Cyril.bib

@article{CSW2016CX,
  author = {{Simon Wedlund, C.} and {Kallio, E.} and {Alho, M.} and {Nilsson, H.} and {Stenberg Wieser, G.} and {Gunell, H.} and {Behar, E.} and {Pusa, J.} and {Gronoff, G.}},
  title = {The atmosphere of comet 67P/Churyumov-Gerasimenko diagnosed by charge-exchanged solar wind alpha particles},
  doi = {10.1051/0004-6361/201527532},
  url = {http://dx.doi.org/10.1051/0004-6361/201527532},
  journal = {A&A},
  year = 2016,
  volume = 587,
  pages = {A154},
  month = {}
}
@article{Nilsson2015Evolution,
  author = {{Nilsson}, H. and {Stenberg Wieser}, G. and {Behar}, E. and {Simon Wedlund}, C. and {Kallio}, E. and {Edberg}, N. and {Eriksson}, A.~I. and {Yamauchi}, M. and {Koenders}, C. and {Wieser}, M. and {Lundin}, R. and {Barabash}, S. and {Mandt}, K. and {Burch}, J.~L. and {Goldstein}, R. and {Mokashi}, P. and {Carr}, C. and {Cupido}, E. and {Fox}, P.~T. and {...}},
  title = {Evolution of the ion environment of comet {67P/Churyumov-Gerasimenko} - Observations between 3.6 and 2.0 AU},
  doi = {10.1051/0004-6361/201526142},
  url = {http://dx.doi.org/10.1051/0004-6361/201526142},
  journal = {A&A},
  year = 2015
}
@article{Gunell201513,
  title = {Acceleration of ions and nano dust at a comet in the solar wind },
  journal = {Planetary and Space Science },
  volume = {119},
  number = {},
  pages = {13 - 23},
  year = {2015},
  note = {},
  issn = {0032-0633},
  doi = {http://dx.doi.org/10.1016/j.pss.2015.08.019},
  url = {http://www.sciencedirect.com/science/article/pii/S0032063315002536},
  author = {H. Gunell and I. Mann and C. Simon Wedlund and E. Kallio and M. Alho and H. Nilsson and J. De Keyser and F. Dhooghe and R. Maggiolo},
  keywords = {Comet},
  keywords = {Dust},
  keywords = {Hybrid model },
  abstract = {Abstract A quasi-neutral hybrid simulation of the interaction of the solar wind with the atmosphere of a comet is used together with a test particle simulation of cometary ions and dust to compute trajectories and velocity distribution functions of charged particles, starting outside the diamagnetic cavity at 150 km cometocentric distance. The simulations are run with parameters suited to make predictions for comet 67P/Churyumov–Gerasimenko when it is at a heliocentric distance of 1.45 AU. It is found that the shape of the ion trajectories depends on the location of the source, and that a velocity distribution that is observed at a given point in space is influenced by the spatial structure of the source. Charged dust grains with radii in the 1–10 nm range are accelerated from the nucleus to a distance of 2.9 × 10 4 km in between 15 min and 2 h approximately. Dust particles smaller than 10 nm in radius are accelerated to speeds over 10 km/s. }
}
@article{Nilsson23012015,
  author = {Nilsson, Hans and Stenberg Wieser, Gabriella and Behar, Etienne and Wedlund, Cyril Simon and Gunell, Herbert and Yamauchi, Masatoshi and Lundin, Rickard and Barabash, Stas and Wieser, Martin and Carr, Chris and Cupido, Emanuele and Burch, James L. and Fedorov, Andrei and Sauvaud, Jean-Andr\'{e} and Koskinen, Hannu and Kallio, Esa and Lebreton, Jean-Pierre and Eriksson, Anders and Edberg, Niklas and Goldstein, Raymond and Henri, Pierre and Koenders, Christoph and Mokashi, Prachet and Nemeth, Zoltan and Richter, Ingo and Szego, Karoly and Volwerk, Martin and Vallat, Claire and Rubin, Martin},
  title = {Birth of a comet magnetosphere: A spring of water ions},
  volume = {347},
  number = {6220},
  year = {2015},
  doi = {10.1126/science.aaa0571},
