Open Access
J. Space Weather Space Clim.
Volume 5, 2015
Article Number A26
Number of page(s) 15
Published online 12 August 2015
  • Aso, T., M. Ejiri, A. Urashima, H. Miyaoka, Å. Steen, U. Brändström, and B. Gustavsson. First results of auroral tomography from ALIS-Japan multi-station observations in March, 1995. Earth, Planets, and Space, 50, 81–86, 1998. [CrossRef] [Google Scholar]
  • Banks, P.M., and G. Kockarts. Aeronomy, Springer, 1973. [Google Scholar]
  • Barthélemy, M., J. Lilensten, F. Pitout, C. Simon Wedlund, R. Thissen, et al. Polarisation in the auroral red line during coordinated EISCAT Svalbard Radar/optical experiments. Ann. Geophys., 29, 1101–1112, 2011. [Google Scholar]
  • Bilitza, D., S.A. Brown, M.Y. Wang, J.R. Souza, and P.A. Roddy. Measurements and IRI model predictions during the recent solar minimum. J. Atmos. Sol. Terr. Phys., 86, 99–106, 2012. [Google Scholar]
  • Bommier, V., S. Sahal-Brechot, J. Dubau, and M. Cornille. The theoretical impact polarization of the O I 6300 A red line of Earth Aurorae. Ann. Geophys., 29, 71–79, 2011. [Google Scholar]
  • Brändström, B.U.E PhD thesis, The auroral large imaging system: design, operation and scientific results, Institutet fr rymdfysik (IRF) Sci. Rep., 279, IRF, Kiruna, Sweden, 2003. [Google Scholar]
  • Brink, D.M., and G.R. Satchler. Angular Momentum, 3rd edn., Clarendon Press, Oxford, 1994. [Google Scholar]
  • Bruinsma, S.L., N. Sanchez-Ortiz, E. Olmedo, and N. Guijarro. Evaluation of the DTM-2009 thermosphere model for benchmarking purposes. J. Space Weather Space Clim., 2, A04, 2012, DOI: 10.1051/swsc/2012005. [CrossRef] [EDP Sciences] [Google Scholar]
  • Bucholtz, A. Rayleigh-scattering calculations for the terrestrial atmosphere. Appl. Opt., 34, 2765, 1959. [Google Scholar]
  • Charvin, P. Étude de la polarisation des raies interdites de la couronne solaire. Application au cas de la raie verte λ 5303. Annales d’Astrophysique, 28, 877, 1965. [Google Scholar]
  • Clarke, D. Stellar Polarimetry, Wiley, ISBN: 978-3-527-40895-5, 2010. [Google Scholar]
  • Culot, F., C. Lathuillère, and J. Lilensten. Influence of geomagnetic activity on the O I 630.0 and 557.7 nm dayglow. J. Geophys. Res. [Space Phys.], 110, 1304–13013, 2005. [CrossRef] [Google Scholar]
  • Goldstein, D. Polarized light, Marcel Dekker, New York, NY, 2003. [Google Scholar]
  • Gustavsson, B. Tomographic inversion for ALIS noise and resolution. J. Geophys. Res., 103, 26621–26632, 1998. [CrossRef] [Google Scholar]
  • Hardy, D.A., M.S. Gussenhoven, and E. Holeman. A statistical model of auroral electron precipitation. J. Geophys. Res., 90, 4229–4248, 1985. [Google Scholar]
  • Landi Degl’Innocenti, E. Polarization in spectral lines. III – Resonance polarization in the non-magnetic, collisionless regime. Sol. Phys., 91, 1–26, 1984. [Google Scholar]
  • Landi Degl’Innocenti, E., and M. Landolfi. Polarization in spectral lines, vol. 307 of Astrophysics and Space Science Library, Kluwer Academic Publishers, 2004. [Google Scholar]
  • Lehtinen, M.S., and A. Huuskonen. General incoherent scatter analysis and GUISDAP. J. Atmos. Terr. Phys., 58, 435–452, 1996. [CrossRef] [Google Scholar]
  • Lilensten, J., and L.R. Cander. Calibration of the TEC derived from GPS measurements and from ionospheric models using the EISCAT radar. J. Atmos. Sol. Terr. Phys., 65, 833–842, 2003. [Google Scholar]
  • Lilensten, J., J. Moen, M. Barthélemy, R. Thissen, C. Simon, D.A. Lorentzen, O. Dutuit, P.O. Amblard, and F. Sigernes. Polarization in aurorae: a new dimension for space environments studies. Geophys. Res. Lett., 35, 8804, 2008. [Google Scholar]
  • Lilensten, J., M. Barthélémy, P.O. Amblard, H. Lamy, C.S. Wedlund, et al. The thermospheric auroral red line polarization: confirmation of detection and first quantitative analysis. J. Space Weather Space Clim., 3, A01, 2013a, DOI: 10.1051/swsc/2012023. [CrossRef] [EDP Sciences] [Google Scholar]
  • Lilensten, J., C. Simon Wedlund, M. Barthélémy, R. Thissen, D. Ehrenreich, G. Gronoff, and O. Witasse. Dications and thermal ions in planetary atmospheric escape. Icarus, 222, 169–187, 2013b. [Google Scholar]
