火星沙尘气溶胶对激光传输特性的影响
[1] STEINBACHER R H, KLIORE A, LORELL J, et al. Mariner 9 science experiments: preliminary results[J]. Science, 1972, 175(4019): 293.
[2] CANTOR B A, JAMES P B, CAPLINGER M, et al. Martian dust storms: 1999 Mars orbiter camera observations[J]. Journal of Geophysical Research Planets, 2001, 106(E10): 23653-23687.
[3] CLANCY R T, LEE S W, GLADSTONE G R, et al. A new model for Mars atmospheric dust based upon analysis of ultraviolet through infrared observations from Mariner 9, Viking, and Phobos[J]. Journal of Geophysical Research Planets, 1995, 100(E3): 5251-5263.
[4] TOON O B, POLLACK J B, SAGAN C. Physical properties of the particles composing the Martian dust storm of 1971-1972[J]. Icarus, 1977, 30(4): 663-696.
[5] TOMASKO M G, DOOSE L R, LEMMON M, et al. Properties of dust in the Martian atmosphere from the Imager on Mars Pathfinder[J]. Journal of Geophysical Research Planets, 1999, 104(E4): 8987-9007.
[6] POLLACK J B, OCKERT‐BELL M E, SHEPARD M K. Viking Lander image analysis of Martian atmospheric dust[J]. Journal of Geophysical Research Planets,1995, 100(E3): 5235-5250.
[7] ELTETO A, TOON O B. Retrieval algorithm for atmospheric dust properties from Mars Global Surveyor Thermal Emission Spectrometer data during global dust storm 2001A[J]. Icarus, 2010, 210(2): 566-588.
[8] WOLFF M J, CLANCY R T. Constraints on the size of Martian aerosols from Thermal Emission Spectrometer Observations[J]. Journal of Geophysical Research Planets, 2003, 108(E9): 5097.
[9] WOLFF M J, SMITH M D, CLANCY R T, et al. Constraints on dust aerosols from the Mars Exploration Rovers using MGS overflights and Mini‐TES[J]. Journal of Geophysical Research Planets, 2006, 111(E12): 41-51.
[10] FEDOROVA A A, MONTMESSIN F, RODIN A V, et al. Evidence for a bimodal size distribution for the suspended aerosol particles on Mars[J]. Icarus, 2014, 231(231): 239-260.
[11] HANSEN, J. E,TRAVIS L. D.Light scattering in planetary atmospheres[J].Space Science Reviews,1974,16: 527-560
[12] MONTMESSIN F, RANNOU P, CABANE M. New insights into Martian dust distribution and water‐ice cloud microphysics[J]. Journal of Geophysical Research Planets, 2002, 107(E6): 4-1-4-14.
[13] MISHCHENKO M I, DLUGACH J M, YANOVITSKIJ E G, et al. Bidirectional reflectance of flat, optically thick particulate layers: an efficient radiative transfer solution and applications to snow and soil surfaces[J]. Journal of Quantitative Spectroscopy & Radiative Transfer, 1999, 63(2-6): 409-432.
[14] OCKERTBELL M E, RD B J, POLLACK J B, et al. Absorption and scattering properties of the Martian dust in the solar wavelengths.[J]. Journal of Geophysical Research Atmospheres, 1997, 102(E4): 9039-9050.
[15] 吴振森,由金光,杨瑞科.激光在沙尘暴中的衰减特性研究[J]. 中国激光, 2004, 31(9): 1075-1080.
杨玉峰, 秦建华, 王昭雷. 火星沙尘气溶胶对激光传输特性的影响[J]. 光子学报, 2018, 47(3): 0329001. YANG Yu-feng, QIN Jian-hua, WANG Zhao-lei. Influence of Martian Dust Aerosol on Laser Transmission Characteristics[J]. ACTA PHOTONICA SINICA, 2018, 47(3): 0329001.