[1] Chen Hongbin. An overview of the space-based observations for upper atmospheric research[J]. Advances in Earth Science, 2009, 24(3): 229-241. (in Chinese)
[2] Spitzer Jr L. The terrestrial atmosphere above 300 km[C]//The Atmospheres of the Earth and Planets, 1949, 1: 211.
[3] Lopez-Puertas M, Rodrigo R, Molina A, et al. A non-LTE radiative transfer model for infrared bands in the middle atmosphere. I. Theoretical basis and application to CO2 15 μm bands [J]. Journal of Atmospheric and Terrestrial Physics, 1986, 48(8): 729-748.
[4] López-Puertas M, Rodrigo R, López-Moreno J J, et al. A non-LTE radiative transfer model for infrared bands in the middle atmosphere. II. CO2(2.7 and 4.3 μm) and water vapour(6.3 μm) bands and N2(1) and O2(1) vibrational levels [J]. Journal of Atmospheric and Terrestrial Physics, 1986, 48(8): 749-764.
[5] Sundberg R L, Duff J W, Gruninger J H, et al. SHARC, a Model for Calculating Atmospheric Infrared Radiation Under Non-Equilibrium Conditions[M]. New York: American Geophysical Union, 1994.
[6] Remsberg E E, Marshall B T, Garcia-Comas M, et al. Assessment of the quality of the Version 1.07 temperature versus pressure profiles of the middle atmosphere from TIMED/SABER[J]. Journal of Geophysical Research: Atmospheres, 2008, 113: D17101.
[7] Funke B, López-Puertas M, García-Comas M, et al. GRANADA: A generic radiative transfer and non-LTE population algorithm[J]. Journal of Quantitative Spectroscopy and Radiative Transfer, 2012, 113(14): 1771-1817.
[8] López-Puertas M, Taylor F W. Non-LTE Radiative Transfer in the Atmosphere [M]. Londom: World Scientific, 2001.
[9] Robertson D C, Acharya P K, Adler-Golden S M, et al. Investigations into atmospheric radiative processes in the 50-300 km regime[R]. Burlington MA: Spectral Sciences INC, 1991.
[10] Kumer J B, James T C. CO2(001) and N2 vibrational temperatures in the 50≤z≤130 km altitude range[J]. Journal of Geophysical Research, 1974, 79(4): 638-648.
[11] Kumer J B. Atmospheric CO2 and N2 vibrational temperatures at 40 to 140 km altitude[J]. Journal of Geophysical Research, 1977, 82(16): 2195-2202.
[12] Wintersteiner P P, Picard R H, Sharma R D, et al. Line-by-line radiative excitation model for the non-equilibrium atmosphere: Application to CO2 15 μm emission [J]. Journal of Geophysical Research: Atmospheres, 1992, 97(D16): 18083-18117.
[13] López-Puertas M, Funke B, Gil-López S, et al. Atmospheric non-local thermodynamic equilibrium emissions as observed by the Michelson Interferometer for Passive Atmospheric Sounding (MIPAS)[J]. Comptes Rendus Physique, 2005, 6(8): 848-863.
[14] López-Puertas M, García-Comas M, Funke B, et al. Evidence for an OH (υ) excitation mechanism of CO2 4.3 μm nighttime emission from SABER/TIMED measurements[J]. Journal of Geophysical Research: Atmospheres, 2003, 109: 10.1029/2003JD004383.
[15] Mertens C J, Mlynczak M G, López-Puertas M, et al. Retrieval of mesospheric and lower thermospheric kinetic temperature from measurements of CO2 15 μm Earth Limb Emission under non-LTE conditions[J]. Geophysical Research Letters, 2001, 28(7): 1391-1394.
[16] Picone J M, Hedin A E, Drob D P, et al. NRLMSISE-00 empirical model of the atmosphere: Statistical comparisons and scientific issues[J]. Journal of Geophysical Research: Space Physics, 2002, 107(A12): SIA 15-1-SIA 15-16.
[17] Rothman L S, Gordon I E, Barbe A, et al. The HITRAN2008 molecular spectroscopic database[J]. Journal of Quantitative Spectroscopy and Radiative Transfer, 2009, 110(9): 533-572.
[18] Kutepov A A, Feofilov A G, Marshall B T, et al. SABER temperature observations in the summer polar mesosphere and lower thermosphere: Importance of accounting for the CO2 v2 quanta V-V exchange[J]. Geophysical Research Letters, 2006, 33(21): 10.1029/2006GL026591.