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411.
Shaping peace     
Soviet General Secretary Gorbachev, in his January 1986 speech, expressed a hope that the level of nuclear weapons would before long be greatly reduced. The Soviet Embassy in Sri Lanka invited Arthur C. Clarke to comment on the General Secretary's speech. This article is his response.  相似文献   
412.
This article presents the views of the Boeing company on the benefits and disadvantages of international participation in the space station. The author outlines the company's goals within the project, and makes some recommendations on how to reduce the concerns which arise from international cooperation, in order to maximize the benefits which could be achieved.  相似文献   
413.
Cosmic Research - The results of an analysis of the space–time characteristics and dynamics of precipitations of magnetospheric electrons with energies in the range from 0.1 to 0.7 MeV are...  相似文献   
414.
Ugolnikov  O. S.  Maslov  I. A. 《Cosmic Research》2021,59(4):305-305
Cosmic Research - An Erratum to this paper has been published: https://doi.org/10.1134/S0010952521110010  相似文献   
415.
Kaportseva  K. B.  Shugay  Yu. S. 《Cosmic Research》2021,59(6):537-537
Cosmic Research - An Erratum to this paper has been published: https://doi.org/10.1134/S0010952521120017  相似文献   
416.
Initial preconditions for solving the problem of ballistic-navigation design of a future-technology space navigation system (SNS) are presented. A technical approach to the SNS design is proposed, whose basis is theoretical results in the field of space navigation applied to the orbital satellite groups, generating the global radio navigation field (RNF) with optimum navigation properties. The mathematical apparatus adequate to the proposed technical approach is introduced to analyze the structure of the orbital group and radio navigation field.  相似文献   
417.
输油管道泄漏自动检测装置的研制   总被引:3,自引:0,他引:3  
介绍一种基于软件的管道泄漏自动检测装置 ,通过检测压力、流量、温度等的变化来判断泄漏是否发生及发生泄漏的位置。该装置具有适应性广、安装简单等优点。  相似文献   
418.
Earth's subsurface offers one of the best possible sites to search for microbial life and the characteristic lithologies that life leaves behind. The subterrain may be equally valuable for astrobiology. Where surface conditions are particularly hostile, like on Mars, the subsurface may offer the only habitat for extant lifeforms and access to recognizable biosignatures. We have identified numerous unequivocally biogenic macroscopic, microscopic, and chemical/geochemical cave biosignatures. However, to be especially useful for astrobiology, we are looking for suites of characteristics. Ideally, "biosignature suites" should be both macroscopically and microscopically detectable, independently verifiable by nonmorphological means, and as independent as possible of specific details of life chemistries--demanding (and sometimes conflicting) criteria. Working in fragile, legally protected environments, we developed noninvasive and minimal impact techniques for life and biosignature detection/characterization analogous to Planetary Protection Protocols. Our difficult field conditions have shared limitations common to extraterrestrial robotic and human missions. Thus, the cave/subsurface astrobiology model addresses the most important goals from both scientific and operational points of view. We present details of cave biosignature suites involving manganese and iron oxides, calcite, and sulfur minerals. Suites include morphological fossils, mineral-coated filaments, living microbial mats and preserved biofabrics, 13C and 34S values consistent with microbial metabolism, genetic data, unusual elemental abundances and ratios, and crystallographic mineral forms.  相似文献   
419.
Eichler D  Beskin G 《Astrobiology》2001,1(4):489-493
We propose using large Air Cerenkov telescopes (ACTs) to search for optical, pulsed signals from extraterrestrial intelligence. Such dishes collect tens of photons from a nanosecond-scale pulse of isotropic equivalent power of tens of solar luminosities at a distance of 100 pc. The field of view for giant ACTs can be on the order of 10 square degrees, and they will be able to monitor 10-100 stars simultaneously for nanosecond pulses of about 6th magnitude or brighter. Using the Earth's diameter as a baseline, orbital motion of the planet could be detected by timing the pulse arrivals.  相似文献   
420.
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