Metal fluorescence lidar (light detection and ranging) and the middle atmosphere, Contemporary Physics, vol.51, issue.1, pp.35-49, 2003. ,
DOI : 10.1029/94JD03109
Physics of the Aurora and Airglow, 1961. ,
Satellite measurements of the global mesospheric sodium layer, Atmos. Chem. Phys, vol.75194, pp.4107-411510, 2007. ,
URL : https://hal.archives-ouvertes.fr/hal-00296306
Mesopause temperatures derived from probing the hyperfine structure of the D2 resonance line of sodium by lidar, Journal of Atmospheric and Terrestrial Physics, vol.47, issue.5, pp.499-512, 2010. ,
DOI : 10.1016/0021-9169(85)90116-3
Mesospheric sodium global, Global measurement of the mesospheric sodium layer by the star occultation instrument GOMOS, p.10, 1029. ,
URL : https://hal.archives-ouvertes.fr/hal-00461846
Seasonal variations of the Na and Fe layers at the South Pole and their implications for the chemistry and general circulation of the polar mesosphere, Journal of Geophysical Research, vol.330, issue.2, p.10302, 2005. ,
DOI : 10.1029/2004JD005670
Retrieval of global mesospheric sodium densities from the Odin satellite, Geophysical Research Letters, vol.67, issue.4, pp.481310-1029, 2007. ,
DOI : 10.1029/2006GL028687
Laser sounding of atmospheric sodium interpretation in terms of global atmospheric parameters, Planetary and Space Science, vol.25, issue.12, pp.1093-1109, 1977. ,
DOI : 10.1016/0032-0633(77)90085-X
Atmospheric Chemistry of Meteoric Metals, Chemical Reviews, vol.103, issue.12, pp.4963-4984, 2003. ,
DOI : 10.1021/cr0205309
Removal of Meteoric Iron on Polar Mesospheric Clouds, Science, vol.304, issue.5669, pp.426-428, 2004. ,
DOI : 10.1126/science.1093236
Eight-year climatology of nocturnal temperature and sodium density in the mesopause region (80 to 105 km) over Fort Collins, Co (41??N, 105??W), 80 to 105 km) over Fort Collins, CO (41 ? N, 105 ? W), pp.3289-3292, 2000. ,
DOI : 10.1029/2000GL003825
Sodium D Line Data, Los Alamos National Laboratory Technical Report LA-UR-03-8639, revision 1.6, available at: http://steck, 2003. ,