  abstract = {The Rosetta mission shall accompany comet 67P/Churyumov-Gerasimenko from a heliocentric distance of >3.6 astronomical units through perihelion passage at 1.25 astronomical units, spanning low and maximum activity levels. Initially, the solar wind permeates the thin comet atmosphere formed from sublimation, until the size and plasma pressure of the ionized atmosphere define its boundaries: A magnetosphere is born. Using the Rosetta Plasma Consortium ion composition analyzer, we trace the evolution from the first detection of water ions to when the atmosphere begins repelling the solar wind (~3.3 astronomical units), and we report the spatial structure of this early interaction. The near-comet water population comprises accelerated ions (<800 electron volts), produced upstream of Rosetta, and lower energy locally produced ions; we estimate the fluxes of both ion species and energetic neutral atoms.},
  url = {http://www.sciencemag.org/content/347/6220/aaa0571.abstract},
  eprint = {http://www.sciencemag.org/content/347/6220/aaa0571.full.pdf},
  journal = {Science}
}
@article{Lilensten2015,
  title = {Prediction of blue, red and green aurorae at mars },
  journal = {Planetary and Space Science },
  volume = {},
  number = {0},
  pages = { - },
  year = {2015},
  note = {},
  issn = {0032-0633},
  doi = {http://dx.doi.org/10.1016/j.pss.2015.04.015},
  url = {http://www.sciencedirect.com/science/article/pii/S0032063315001300},
  author = {J. Lilensten and D. Bernard and M. Barth\'{e}lemy and G. Gronoff and C. Simon Wedlund and A. Opitz},
  keywords = {Mars},
  keywords = {Aurora },
  abstract = {Abstract The upper atmosphere of Mars is a laboratory for better understanding the planetary atmosphere evolution, and is an example of the interaction of the solar wind with an unmagnetized planet that has only patches of crustal magnetic field. In that context, several space missions were launched to study the Martian environment and its aurorae, notably ESA's Mars Express discovered the first aurora-like structures, and more recently NASA's MAVEN, which is dedicated to understand the atmospheric escape. However, none of the existing missions have spectrometers in the visible spectral range for the observation of the upper atmosphere and the aurorae, but there are \{UV\} spectrometer which can be used to infer visible aurora emission. The \{UV\} aurorae on Mars have a counterpart in the visible spectral range which should be detectable under the right conditions. We discuss what are the most favorable conditions to observe these aurorae discernible with the naked eye. In this article, we simulate the Martian aurora in the visible spectral range both with an experimental setup (the Planeterrella, which we use to measure intensity with respect to the naked eye) and with a numerical ionosphere simulation model (Trans⁎/Aeroplanets). We show that the electron impact on \{CO2\} produces strong emissions at 412 nm and 434 nm, i.e., in the blue part of the visible spectrum which are due to the CO2+(A) Fox-Duffendack-Barker bands. The modeling of the electron transport at Mars shows that these blue emissions as well as the emissions of the 630 nm (red) and 557.7 nm (green) lines of atomic oxygen may be observable several times during a solar cycle during strong solar events. The absence of visible spectrometers dedicated to these observations onboard existing space missions and the location of the different Martian rovers, far from the vertically aligned crustal magnetic field lines of Mars, have prevented so far the observations of such an aurora. In the foreseeable future, two missions may help observing these aurorae: The exo-Mars/Trace Gas Orbiter mission will carry a visible spectrometer which could be used to detect these events in the visible spectral range. \{NOMAD\} (Nadir and Occultation for Mars Discovery) will carry a UV-visible spectrometer in the 200–650 nm range. This work is dedicated to Kristian Birkeland (1867–1917). }
