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The martian surface environment exhibits extremes of salinity, temperature, desiccation, and radiation that would make it difficult for terrestrial microbes to survive. Recent evidence suggests that martian soils contain high concentrations of MgSO? minerals. Through warming of the soils, meltwater derived from subterranean ice-rich regolith may exist for an extended period of time and thus allow the propagation of terrestrial microbes and create significant bioburden at the near surface of Mars. The current report demonstrates that halotolerant bacteria from the Great Salt Plains (GSP) of Oklahoma are capable of growing at high concentrations of MgSO? in the form of 2 M solutions of epsomite. The epsotolerance of isolates in the GSP bacterial collection was determined, with 35% growing at 2 M MgSO?. There was a complex physiological response to mixtures of MgSO? and NaCl coupled with other environmental stressors. Growth also was measured at 1 M concentrations of other magnesium and sulfate salts. The complex responses may be partially explained by the pattern of chaotropicity observed for high-salt solutions as measured by agar gelation temperature. Select isolates could grow at the high salt concentrations and low temperatures found on Mars. Survival during repetitive freeze-thaw or drying-rewetting cycles was used as other measures of potential success on the martian surface. Our results indicate that terrestrial microbes might survive under the high-salt, low-temperature, anaerobic conditions on Mars and present significant potential for forward contamination. Stringent planetary protection requirements are needed for future life-detection missions to Mars. 相似文献
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Litvak ML Mitrofanov IG Barmakov YN Behar A Bitulev A Bobrovnitsky Y Bogolubov EP Boynton WV Bragin SI Churin S Grebennikov AS Konovalov A Kozyrev AS Kurdumov IG Krylov A Kuznetsov YP Malakhov AV Mokrousov MI Ryzhkov VI Sanin AB Shvetsov VN Smirnov GA Sholeninov S Timoshenko GN Tomilina TM Tuvakin DV Tretyakov VI Troshin VS Uvarov VN Varenikov A Vostrukhin A 《Astrobiology》2008,8(3):605-612
We present a summary of the physical principles and design of the Dynamic Albedo of Neutrons (DAN) instrument onboard NASA's 2009 Mars Science Laboratory (MSL) mission. The DAN instrument will use the method of neutron-neutron activation analysis in a space application to study the abundance and depth distribution of water in the martian subsurface along the path of the MSL rover. 相似文献
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本文介绍了几种事后数值滤波技术。在数字遥测数据用于自动化计算机数据分析以前,利用这些技术减少或/和消除数字遥测数据中的噪声。这种遥测数据噪声来源于遥测载波信号过小或完全丢失,引起接收的脉码调制(PCM)数据出错。剔除错误的采样数据是事后分析中一项特别重要的工作,因为被污染数据可能给自动化计算机事后数据分析过程造成错误或偏差。当这些错误在最终换算后的数据中常接近测量值的上限或下限(数据跳点),很容易从采样数据中滤除。数据噪声偶尔表现为比较小的、不明显的波动,则分析员只有从图形(而不是数表)才能看出有噪声。因此,这类噪声更难于数字滤波。通常,采用手工噪声剔除或平滑,其结果变化较大。其主要缺点是:对现今的高采样率数字系统,采样数据量很大,因而耗时过大。另外,任何一种手工滤波总是对操作员依赖性很大。对错误采样数据的检测和识别显然是数据滤波中最困难的一步。我们已研究出几种识别方法,并在消除和平滑技术以前先加以详细介绍。研究了这些方法的技术局限性,对此也作了介绍。最后,对每种方法用图形绘出滤波处理前后的几组数据例子。 相似文献
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