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151.
Des Marais DJ Nuth JA Allamandola LJ Boss AP Farmer JD Hoehler TM Jakosky BM Meadows VS Pohorille A Runnegar B Spormann AM 《Astrobiology》2008,8(4):715-730
The NASA Astrobiology Roadmap provides guidance for research and technology development across the NASA enterprises that encompass the space, Earth, and biological sciences. The ongoing development of astrobiology roadmaps embodies the contributions of diverse scientists and technologists from government, universities, and private institutions. The Roadmap addresses three basic questions: how does life begin and evolve, does life exist elsewhere in the universe, and what is the future of life on Earth and beyond? Seven Science Goals outline the following key domains of investigation: understanding the nature and distribution of habitable environments in the universe, exploring for habitable environments and life in our own Solar System, understanding the emergence of life, determining how early life on Earth interacted and evolved with its changing environment, understanding the evolutionary mechanisms and environmental limits of life, determining the principles that will shape life in the future, and recognizing signatures of life on other worlds and on early Earth. For each of these goals, Science Objectives outline more specific high priority efforts for the next three to five years. These eighteen objectives are being integrated with NASA strategic planning. 相似文献
152.
配置管理是PDM的核心业务基础,本文从论述实现PDM应用中配置管理功能的重要性出发,介绍分析了国际上多种标准对配置管理的基本要求和方法. 相似文献
153.
Koczela Louis J. Burnett Gerald J. 《IEEE transactions on aerospace and electronic systems》1968,(3):456-467
Computer requirements for future space missions are developed and three different approaches to multiprocessing computer organizations are presented. These approaches are shown to have considerable advantages over conventional computers for advanced space missions. Reliability requirements also are assessed by a simulation method and shown to be attainable for long-duration missions. 相似文献
154.
One long-standing difficulty in estimating the large-scale ocean circulation is the inability to observe absolute current
velocities. Both conventional hydrographic measurements and altimetric measurements provide observations of currents relative
to an unknown velocity at a reference depth in the case of hydrographic data, and relative to mean currents calculated over
some averaging period in the case of altimetric data. Space gravity missions together with altimetric observations have the
potential to overcome this difficulty by providing absolute estimates of the velocity of surface oceanic currents. The absolute
surface velocity estimates will in turn provide the reference level velocities that are necessary to compute absolute velocities
at any depth level from hydrographic data.
Several studies have been carried out to quantify the improvements expected from ongoing and future space gravity missions.
The results of these studies in terms of volume flux estimates (transport of water masses) and heat flux estimates (transport
of heat by the ocean) are reviewed in this paper. The studies are based on ocean inverse modeling techniques that derive impact
estimates solely from the geoid error budgets of forthcoming space gravity missions. Despite some differences in the assumptions
made, the inverse modeling calculations all point to significant improvements in estimates of oceanic fluxes. These improvements,
measured in terms of reductions of uncertainties, are expected to be as large as a factor of 2.
New developments in autonomous ocean observing systems will complement the developments expected from space gravity missions.
The synergies of in situ and satellite observing systems are considered in the conclusion of this paper.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
155.
P Chagvardieff B Dimon A Souleimanov D Massimino S Le Bras M Pean D Louche-Teissandier 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1997,20(10):1971-1974
Wheat, potato, pea and tomato crops were cultivated from seeding to harvest in a controlled and confined growth chamber at elevated CO2 concentration (3700 microL L-1) to examine the effects on biomass production and edible part yields. Different responses to high CO2 were recorded, ranging from a decline in productivity for wheat, to slight stimulation for potatoes, moderate increase for tomatoes, and very large enhancement for pea. Mineral content in wheat and pea seeds was not greatly modified by the elevated CO2. Short-term experiments (17 d) were conducted on potato at high (3700 microL L-1) and very high (20,000 microL L-1) CO2 concentration and/or low O2 partial pressure (approximately 20,600 microL L-1 or 2 kPa). Low O2 was more effective than high CO2 in total biomass accumulation, but development was affected: Low O2 inhibited tuberization, while high CO2 significantly increased production of tubers. 相似文献
156.
Baqué M Le Postollec A Ravelet C Peyrin E Coussot G Desvignes I Incerti S Moretto P Dobrijevic M Vandenabeele-Trambouze O 《Astrobiology》2011,11(3):207-211
Biochips are promising instruments for the search for organic molecules in planetary environments. Nucleic acid aptamers are powerful affinity receptors known for their high affinity and specificity, and therefore are of great interest for space biochip development. A wide variety of aptamers have already been selected toward targets of astrobiological interest (from amino acids to microorganisms). We present a first study to test the resistance of these receptors to the constraints of the space environment. The emphasis is on the effect of cosmic rays on the molecular recognition properties of DNA aptamers. Experiments on beam-line facilities have been conducted with 2 MeV protons and fluences much higher than expected for a typical mission to Mars. Our results show that this irradiation process did not affect the performances of DNA aptamers as molecular recognition tools. 相似文献
157.
Gauvrit H. Le Cadre J.P. Jauffret C. 《IEEE transactions on aerospace and electronic systems》1997,33(4):1242-1257
Traditional multihypothesis tracking methods rely upon an enumeration of all the assignments of measurements to tracks. Pruning and gating are used to retain only the most likely hypotheses in order to drastically limit the set of feasible associations. The main risk is to eliminate correct measurement sequences. The probabilistic multiple hypothesis tracking (PMHT) method has been developed by Streit and Luginbuhl in order to reduce the drawbacks of "strong" assignments. The PMHT method is presented in a general mixture densities perspective. The Expectation-Maximization (EM) algorithm is the basic ingredient for estimating mixture parameters. This approach is then extended and applied to multitarget tracking for nonlinear measurement models in the passive sonar perspective. 相似文献
158.
159.
将三维MHD双温入口模型的计算结果作为入口条件,运用DSMC(Direct Simulation Monte-Carlo)/PIC(Particle in Cell)流体混合算法,模拟实验室PPT样机羽流。验证计算显示,该模型具有模拟脉冲等离子体推力器羽流的能力。对不同初始电压和电容下的羽流场进行了模拟,给出了出口平面返流质量流率的变化情况和20μs羽流中离子和CEX离子的分布情况。计算结果显示,高能量状态对应高质量流率,高质量流率对应高动量,高动量离子和中性粒子对航天器撞击会造成更强影响。 相似文献
160.