}
@article{2014GeoRL..41.4844G,
  author = {{Gronoff}, G. and {Rahmati}, A. and {Wedlund}, C.~S. and {Mertens}, C.~J. and 
	{Cravens}, T.~E. and {Kallio}, E.},
  title = {{The precipitation of keV energetic oxygen ions at Mars and their effects during the comet Siding Spring approach}},
  journal = {Geophys. Res. Lett.},
  keywords = {Mars, comet, O$^{+}$, pickup},
  year = 2014,
  month = jul,
  volume = 41,
  pages = {4844-4850},
  doi = {10.1002/2014GL060902},
  adsurl = {http://adsabs.harvard.edu/abs/2014GeoRL..41.4844G},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2014ApJ...788..191G,
  author = {{Gronoff}, G. and {Maggiolo}, R. and {Wedlund}, C.~S. and {Mertens}, C.~J. and 
	{Norman}, R.~B. and {Bell}, J. and {Bernard}, D. and {Parkinson}, C.~J. and 
	{Vidal-Madjar}, A.},
  title = {{Theoretical UV Absorption Spectra of Hydrodynamically Escaping O$_{2}$/CO$_{2}$-Rich Exoplanetary Atmospheres}},
  journal = {Astrophys. J.},
  keywords = {molecular data, planets and satellites: atmospheres, planets and satellites: detection, ultraviolet: planetary systems },
  year = 2014,
  month = jun,
  volume = 788,
  eid = {191},
  pages = {191},
  doi = {10.1088/0004-637X/788/2/191},
  adsurl = {http://adsabs.harvard.edu/abs/2014ApJ...788..191G},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2013JGRA..118.3672S,
  author = {{Simon Wedlund}, C. and {Lamy}, H. and {Gustavsson}, B. and 
	{Sergienko}, T. and {Br{\"a}ndstr{\"o}m}, U.},
  title = {{Estimating energy spectra of electron precipitation above auroral arcs from ground-based observations with radar and optics}},
  journal = {J. Geophys. Res.},
  keywords = {aurora, electron precipitation, electron energy, magnetosphere-ionosphere coupling, tomography (optics), inversion techniques},
  year = 2013,
  month = jun,
  volume = 118,
  pages = {3672-3691},
  doi = {10.1002/jgra.50347},
  adsurl = {http://adsabs.harvard.edu/abs/2013JGRA..118.3672S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2013JSWSC...3A..07L,
  author = {{Lilensten}, J. and {Provan}, G. and {Grimald}, S. and {Brekke}, A. and 
	{Fl{\"u}ckiger}, E. and {Vanlommel}, P. and {Wedlund}, C.~S. and 
	{Barth{\'e}l{\'e}my}, M. and {Garnier}, P.},
  title = {{The Planeterrella experiment: from individual initiative to networking}},
  journal = {J. Space Weath. Space Clim.},
  archiveprefix = {arXiv},
  eprint = {1207.1866},
  primaryclass = {physics.ed-ph},
  keywords = {outreach, aurora, experimental},
  year = 2013,
  month = feb,
  volume = 3,
  number = 27,
  eid = {A07},
  pages = {A7},
  doi = {10.1051/swsc/2013029},
  adsurl = {http://adsabs.harvard.edu/abs/2013JSWSC...3A..07L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2013JSWSC...3A..01L,
  author = {{Lilensten}, J. and {Barth{\'e}l{\'e}my}, M. and {Amblard}, P.-O. and 
	{Lamy}, H. and {Wedlund}, C.~S. and {Bommier}, V. and {Moen}, J. and 
	{Rothkaehl}, H. and {Eymard}, J. and {Ribot}, J.},
  title = {{The thermospheric auroral red line polarization: confirmation of detection and first quantitative analysis}},
  journal = {J. Space Weath. Space Clim.},
  keywords = {thermosphere, auroral emissions, polarization},
  year = 2013,
  month = jan,
  volume = 3,
  number = 27,
  eid = {A01},
  pages = {A1},
  doi = {10.1051/swsc/2012023},
  adsurl = {http://adsabs.harvard.edu/abs/2013JSWSC...3A..01L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2013Icar..222..169L,
  author = {{Lilensten}, J. and {Simon Wedlund}, C. and {Barth{\'e}l{\'e}my}, M. and 
	{Thissen}, R. and {Ehrenreich}, D. and {Gronoff}, G. and {Witasse}, O.
