Simulation of Limb Measurements for Mesospheric Hydroxyl Radical Based on SHS Detector
ZHANG Hong-hai1, 2, 3, GAO Yi-bo1, 2, 3, LI Chao1, 2, 3, MA Jin-ji1, 2, 3*, FANG Xue-jing4, XIONG Wei4
1. College of Territorial Resources and Tourism, Anhui Normal University, Wuhu 241000, China
2. Engineering Technology Research Center of Resources Environment and GIS, Anhui Province, Wuhu 241000, China
3. Anhui Key Laboratory of Natural Disaster Process and Prevention, Anhui Normal University, Wuhu 241003, China
4. Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, China
Abstract:OH radicals in atmosphere, an important mediator of the photochemical reactions between various atmospheric compositions, play a key role in the formation and transformation of other atmospheric components. Based on the OH concentration spatiotemporal database constructed by MLS global observation results of OH, and the OH emission spectra database from Lifbase, SCIATRAN was modified according to the radiation transmission theory. The simulated image of spatial heterodyne spectrum (SHS) detector was obtained in the state of limb scanning and the contribution of atmospheric OH radical fluorescence emission in observing energy was extracted. Based on the radiation transmission theory, the quantitative influence of the uncertainty of each parameter in the simulation process was analyzed quantitatively. The results can not only provide scientific theoretical supports for the construction of detector for mesospheric OH radical, but also provide the basis for the design of relevant parameters of detector.
Key words:Atmospheric light;Radiation transmission;OH radicals;Simulations of limb observation
[1] Stevens M, Englert C, Grossmann K, et al. MAHRSI and CRISTA Observations of the Arctic Summer Mesosphere. AIAA Space 2001 Conference and Exposition,2001.
[2] Englert C R, Stevens M H, Siskind D E, et al. Journal of Geophysical Research Atmospheres, 2010, 115(D20): 898.
[3] Shuhui W, King-Fai L, Pongetti T J, et al. Proceedings of the National Academy of Sciences of the United States of America, 2013, 110(6): 2023.
[4] NSO/Kitt Peak FTS Data Used Here were Produced by NSF/NOAO.
[5] PENG Zhi-min, DING Yan-jun, YANG Qian-suo, et al(彭志敏, 丁艳军, 杨乾锁, 等). Acta Phys. Sin.(物理学报), 2011, 4(5): 250.
[6] Luque J, Crosley D R, Luque J, et al. LIFbase: Database and Spectral Simulation,1996.
[7] Piasecki B, Fletcher K. Journal of Physics D Applied Physics, 2010, 43(12): 364.
[8] LU Xiao-hui, SUN Ming, HAO Xia-tong, et al(鲁晓辉, 孙 明, 郝夏桐, 等). Journal of Shanghai Maritime University(上海海事大学学报), 2014,(4): 89.
[9] Hortal Mariano, Simmons A J. Monthly Weather Review,1991,119(4): 1057.
[10] ZHANG Hong-hai, LI Chao, GAO Yi-bo, et al(张洪海, 李 超, 高一博, 等). Journal of Atmospheric and Environmental Optics(大气与环境光学学报), 2017. 4.
[11] LUO Hai-yan, LI Shuang, SHI Hai-liang, et al(罗海燕, 李 双, 施海亮, 等). Infrared & Laser Engineering(红外与激光工程), 2016, 45(8): 0818005.
[12] Perkins C P, Kerekes J P, Cartley M G. Proc. SPIE, 2013, 8870(5755): 88700k-14.
[13] Degenstein D A, Bourassa A E, Roth C Z, et al. Atmospheric Chemistry & Physics, 2008, 8(3): 6521.
[14] Stevens M H, Conway R R. Calculated OH A. Journal of Geophysical Research Atmospheres, 1999, 1041(D13): 16369.
[15] GAO Hong, XU Ji-yao, CHEN Guang-ming, et al(高 红, 徐寄遥, 陈光明, 等). Chinese Journal of Space Science(空间科学学报), 2009, 29(3): 304.