Publications
166 results found
Galand M, Yelle R, Cui J, et al., 2010, Ionization sources in Titan's deep ionosphere, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 115, ISSN: 2169-9380
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- Citations: 42
Cui J, Galand M, Yelle RV, et al., 2010, Ion transport in Titan's upper atmosphere, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 115, ISSN: 2169-9380
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- Citations: 45
Chakrabarti S, Galand M, 2010, Aurora on Jupiter: A Magnetic Connection with the Sun and the Medicean Moons, 269th Symposium of the International Astronomical Union, Publisher: CAMBRIDGE UNIV PRESS, Pages: 71-79, ISSN: 1743-9213
Moore L, Galand M, Mueller-Wodarg I, et al., 2009, Response of Saturn's ionosphere to solar radiation: Testing parameterizations for thermal electron heating and secondary ionization processes, PLANETARY AND SPACE SCIENCE, Vol: 57, Pages: 1699-1705, ISSN: 0032-0633
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- Citations: 25
Agren K, Wahlund J-E, Garnier P, et al., 2009, On the ionospheric structure of Titan, PLANETARY AND SPACE SCIENCE, Vol: 57, Pages: 1821-1827, ISSN: 0032-0633
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- Citations: 92
Wahlund J-E, Galand M, Mueller-Wodarg I, et al., 2009, On the amount of heavy molecular ions in Titan's ionosphere, PLANETARY AND SPACE SCIENCE, Vol: 57, Pages: 1857-1865, ISSN: 0032-0633
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- Citations: 66
Vuitton V, Lavvas P, Yelle RV, et al., 2009, Negative ion chemistry in Titan's upper atmosphere, PLANETARY AND SPACE SCIENCE, Vol: 57, Pages: 1558-1572, ISSN: 0032-0633
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- Citations: 205
Galand M, Moore L, Charnay B, et al., 2009, Solar primary and secondary ionization at Saturn, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 114, ISSN: 2169-9380
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- Citations: 47
Cui J, Galand M, Yelle RV, et al., 2009, Diurnal variations of Titan's ionosphere, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 114, ISSN: 2169-9380
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- Citations: 72
Crooker NU, Galand M, 2009, Heliophysics: A field with its own universal laws, Eos, Vol: 90, ISSN: 0096-3941
Coustenis A, Atreya SK, Balint T, et al., 2009, TandEM: Titan and Enceladus mission, EXPERIMENTAL ASTRONOMY, Vol: 23, Pages: 893-946, ISSN: 0922-6435
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- Citations: 69
Moore L, Galand M, Mueller-Wodarg I, et al., 2008, Plasma temperatures in Saturn's ionosphere, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 113, ISSN: 2169-9380
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- Citations: 33
Huestis DL, Bougher SW, Fox JL, et al., 2008, Cross Sections and Reaction Rates for Comparative Planetary Aeronomy, SPACE SCIENCE REVIEWS, Vol: 139, Pages: 63-105, ISSN: 0038-6308
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- Citations: 68
Fox JL, Galand MI, Johnson RE, 2008, Energy Deposition in Planetary Atmospheres by Charged Particles and Solar Photons, SPACE SCIENCE REVIEWS, Vol: 139, Pages: 3-62, ISSN: 0038-6308
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- Citations: 75
Branduardi-Raymont G, Elsner RF, Galand M, et al., 2008, Spectral morphology of the X-ray emission from Jupiter's aurorae, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 113, ISSN: 2169-9380
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- Citations: 66
Agren K, Wahlund J-E, Modolo R, et al., 2007, On magnetospheric electron impact ionisation and dynamics in Titan's ram-side and polar ionosphere - a Cassini case study, ANNALES GEOPHYSICAE, Vol: 25, Pages: 2359-2369, ISSN: 0992-7689
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- Citations: 74
Galand M, Yelle RV, Coates AJ, et al., 2006, Electron temperature of Titan's sunlit ionosphere, GEOPHYSICAL RESEARCH LETTERS, Vol: 33, ISSN: 0094-8276
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- Citations: 61
