火星O_2(a~1Δ_g)气辉高光谱分辨辐射传输特性研究
Hyperspectral-resolved radiative transmission theory of O_2(a~1Δ_g)dayglow on Mars
查看参考文献41篇
|
文摘
|
1.27μm波段的氧分子近红外气辉是火星大气最重要的气辉辐射之一,该气辉高光谱分辨辐射传输模型的建立对于研制火星探测载荷,反演火星大气的风场温度场与臭氧浓度,以及研究火星空间物理,有重要的科学价值与工程意义.在研究火星大气O_2(a~1Δ_g)气辉光化学反应模型的基础上,提出了O_2(a~1Δ_g)气辉体辐射率的计算方法,并建立了火星大气气辉辐射传输理论;通过与用于研究火星大气特征的光谱学探测仪(Spectroscopy Spectrograph for the Investigation of Characteristics of the Atmosphere of Mars,SPICAM)的实测数据进行对比,验证了所建立的火星O_2(a~1Δ_g)气辉高光谱分辨辐射传输模型的准确性;针对火星与地球大气的O_2(a~1Δ_g)气辉,在体辐射率、自吸收效应,以及临边辐射光谱特性三个方面进行了系统深入的比较,对比结果表明,火星大气由于密度低、氧气丰度小,其自吸收效应可以忽略不计,但其O_2(a~1Δ_g)气辉辐射强度与地球大气相当,可以用于火星大气的风场温度场与臭氧浓度的探测与反演. |
|
其他语种文摘
|
The near-infrared O_2 dayglow in the 1.27μm band is one of the most important dayglow emission in the Martian atmosphere.The establishment of this hyperspectral-resolved radiative transmission model has important scientific value and engineering significance for the development of Mars detection load,the inversion of Mars atmospheric wind field temperature field and ozone concentration,and the study of Mars space physics.Based on the chemical reaction model of Martian atmospheric O_2(a~1Δ_g)dayglow,the calculation method of the O_2(a~1Δ_g)dayglow radiance is proposed and the transmission theory of Martian atmospheric dayglow radiation is established in this paper.The accuracy of the established Mars O_2(a~1Δ_g)dayglow hyperspectral radiative transfer model was verified by comparing with the measured data of the Spectroscopy Spectrograph for the Investigation of Characteristics of the Atmosphere of Mars(SPICAM).The O_2(a~1Δ_g)dayglow of Mars and the Earth's atmosphere are systematically and deeply compared in three aspects:volume emissivity, self-absorption effect and limb radiation spectral characteristics.The comparison results show that the self-absorption effect of Martian atmosphere is negligible due to its low density and low oxygen abundance,but its O_2(a~1Δ_g)dayglow radiation intensity is comparable to that of the Earth's atmosphere,so it can be used to detect and retrieve the wind field,temperature field and ozone concentration of Martian atmosphere. |
|
来源
|
地球物理学报
,2023,66(5):1864-1875 【核心库】
|
|
DOI
|
10.6038/cjg2022Q0592
|
|
关键词
|
临近空间
;
O_2(a~1Δ_g)←O_2(X~3Σ_g~-)波段
;
气辉
;
体辐射率
;
临边辐射强度
|
|
地址
|
1.
烟台大学物理与电子信息学院, 山东, 烟台, 264005
2.
中国科学院国家空间科学中心, 北京, 100190
3.
中国科学院精密测量科学与技术创新研究院, 武汉, 430071
4.
中国科学院西安光学精密机械研究所, 西安, 710119
|
|
语种
|
中文 |
|
文献类型
|
研究性论文 |
|
ISSN
|
0001-5733 |
|
学科
|
大气科学(气象学) |
|
基金
|
国家自然科学基金项目
;
山东省自然科学基金
;
山东省高等学校"青创科技支持计划"
|
|
文献收藏号
|
CSCD:7462087
|
参考文献 共
41
共3页
|
|
1.
Altieri F. Gravity waves mapped by the OMEGA/MEX instrument through O_2 dayglow at 1.27 μm:data analysis and atmospheric modeling.
Journal of Geophysical Research:Planets,2012,117(E11):E00J08
|
被引
1
次
|
|
|
|
|
2.
