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931.
K Lumme J Peltoniemi W M Irvine 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1990,10(1):187-193
We discuss various photometric techniques and their absolute scales in relation to the information that can be derived from the relevant data. We also outline a new scattering model for atmosphereless bodies in the solar system and show how it fits Mariner 10 surface photometry of the planet Mercury. It is shown how important the correct scattering law is while deriving the topography by photoclinometry. 相似文献
932.
W K Sinclair 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1994,14(10):879-884
Radiation protection involves the limitation of exposure to below threshold doses for direct (or deterministic) effects and a knowledge of the risk of stochastic effects after low doses. The principal stochastic risk associated with low dose rate galactic cosmic rays is the increased risk of cancer. Estimates of this risk depend on two factors (a) estimates of cancer risk for low-LET radiation and (b) values of the appropriate radiation weighting factors, WR, for the high-LET radiations of galactic cosmic rays. Both factors are subject to considerable uncertainty. The low-LET cancer risk derived from the late effects of the atomic bombs is vulnerable to a number of uncertainties including especially that from projection in time, and from extrapolation from high to low dose rate. Nevertheless, recent low dose studies of workers and others tend to confirm these estimates. WR, relies on biological effects studied mainly in non-human systems. Additional laboratory studies could reduce the uncertainties in WR and thus produce a more confident estimate of the overall risk of galactic cosmic rays. 相似文献
933.
Patterson R.L. Rose A.H. Tang D. Day G.W. 《Aerospace and Electronic Systems Magazine, IEEE》1990,5(12):10-14
A robust, accurate, broadband, AC sensor using fiber optics that is being developed for space applications at power frequencies as high as 20 kHz is described. It can also be used in low- and high-voltage 60-Hz terrestrial power systems and in 400-Hz aircraft systems. It is intrinsically immune to electromagnetic interference (EMI) and has the added benefit of excellent isolation. The sensor uses the Faraday effect in optical fiber and standard polarimetric measurements to sense electrical current. The primary component of the sensor is a specially treated coil of single-mode optical fiber, through which the current-carrying conductor passes. Improved precision is accomplished by temperature compensation by means of signals from a novel fiber-optic temperature sensor embedded in the sensing head. The technology used in the sensor is discussed, and the results of precision tests conducted at various temperatures within the wide operating range as well as the results of early EMI tests are reported 相似文献
934.
R C Morrow R J Bula T W Tibbitts W R Dinauer 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1994,14(11):29-37
A flight experiment, ASTROCULTURE(TM)-1 (ASC-1), to evaluate the operational characteristics and hardware performance of a porous tube nutrient delivery system (PTNDS) was flown on STS-50 as part of the U.S. Microgravity Laboratory-1 mission, 25 June to 9 July, 1992. This experiment is the first in a series of planned ASTROCULTURE(TM) flights to validate the performance of subsystems required to grow plants in microgravity environments. Results indicated that the PTNDS was capable of supplying water and nutrients to plants in microgravity and that its performance was similar in microgravity to that in 1g on Earth. The data demonstrated that water transfer rates through a rooting matrix are a function of pore size of the tubes, the degree of negative pressure on the 'supply' fluid, and the pressure differential between the 'supply' and 'recovery' fluid loops. A slightly greater transfer rate was seen in microgravity than in 1g, but differences were likely related to the presence of hydrostatic pressure effects at 1g. Thus, this system can be used to support plant growth in microgravity or in partial gravity as on a lunar or Mars base. Additional subsystems to be evaluated in the ASTROCULTURE(TM) flight series of experiments include lighting, humidity control and condensate recovery, temperature control, nutrient composition control, CO2 and O2 control, and gaseous contaminant control. 相似文献
935.
This guide introduces the basics of neural networks and is intended to prepare the reader to search, read, use, and understand the literature. A brief history is followed by a section devoted to keywords, phrases, and definitions. The basic building blocks with illustrations are included. A matrix of major neural-network paradigms with intended use and suggested applications is presented. Recommended readings and software programs with problem types are suggested. The potentials and limitations of neural networks are highlighted 相似文献
936.
