Inferring the global cosmic dust influx to the Earth's atmosphere from lidar observations of the vertical flux of mesospheric Na

被引:48
|
作者
Gardner, Chester S. [1 ]
Liu, Alan Z. [2 ]
Marsh, D. R. [3 ]
Feng, Wuhu [4 ]
Plane, J. M. C. [4 ]
机构
[1] Univ Illinois, Dept Elect & Comp Engn, Urbana, IL 61820 USA
[2] Embry Riddle Aeronaut Univ, Dept Phys Sci, Daytona Beach, FL USA
[3] Natl Ctr Atmospher Res, Div Atmospher Chem, Boulder, CO 80307 USA
[4] Univ Leeds, Sch Chem, Leeds LS2 9JT, W Yorkshire, England
基金
欧洲研究理事会; 美国国家科学基金会; 中国国家自然科学基金;
关键词
STARFIRE OPTICAL-RANGE; DISSIPATING GRAVITY-WAVES; MESOPAUSE REGION; INPUT FUNCTION; CHEMICAL-MODEL; NEW-MEXICO; TRANSPORT; FLUCTUATIONS; ACCRETION; ABLATION;
D O I
10.1002/2014JA020383
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Estimates of the global influx of cosmic dust are highly uncertain, ranging from 0.4-110 t/d. All meteoric debris that enters the Earth's atmosphere is eventually transported to the surface. The downward fluxes of meteoric metals like mesospheric Na and Fe, in the region below where they are vaporized and where the majority of these species are still in atomic form, are equal to their meteoric ablation influxes, which in turn, are proportional to the total cosmic dust influx. Doppler lidar measurements of mesospheric Na fluxes made throughout the year at the Starfire Optical Range, New Mexico, (35 degrees N) are combined with the Whole Atmosphere Community Climate Model predictions of the relative geographic variations of the key wave-induced vertical transport processes to infer the global influxes of Na vapor and cosmic dust. The global mean Na influx is estimated to be 16,100 +/- 3200 atoms/cm(2)/s, which corresponds to 278 +/- 54 kg/d for the global input of Na vapor and 60 +/- 16 t/d for the global influx of cosmic dust.
引用
收藏
页码:7870 / 7879
页数:10
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