	},
  title = {{Dications and thermal ions in planetary atmospheric escape}},
  journal = {Icarus},
  year = 2013,
  month = jan,
  volume = 222,
  pages = {169-187},
  doi = {10.1016/j.icarus.2012.09.034},
  adsurl = {http://adsabs.harvard.edu/abs/2013Icar..222..169L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2012JGRA..117.5312S,
  author = {{Sheel}, V. and {Haider}, S.~A. and {Withers}, P. and {Kozarev}, K. and 
	{Jun}, I. and {Kang}, S. and {Gronoff}, G. and {Simon Wedlund}, C.
	},
  title = {{Numerical simulation of the effects of a solar energetic particle event on the ionosphere of Mars}},
  journal = {J. Geophys. Res.},
  keywords = {Planetary Sciences: Solid Surface Planets: Ionospheres (2459), Planetary Sciences: Solar System Objects: Mars, Radio Science: Ionospheric propagation (0689, 2487, 3285, 4275, 4455)},
  year = 2012,
  month = may,
  volume = 117,
  eid = {A05312},
  pages = {5312},
  doi = {10.1029/2011JA017455},
  adsurl = {http://adsabs.harvard.edu/abs/2012JGRA..117.5312S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2012JGRA..117.5309G,
  author = {{Gronoff}, G. and {Simon Wedlund}, C. and {Mertens}, C.~J. and 
	{Barth{\'e}lemy}, M. and {Lillis}, R.~J. and {Witasse}, O.},
  title = {{Computing uncertainties in ionosphere-airglow models: II. The Martian airglow}},
  journal = {J. Geophys. Res.},
  keywords = {Planetary Sciences: Solid Surface Planets: Atmospheres (0343, 1060), Planetary Sciences: Solid Surface Planets: Aurorae and airglow, Planetary Sciences: Solid Surface Planets: Ionospheres (2459), Planetary Sciences: Solid Surface Planets: Instruments and techniques, Planetary Sciences: Solar System Objects: Mars},
  year = 2012,
  month = may,
  volume = 117,
  eid = {A05309},
  pages = {5309},
  doi = {10.1029/2011JA017308},
  adsurl = {http://adsabs.harvard.edu/abs/2012JGRA..117.5309G},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2012JGRA..117.4306G,
  author = {{Gronoff}, G. and {Simon Wedlund}, C. and {Mertens}, C.~J. and 
	{Lillis}, R.~J.},
  title = {{Computing uncertainties in ionosphere-airglow models: I. Electron {fl}ux and species production uncertainties for Mars}},
  journal = {J. Geophys. Res.},
  keywords = {Ionosphere: Particle acceleration, Ionosphere: Particle precipitation, Planetary Sciences: Fluid Planets: Aurorae, Planetary Sciences: Solar System Objects: Mars, Space Plasma Physics: Ionization processes (2423)},
  year = 2012,
  month = apr,
  volume = 117,
  eid = {A04306},
  pages = {4306},
  doi = {10.1029/2011JA016930},
  adsurl = {http://adsabs.harvard.edu/abs/2012JGRA..117.4306G},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2012Icar..218..308C,
  author = {{Cessateur}, G. and {Lilensten}, J. and {Barth{\'e}l{\'e}my}, M. and 
	{Dudok de Wit}, T. and {Simon Wedlund}, C. and {Gronoff}, G. and 
	{M{\'e}nager}, H. and {Kretzschmar}, M.},
  title = {{Photoabsorption in Ganymede{\rsquo}s atmosphere}},
  journal = {Icarus},
  year = 2012,
  month = mar,
  volume = 218,
  pages = {308-319},
  doi = {10.1016/j.icarus.2011.11.025},
  adsurl = {http://adsabs.harvard.edu/abs/2012Icar..218..308C},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2012AnGeo..30..283M,
