L. Huguenin ( 1979 ), Mars surface composition from reflectance spectroscopy: A summary , J. Geophys. Res. , 84 , 8415 – 8416 .Singer, R. B. , T. B. McCord , R. N. Clark , J. B. Adams , R. L. Huguenin , Mars surface composition from reflectance spectroscopy: A summary , ...
由中国科学院上海技术物理研究所负责研制的火星表面成分探测仪MarSCoDe (Mars Surface Composition Detector) 是我国首台LIBS行星物质成分分析仪，搭载在“祝融”号火星车成功着陆并开展科学任务，仪器的结构设计、功能及实现等研究内容将以封面文章的形式发表在国际老牌光谱期刊《Atomic Spectroscopy》上（https://doi.org/...
The six scientific payloads2 include NaTeCam3, Multispectral Camera (MSCam), Mars Rover Penetrating Radar (RoPeR)4, Mars surface Composition Detector (MarSCoDe)7, Mars Rover Magnetometer (RoMAG)6, and Mars Climate Station (MCS)5. Two pairs of hazard avoidance cameras (HazCam), of engineering...
Mars - Atmosphere, Structure, Composition: The vertical structure of the Martian atmosphere—that is, the relation of temperature and pressure to altitude—is determined partly by a complicated balance of several energy-transport mechanisms and partly by
(called sols) on the surface of Mars. It is equipped with high-resolution cameras for photographing andmapping its Utopia Planita home. The rover also carries a subsurface radar to look inside the Martian surface, a multi-spectral camera and surface composition detector, a magnetic field ...
Geography and Composition Mars is characterized its barren, rocky surface, which is covered with a thick layer of iron oxide, or rust, giving it its distinctive red color. The planet's landscape features a variety of terrain, including vast plains, towering volcanoes, and deep canyons. One of...
- 《Journal of Geophysical Research Planets》 被引量: 128发表: 2005年 The Mars Geoscience/Climatology Orbiter 1990 mission The fundamental objectives of the Mars Geoscience/Climatology Orbiter (MGCO) 1990 mission are related to the determination of the surface composition and t... GD Low,JR ...
The Observatoire pour La Minéralogie, l'Eau, les Glaces,et l'Activité (OMEGA) investigation, on board the EuropeanSpace Agency Mars Express mission, is mapping the surface composition ofMars at a 0.3- to 5-kilometer resolution by means ofvisible-near-infrared hyperspectral reflectance imagery. ...
Therefore, one of the outstanding questions is whether the mantle is subject to convective motions at the present day or the convection ceased sometime in the past. Given the absence of a magnetic field and uncertainties on the Martian core’s chemical composition2, the Martian core could still...
K. Hamara (2006) Composition of northern low-albedo regions of Mars: Insights from the Mars Odyssey Gamma Ray Spectrometer, J. Geophys. Res., 111, doi:10.1029/2006JE002675.Karunatillake, S. K., et al. (2006), Composition of northern low-albedo regions of Mars: Insights from the Mars ...