  • Lummerzheim, D., and J. Lilensten. Electron transport and energy degradation in the ionosphere: evaluation of the numerical solution, comparison with laboratory experiments and auroral observations. Ann. Geophys., 12, 1039–1051, 1994. [CrossRef] [Google Scholar]
  • Lummerzheim, D., M.H. Rees, and H.R. Anderson. Angular dependent transport of auroral electrons in the upper atmosphere. Planet. Space Sci., 37, 109–129, 1989. [Google Scholar]
  • Lummerzheim, D., M. Galand, J. Semeter, M.J. Mendillo, M.H. Rees, and F.J. Rich. Emission of O I(630 nm) in proton aurora. J. Geophys. Res., 106, 141–148, 2001. [CrossRef] [Google Scholar]
  • Martinez Herrero, R., P.M. Mejias, and G. Piquero. Characterization of partially polarized light field. Springer Series on Optical Sciences, 147, 2009, DOI: 10.1007/978-3-642-01327-0. [CrossRef] [Google Scholar]
  • Moore, C.E., and J.W. Gallagher. Tables of spectra of hydrogen, carbon, nitrogen, and oxygen atoms and ions, CRC Press, Boca Raton, FL, 1993. [Google Scholar]
  • Opal, C., W. Peterson, and E. Beaty. Measurements of secondary-electron spectra produced by electron impact ionization of a number of simple gases. J. Chem. Phys., 55, 4100, 1971. [Google Scholar]
  • Picone, J.M., A.E. Hedin, D.P. Drob, and A.C. Aikin. NRLMSISE-00 empirical model of the atmosphere: statistical comparisons and scientific issues. J. Geophys. Res. [Space Phys.], 107, 1468, 2002. [Google Scholar]
  • Porter, H.S., F. Varosi, and H.G. Mayr. Iterative solution of the multistream electron transport equation. I – Comparison with laboratory beam injection experiments. J. Geophys. Res., 92, 5933–5959, 1987. [NASA ADS] [CrossRef] [Google Scholar]
  • Press, W.H., S.A. Teukolsky, W.T. Vetterling, and B.P. Flannery. Numerical recipes in FORTRAN. The art of scientific computing, 2nd edn., University Press, Cambridge, 1992. [Google Scholar]
  • Rees, M.H. Physics and chemistry of the upper atmosphere, University Press, Cambridge, ISBN: 0521368480, 1989. [CrossRef] [Google Scholar]
  • Roble, R.G., E.C. Ridley, and R.E. Dickinson. On the global mean structure of the thermosphere. J. Geophys. Res., 92, 8745–8758, 1987. [NASA ADS] [CrossRef] [Google Scholar]
  • Safargaleev, V.V., T.I. Sergienko, A.E. Kozlovsky, I. Sandahl, U. Brändström, and D.N. Shibaeva. Electric field enhancement in an auroral arc according to the simultaneous radar (EISCAT) and optical (ALIS) observations. Geomag. Aeron., 49, 353–367, 2009. [CrossRef] [Google Scholar]
  • Sahal-Bréchot, S. Role of collisions in the polarization degree of the forbidden emission lines of the Solar Corona. II – Depolarization by electron impact and calculation of the polarization degree of the Green line of Fe XIV. Astron. Astrophys., 36, 355–363, 1974. [Google Scholar]
  • Simon, C., J. Lilensten, J. Moen, J. Holmes, Y. Ogawa, K. Oksavik, and W. Denig. TRANS4: a new coupled electron/proton transport code comparison to observations above Svalbard using ESR, DMSP and optical measurements. Ann. Geophys., 25, 661–673, 2007. [Google Scholar]
  • Solomon, S.C., and V.J. Abreu. The 630 nm dayglow. J. Geophys. Res., 94, 6817–6824, 1989. [CrossRef] [Google Scholar]
  • Stenflo, J. Solar Magnetic Fields: Polarized Radiation Diagnostics, vol. 189, Kluwer Academic Pub.; Astrophysics and Space Science Library (ASSL), 1994. [CrossRef] [Google Scholar]
  • Swartz, W.E., and J.S. Nisbet. Revised calculations of the f region ambient electron heating by photoelectrons. J. Geophys. Res., 77, 6259–6277, 1972. [Google Scholar]
  • Vallance Jones, A. Historical review of great auroras. Can. J. Phys., 70, 479–487, 1992. [Google Scholar]
  • Wiscombe, W., and G. Gums. The backscattered fraction in two-stream approximations. Genesis, 2, 11, 1998. [Google Scholar]
  • Witasse, O., J. Lilensten, C. Lathuillere, and B. Pibaret. Meridional thermospheric neutral wind at high latitude over a full solar cycle. Ann. Geophys., 16, 1400–1409, 1998. [CrossRef] [Google Scholar]
  • Witasse, O., J. Lilensten, C. Lathuillère, and P.-L. Blelly. Modeling the OI 630.0 and 557.7 nm thermospheric dayglow during EISCAT-WINDII coordinated measurements. J. Geophys. Res., 104, 24639–24656, 1999. [NASA ADS] [CrossRef] [Google Scholar]

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