Clancy R T. Minimal aerosol loading and global increases in atmospheric ozone during the 1996-1997martian northern spring season.
Icarus,1999,138(1):49-63
|
被引
1
次
|
|
|
|
|
3.
Clancy R T. Extensive MRO CRISM observations of 1.27μm O_2 airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations.
Journal of Geophysical Research:Planets,2012,117(E11):E00J10
|
被引
1
次
|
|
|
|
|
4.
Clancy R T. Vertical profiles of Mars 1.27μm O_2 dayglow from MRO CRISM limb spectra: seasonal/global behaviors,comparisons to LMDGCM simulations,and a global definition for Mars water vapor profiles.
Icarus,2017,293:132-156
|
被引
1
次
|
|
|
|
|
5.
de Vera J P. Limits of life and the habitability of mars:the ESA space experiment BIOMEX on the ISS.
Astrobiology,2019,19(2):145-157
|
被引
3
次
|
|
|
|
|
6.
Espenak F. Ground-based infrared measurements of the global distribution of ozone in the atmosphere of Mars.
Icarus,1991,92(2):252-262
|
被引
1
次
|
|
|
|
|
7.
Fairen A G. Astrobiology through the ages of Mars:the study of terrestrial analogues to understand the habitability of Mars.
Astrobiology,2010,10(8):821-843
|
被引
4
次
|
|
|
|
|
8.
Fedorova A. Mars water vapor abundance from SPICAM IR spectrometer:seasonal and geographic distributions.
Journal of Geophysical Research:Planets,2006,111(E9):E09S08
|
被引
3
次
|
|
|
|
|
9.
Fedorova A. Observation of O_2 1.27μm dayglow by SPICAM IR:seasonal distribution for the first Martian year of Mars Express.
Journal of Geophysical Research:Planets,2006,111(E9):E09S07
|
被引
1
次
|
|
|
|
|
10.
Gagne M E. Modeled O_2 airglow distributions in the Martian atmosphere.
Journal of Geophysical Research:Planets,2012,117(E6):E06005
|
被引
1
次
|
|
|
|
|
11.
Gerard J C. Detection of green line emission in the dayside atmosphere of Mars from NOMADTGO observations.
Nature Astronomy,2020,4(11):1049-1052
|
被引
4
次
|
|
|
|
|
12.
Gerard J C. First observation of the oxygen 630nm emission in the Martian Dayglow.
Geophysical Research Letters,2021,48(8):e2020GL092334
|
被引
1
次
|
|
|
|
|
13.
Guslyakova S. O_2(a1Δg) dayglow limb observations on Mars by SPICAM IR on Mars-Express and connection to water vapor distribution.
Icarus,2014,239:131-140
|
被引
1
次
|
|
|
|
|
14.
Harris R D. Where does the O(1 D)energy go?.
Journal of Geophysical Research:Space Physics,1983,88(A6):4918-4928
|
被引
1
次
|
|
|
|
|
15.
He W W. The radiative transfer characteristics of the O_2 infrared atmospheric band in limbviewing geometry.
Remote Sensing,2019,11(22):2702
|
被引
2
次
|
|
|
|
|
16.
Krasnopolsky V A. Photochemical mapping of Mars.
Journal of Geophysical Research:Planets,1997,102(E6):13313-13320
|
被引
1
次
|
|
|
|
|
17.
Krasnopolsky V A. Mapping of Mars O_2 1.27μm dayglow at four seasonal points.
Icarus,2003,165(2):315-325
|
被引
1
次
|
|
|
|
|
18.
Krasnopolsky V A. Seasonal variations of photochemical tracers at low and middle latitudes on Mars:observations and models.
Icarus,2009,201(2):564-569
|
被引
2
次
|
|
|
|
|
19.
Krasnopolsky V A. Night and day airglow of oxygen at 1.27 μm on Mars.
Planetary and Space Science,2013,85:243-249
|
被引
1
次
|
|
|
|
|
20.
Lefevre F. Three-dimensional modeling of ozone on Mars.
Journal of Geophysical Research: Planets,2004,109(E7):E07004
|
被引
2
次
|
|
|
|
|
了解气象卫星更多信息，请访问