Galand M, Chakrabarti S, 2006, Proton aurora observed from the ground, JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, Vol: 68, Pages: 1488-1501, ISSN: 1364-6826
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- Citations: 20
Robertson SC, Lanchester BS, Galand M, et al., 2006, First ground-based optical analysis of H<sub>β</sub> Doppler profiles close to local noon in the cusp, ANNALES GEOPHYSICAE, Vol: 24, Pages: 2543-2552, ISSN: 0992-7689
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- Citations: 8
Galand M, Bhardwaj A, Chakrabarti S, 2006, On the importance of the cross-body approach in planetary aeronomy, Advances in Geosciences, Vol: Volume 2: Solar Terrestrial, Pages: 239-248, ISSN: 1680-7340
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
Ivchenko N, Rees MH, Lanchester BS, et al., 2004, Observation of O<sup>+</sup> (<sup>4</sup>P-<sup>4</sup>D<sup>0</sup>) lines in electron aurora over Svalbard, Annales Geophysicae, Vol: 22, Pages: 2805-2817, ISSN: 0992-7689
This work reports on observations of 0+ lines in aurora over Svalbard, Norway. The Spectrographic Imaging Facility measures auroral spectra in three wavelength intervals (Hβ, N+2 1N(0,2) and N+2 1N(1,3) . The oxygen ion 4P-4D0 multiplet (4639-4696 Å) is blended with the N+2 1N(1,3 band. It is found that in electron aurora, the brightness of this multiplet, is on average, about 0. 1 of the N+2 1N(0,2) total brightness. A joint optical and incoherent scatter radar study of an electron aurora event shows that the ratio is enhanced when the ionisation in the upper E-layer (140-190 km) is significant with respect to the E-layer peak below 130 km. Rayed arcs were observed on one such occasion, whereas on other occasions the auroral intensity was below the threshold of the imager. A one-dimensional electron transport model is used to estimate the cross section for production of the multiplet in electron collisions, yielding 0. 18 × 10-18 cm2. © European Geosciences Union 2004.
Galand M, Baumgardner J, Pallamraju D, et al., 2004, Spectral imaging of proton aurora and twilight at Tromso, Norway, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 109, ISSN: 2169-9380
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- Citations: 19
Ivchenko N, Galand M, Lanchester BS, et al., 2004, Observation of O<SUP>+4</SUP>P-<SUP>4</SUP>D<SUP>0</SUP> lines in proton aurora over Svalbard -: art. no. L10807, GEOPHYSICAL RESEARCH LETTERS, Vol: 31, ISSN: 0094-8276
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- Citations: 6
Galand M, Lummerzheim D, 2004, Contribution of proton precipitation to space-based auroral FUV observations, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 109, ISSN: 2169-9380
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- Citations: 23
Ivchenko N, Rees MH, Lanchester BS, et al., 2004, Observation of O<SUP>+</SUP> (<SUP>4</SUP>P-<SUP>4</SUP>D<SUP>0</SUP>) lines in electron aurora over Svalbard, ANNALES GEOPHYSICAE, Vol: 22, Pages: 2805-2817, ISSN: 0992-7689
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- Citations: 6
Lanchester BS, Galand M, Robertson SC, et al., 2003, High resolution measurements and modeling of auroral hydrogen emission line profiles, ANNALES GEOPHYSICAE, Vol: 21, Pages: 1629-1643, ISSN: 0992-7689
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- Citations: 10
Galand M, Lummerzheim D, Stephan AW, et al., 2002, Electron and proton aurora observed spectroscopically in the far ultraviolet, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 107, ISSN: 2169-9380
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- Citations: 21
Galand M, Chakrabarti S, 2002, Auroral processes in the solar system, Atmospheres in the solar system: comparative aeronomy, Editors: Mendillo, Nagy, Waite, Publisher: American Geophysical Union, Pages: 55-76, ISBN: 9780875909899
Vontrat-Reberac A, Fontaine D, Blelly PL, et al., 2001, Theoretical predictions of the effect of cusp and dayside precipitation on the polar ionosphere, JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Vol: 106, Pages: 28857-28865, ISSN: 2169-9380
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- Citations: 26
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