  author = {{Maggiolo}, R. and {Echim}, M. and {Wedlund}, C.~S. and {Zhang}, Y. and 
	{Fontaine}, D. and {Lointier}, G. and {Trotignon}, J.-G.},
  title = {{Polar cap arcs from the magnetosphere to the ionosphere: kinetic modelling and observations by Cluster and TIMED}},
  journal = {Ann. Geophys.},
  year = 2012,
  month = feb,
  volume = 30,
  pages = {283-302},
  doi = {10.5194/angeo-30-283-2012},
  adsurl = {http://adsabs.harvard.edu/abs/2012AnGeo..30..283M},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2011ITPS...39.2712G,
  author = {{Gronoff}, G. and {Wedlund}, C.~S.},
  title = {{Auroral Formation and Plasma Interaction Between Magnetized Objects Simulated With the Planeterrella}},
  journal = {IEEE Trans. Plasma Sci.},
  year = 2011,
  month = nov,
  volume = 39,
  pages = {2712-2713},
  doi = {10.1109/TPS.2011.2147804},
  adsurl = {http://adsabs.harvard.edu/abs/2011ITPS...39.2712G},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2011AnGeo..29.1101B,
  author = {{Barth{\'e}l{\'e}my}, M. and {Lilensten}, J. and {Pitout}, F. and 
	{Wedlund}, C.~S. and {Thissen}, R. and {Lorentzen}, D. and {Sigernes}, F. and 
	{Moen}, J. and {Gronoff}, G. and {McCrea}, I. and {Rothkael}, H. and 
	{M{\'e}nager}, H. and {Aruliah}, A.},
  title = {{Polarisation in the auroral red line during coordinated EISCAT Svalbard Radar/optical experiments}},
  journal = {Ann. Geophys.},
  year = 2011,
  month = jun,
  volume = 29,
  pages = {1101-1112},
  doi = {10.5194/angeo-29-1101-2011},
  adsurl = {http://adsabs.harvard.edu/abs/2011AnGeo..29.1101B},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2011AnGeo..29..187S,
  author = {{Simon Wedlund}, C. and {Gronoff}, G. and {Lilensten}, J. and 
	{M{\'e}nager}, H. and {Barth{\'e}lemy}, M.},
  title = {{Comprehensive calculation of the energy per ion pair or W values for five major planetary upper atmospheres}},
  journal = {Ann. Geophys.},
  year = 2011,
  month = jan,
  volume = 29,
  pages = {187-195},
  doi = {10.5194/angeo-29-187-2011},
  adsurl = {http://adsabs.harvard.edu/abs/2011AnGeo..29..187S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2011PCCP...1318264T,
  author = {{Thissen}, R. and {Witasse}, O. and {Dutuit}, O. and {Wedlund}, C.~S. and 
	{Gronoff}, G. and {Lilensten}, J.},
  title = {{Doubly-charged ions in the planetary ionospheres: a review}},
  journal = {Physical Chemistry Chemical Physics (Incorporating Faraday Transactions)},
  year = 2011,
  volume = 13,
  pages = {18264},
  doi = {10.1039/c1cp21957j},
  adsurl = {http://adsabs.harvard.edu/abs/2011PCCP...1318264T},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2009MNRAS.400..369N,
  author = {{Nicholson}, W.~P. and {Gronoff}, G. and {Lilensten}, J. and 
	{Aylward}, A.~D. and {Simon}, C.},
  title = {{A fast computation of the secondary ion production in the ionosphere of Mars}},
  journal = {Month. Not. Roy. Astron. Soc.},
  keywords = {planets and satellites: individual: Mars , Solar system: general},
  year = 2009,
  month = nov,
  volume = 400,
  pages = {369-382},
  doi = {10.1111/j.1365-2966.2009.15463.x},