E W Lang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1986,6(12):251-255
Water is an indispensable prerequisite for the existence of life. Only in an aqueous environment can biomolecules take up their native, tertiary structure and organize themselves into higher aggregates like multienzyme complexes or cell-organelles. In most of these processes interactions between biomolecules and water play an important role. The influence of pressure and temperature upon intramolecular interactions of biopolymers and biopolymer-water interactions are discussed. Because of fast hydrolysis biomolecules should be unstable at T > or = 500 K. Hydrostatic pressure leads to an accelerated hydrolysis. The p,T-dependence of hydrophobic interactions suggest an even lower upper boundary around T approximately 400 K. In the model system t-butanol/water compression weakens hydrophobic interactions. However, within the modest pressure range p < or = 120 MPa observed on earth hydrostatic pressure does not seem to limit the stability of biomolecules at temperatures below 400 K severely. 相似文献
937.
W Schimmerling 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1992,12(2-3):445-459
The mean free path for nuclear interactions of galactic cosmic-rays is comparable to shielding and tissue thicknesses present in human interplanetary exploration, resulting in a significant fraction of nuclear reaction products at depth. In order to characterize the radiation field, the energy spectrum, the angular distribution, and the multiplicity of each type of secondary particles must also be known as a function of depth. Reactions can take place anywhere in a thick absorber; therefore, it is necessary to know these quantities as a function of particle energy for all particles produced. HZE transport methods are used to predict the radiation field; they are dependent on models of the interaction of man-made systems with the space environment to an even greater extent than methods used for other types of radiation. Hence, there is a major need to validate these transport codes by comparison with experimental data. The most cost-effective method of validation is a comparison with ground-based experimental measurements. A research program to provide such validation measurements using neon, iron and other accelerated heavy ion beams will be discussed and illustrated using results from ongoing experiments and their comparison with current transport codes. The extent to which physical measurements yield radiobiological predictions will be discussed. 相似文献
938.
B. S. NG W. H. REID Department of Mathematical Sciences Indiana University Purdue University Indianapolis Indiana 《南京航空航天大学学报(英文版)》2001,18(Z1)
INTRODUCTIONLarge- scale complex eigenvalue problemsarising in continuum physics and engineering ap-plications are important not only because theyyield fundamental knowledge on the systems be-ing studied,they also provide a challenging con-textforthe developmentof numerical and analyt-ical techniques in their solution.In this paper,we re- examine the well- known Orr- Sommerfeldproblem which governs the linear stability of par-allel shear flows.More specifically,we are con-cerned with the … 相似文献
939.
Deutsche Aerospace Airbus (division of DASA) and Rosemount Aerospace Inc. Jointly sponsored a flight test program to evaluate in-flight performance of distributed multifunction air data smart probes. The probes measure pitot pressure, static pressure, and angle of attack. The tests were conducted at the DLR Flight Test Center, near Braunschweig, Germany. Two smart probes were installed on the DLR VFW 614 ATTAS Flight Test Aircraft and tested between June of 1992 and January of 1993. Flight test results are presented together with suggested air data system architectures, including ARINC 738, that can be used with the distributed smart probe concept. New architectures are developed for future commercial aircraft. The smart probe concept offers several advantages including reduced weight and size, reduced number of line replaceable units (LRUs), and increased reliability. Overall cost of ownership is significantly lowered 相似文献
940.
Wiring system failures have resulted from arc propagation in the wiring harnesses of many aircraft and space vehicles. These failures occur when the insulation becomes conductive upon the initiation of an arc. In some cases, the conductive path of the carbon arc track displays a high enough resistance such that the current is limited, and therefore may be difficult to detect using conventional circuit protection. Often, such wiring failures are not simply the result of insulation failure but are due to a combination of wiring system factors. Inadequate circuit protection, unreliable system designs, and careless maintenance procedures can contribute to a wiring system failure. This paper approaches the problem with respect to the overall wiring system, in order to determine what steps can be taken to improve the reliability, maintainability, and safety of space power systems. Power system technologies, system designs, and maintenance procedures which have contributed to past wiring system failures are discussed. New technologies, design processes, and management techniques which may lead to improved wiring system safety are introduced 相似文献