-226, ISSN: 0379-6566
A wide variety of solar system bodies are now known to radiate in the soft x-ray energy (<5 keV) regime. These include planets (Earth, Jupiter, Venus, Saturn, Mars): bodies having thick atmospheres, with or without intrinsic magnetic field; planetary satellites (Moon, Io, Europa, Ganymede): bodies with thin or no atmospheres; and comets and Io plasma torus: bodies having extended tenuous atmospheres. Several different mechanisms have been proposed to explain the generation of soft x-rays from these objects, whereas in the hard x-ray energy range (>10 keV) x-rays mainly result from the electron bremsstrahlung process. In this paper we present a brief review of the x-ray observations on each of the planetary bodies and discuss their characteristics and proposed source mechanisms.
Kurth WS, Gurnett DA, Hospodarsky GB, et al., 2002, The dusk flank of Jupiter's magnetosphere, NATURE, Vol: 415, Pages: 991-994, ISSN: 0028-0836
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- Citations: 38
Gurnett DA, Kurth WS, Hospodarsky GB, et al., 2002, Control of Jupiter's radio emission and aurorae by the solar wind, NATURE, Vol: 415, Pages: 985-987, ISSN: 0028-0836
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- Citations: 124
Gladstone GR, Waite JH, Grodent D, et al., 2002, A pulsating auroral X-ray hot spot on Jupiter, NATURE, Vol: 415, Pages: 1000-1003, ISSN: 0028-0836
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- Citations: 165
Blanc M, Bolton S, Bradley J, et al., 2002, Magnetospheric and plasma science with Cassini-Huygens, SPACE SCIENCE REVIEWS, Vol: 104, Pages: 253-346, ISSN: 0038-6308
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- Citations: 43
Lagg A, Krupp N, Livi S, et al., 2001, Energetic particle measurements during the Earth swing-by of the Cassini spacecraft in August 1999, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 106, Pages: 30209-30222, ISSN: 2169-9380
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- Citations: 6
Tsurutani BT, Smith EJ, Burton ME, et al., 2001, Oblique "1-Hz" whistler mode waves in an electron foreshock: The Cassini near-Earth encounter, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 106, Pages: 30223-30238, ISSN: 2169-9380
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- Citations: 12
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