Design of a direct-detection wind and aerosol lidar for mars orbit

被引:13
作者
Cremons, Daniel R. [1 ]
Abshire, James B. [1 ,2 ]
Sun, Xiaoli [1 ]
Allan, Graham [1 ,3 ]
Riris, Haris [1 ]
Smith, Michael D. [1 ]
Guzewich, Scott [1 ]
Yu, Anthony [1 ]
Hovis, Floyd [4 ]
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Univ Maryland, College Pk, MD 20742 USA
[3] Sigma Space Corp, Lanham, MD USA
[4] Fibertek Inc, Herndon, VA USA
关键词
Mars; Lidar; Wind; Doppler; Remote sensing; Aerosol; DOPPLER LIDAR; RADIATIVE-TRANSFER; EDGE TECHNIQUE; ETALON FILTER; GALE CRATER; DUST; INTERFEROMETER; AIRBORNE; WATER;
D O I
10.1007/s12567-020-00301-z
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The present knowledge of the Mars atmosphere is greatly limited by a lack of global measurements of winds and aerosols. Hence, measurements of height-resolved wind and aerosol profiles are a priority for new Mars orbiting missions. We have designed a direct-detection lidar (MARLI) to provide global measurements of dust, winds and water ice profiles from Mars orbit. From a 400-km polar orbit, the instrument is designed to provide wind and backscatter measurements with a vertical resolution of 2 km and with resolution of 2 degrees in latitude along track. The instrument uses a single-frequency, seeded Nd:YAG laser that emits 4 mJ pulses at 1064 nm at a 250 Hz pulse rate. The receiver utilizes a 50-cm diameter telescope and a double-edge Fabry-Perot etalon as a frequency discriminator to measure the Doppler shift of the aerosol-backscatter profiles. The receiver also includes a polarization-sensitive channel to detect the cross-polarized backscatter profiles from water ice. The receiver uses a sensitive 4 x 4 pixel HgCdTe avalanche photodiode array as a detector for all signals. Here we describe the measurement concept, instrument design, and calculate its performance for several cases of Mars atmospheric conditions. The calculations show that under a range of atmospheric conditions MARLI is capable of measuring wind speed profiles with random error of 2-4 m/s within the first three scale heights, enabling vertically resolved mapping of transport processes in this important region of the atmosphere.
引用
收藏
页码:149 / 162
页数:14
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