  adsurl = {http://adsabs.harvard.edu/abs/2009MNRAS.400..369N},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2009P&SS...57.1008S,
  author = {{Simon}, C. and {Witasse}, O. and {Leblanc}, F. and {Gronoff}, G. and 
	{Bertaux}, J.-L.},
  title = {{Dayglow on Mars: Kinetic modelling with SPICAM UV limb data}},
  journal = {Plan. Space Sci.},
  year = 2009,
  month = jul,
  volume = 57,
  pages = {1008-1021},
  doi = {10.1016/j.pss.2008.08.012},
  adsurl = {http://adsabs.harvard.edu/abs/2009P%26SS...57.1008S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2009AcGeo..57..220L,
  author = {{Lilensten}, J. and {Barth{\'e}lemy}, M. and {Simon}, C. and 
	{Jeanjacquot}, P. and {Gronoff}, G.},
  title = {{The Planeterrella, a pedagogic experiment in planetology and plasma physics}},
  journal = {Acta Geophys.},
  keywords = {Aurora, planetary ionospheres, plasma, the Planeterrella experiment},
  year = 2009,
  month = mar,
  volume = 57,
  pages = {220-235},
  doi = {10.2478/s11600-008-0079-x},
  adsurl = {http://adsabs.harvard.edu/abs/2009AcGeo..57..220L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2008A&A...482.1015G,
  author = {{Gronoff}, G. and {Lilensten}, J. and {Simon}, C. and {Barth{\'e}lemy}, M. and 
	{Leblanc}, F. and {Dutuit}, O.},
  title = {{Modelling the Venusian airglow}},
  journal = {\aap},
  keywords = {planets and satellites: individual: Venus, atmospheric effects, Sun: UV radiation, space vehicles: instruments},
  year = 2008,
  month = may,
  volume = 482,
  pages = {1015-1029},
  doi = {10.1051/0004-6361:20077503},
  adsurl = {http://adsabs.harvard.edu/abs/2008A%26A...482.1015G},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2008GeoRL..35.8804L,
  author = {{Lilensten}, J. and {Moen}, J. and {Barth{\'e}lemy}, M. and 
	{Thissen}, R. and {Simon}, C. and {Lorentzen}, D.~A. and {Dutuit}, O. and 
	{Amblard}, P.~O. and {Sigernes}, F.},
  title = {{Polarization in aurorae: A new dimension for space environments studies}},
  journal = {Geophys. Res. Lett.},
  keywords = {Ionosphere: Ionosphere/atmosphere interactions (0335), Ionosphere: Auroral ionosphere (2704), Atmospheric Processes: Thermospheric dynamics (0358), Planetary Sciences: Fluid Planets: Ionospheres (2459), Space Weather: General or miscellaneous},
  year = 2008,
  month = apr,
  volume = 35,
  eid = {L08804},
  pages = {8804},
  doi = {10.1029/2007GL033006},
  adsurl = {http://adsabs.harvard.edu/abs/2008GeoRL..35.8804L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2007A&A...465..641G,
  author = {{Gronoff}, G. and {Lilensten}, J. and {Simon}, C. and {Witasse}, O. and 
	{Thissen}, R. and {Dutuit}, O. and {Alcaraz}, C.},
  title = {{Modelling dications in the diurnal ionosphere of Venus}},
  journal = {\aap},
  keywords = {planets and satellites: individual: Venus, atmospheric effects, Sun: UV radiation, space vehicles: instruments},
  year = 2007,
  month = apr,
  volume = 465,
  pages = {641-645},
  doi = {10.1051/0004-6361:20065991},
  adsurl = {http://adsabs.harvard.edu/abs/2007A%26A...465..641G},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2007AnGeo..25..661S,
  author = {{Simon}, C. and {Lilensten}, J. and {Moen}, J. and {Holmes}, J.~M. and 
	{Ogawa}, Y. and {Oksavik}, K. and {Denig}, W.~F.},
  title = {{TRANS4: a new coupled electron/proton transport code - comparison to observations above Svalbard using ESR, DMSP and optical measurements}},
  journal = {Ann. Geophys.},
  year = 2007,
  month = mar,
  volume = 25,
  pages = {661-673},
  doi = {10.5194/angeo-25-661-2007},
  adsurl = {http://adsabs.harvard.edu/abs/2007AnGeo..25..661S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2006SpWea...411002L,
  author = {{Lilensten}, J. and {Simon}, C. and {Barth{\'e}L{\'e}My}, M. and 
	{Moen}, J. and {Thissen}, R. and {Lorentzen}, D.~A.},
  title = {{Considering the polarization of the oxygen thermospheric red line for space weather studies}},
  journal = {Space Weather},
  keywords = {Space Weather: Forecasting (2722), Space Weather: Satellite drag (1241), Space Weather: Solar effects, space weather, thermosphere, ionosphere, polarization, nightglow, experiment},
  year = 2006,
  month = nov,
  volume = 4,
  eid = {S11002},
  pages = {11002},
  doi = {10.1029/2006SW000228},
  adsurl = {http://adsabs.harvard.edu/abs/2006SpWea...411002L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2005Icar..174..285L,
  author = {{Lilensten}, J. and {Simon}, C. and {Witasse}, O. and {Dutuit}, O. and 
	{Thissen}, R. and {Alcaraz}, C.},
  title = {{A fast computation of the diurnal secondary ion production in the ionosphere of Titan}},
  journal = {Icarus},
  year = 2005,
  month = mar,
  volume = 174,
  pages = {285-288},
  doi = {10.1016/j.icarus.2004.12.002},
  adsurl = {http://adsabs.harvard.edu/abs/2005Icar..174..285L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2005AnGeo..23..781S,
  author = {{Simon}, C. and {Lilensten}, J. and {Dutuit}, O. and {Thissen}, R. and 
	{Witasse}, O. and {Alcaraz}, C. and {Soldi-Lose}, H.},
  title = {{Prediction and modelling of doubly-charged ions in the Earth's upper atmosphere}},
  journal = {Ann. Geophys.},
  year = 2005,
  month = mar,
  volume = 23,
  pages = {781-797},
  doi = {10.5194/angeo-23-781-2005},
  adsurl = {http://adsabs.harvard.edu/abs/2005AnGeo..23..781S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{2005GeoRL..32.3203L,
  author = {{Lilensten}, J. and {Witasse}, O. and {Simon}, C. and {Soldi-Lose}, H. and 
	{Dutuit}, O. and {Thissen}, R. and {Alcaraz}, C.},
  title = {{Prediction of a N$_{2}$$^{++}$ layer in the upper atmosphere of Titan}},
  journal = {Geophys. Res. Lett.},
  keywords = {Atmospheric Composition and Structure: Airglow and aurora, Atmospheric Composition and Structure: Ion chemistry of the atmosphere (2419, 2427), Atmospheric Composition and Structure: Planetary atmospheres (5210, 5405, 5704), Ionosphere: Planetary ionospheres (5435, 5729, 6026), Planetary Sciences: Solar System Objects: Titan},
  year = 2005,
  month = feb,
  volume = 32,
  eid = {L03203},
  pages = {3203},
  doi = {10.1029/2004GL021432},
  adsurl = {http://adsabs.harvard.edu/abs/2005GeoRL..32.3203L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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