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991.
I review standard big bang nucleosynthesis and some versions of nonstandard BBN. The abundances of the primordial isotopes D, He-3, and Li-7 produced in standard BBN can be calculated as a function of the baryon density with an accuracy of about 10%. For He-4 the accuracy is better than 1%. The calculated abundances agree fairly well with observations, but the baryon density of the universe cannot be determined with high precision. Possibilities for nonstandard BBN include inhomogeneous and antimatter BBN and nonzero neutrino chemical potentials. 相似文献
992.
993.
D.N.H. Horler M. Dockray J. Barber A.R. Barringer 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1983,3(2):273-277
The feasibility of using the wavelength of the maximum slope of the red edge of leaf reflectance spectra (λre) as an indication of plant chlorophyll status was examined in the laboratory for single leaves of several species. λre for each sample was determined by derivative reflectance spectroscopy. A high positive correlation was found between λre and leaf chlorophyll content for all species, although there were some differences in the quantitative nature of the relationship for plants of different types. The position of the red edge was found to be unaffected by simulated change in ground cover, but multiple leaf layers produced a shift in its position. Appropriate spectral measurements and processing for obtaining useful information from the red edge are discussed, and the potential of the red edge in relation to other spectral measurements is considered. 相似文献
994.
We review the details of the glint (angular scintillation) problem in electromagnetic scattering. These results are employed to develop a statistical glint and radar cross section (RCS) target model featuring the correct glint probability density function, the correct time correlations of RCS and glint, and the correct cross correlation between RCS and glint. This model is suitable for simulation applications, and an implementation scheme for a glint/RCS signal generator is included. 相似文献
995.
R H Anken M Beier H Rahmann 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2002,30(4):721-725
Inner ear stones (otoliths) of larval cichlid fish Oreochromis mossambicus were marked with the calcium-tracer alizarin-complexone (AC) at 1 g earth gravity before and after a 3, 7, 14 or 21 days stay of the animals at hypergravity conditions (hg; 3 g, centrifuge). After the experiment, the otoliths' area between the two AC-labellings was measured with regard to size and asymmetry (size difference between the left and the right stones). Both utricular and saccular otoliths (lapilli and sagittae, respectively) continued growing in a linear way at hg, but growth was significantly slowed down as compared to parallely raised 1 g-control specimens. In case of bilateral asymmetry between the corresponding otoliths its formation in hg-animals became reduced as compared to the 1 g controls. The reduction of asymmetry was much more pronounced in the sagittae than in the lapilli. The latter result supports an earlier hypothesis, according to which especially a low sagittal asymmetry has a functional advantage. In general, the results strongly suggest that otolith growth is continuously regulated in dependence of the environmental gravity vector. 相似文献
996.
997.
J. Nishimura H. Hirosawa O. Ohta H. Akiyama T. Yamagami 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1983,3(6):67-70
A relay balloon system for long-duration or large-area observations is described. The system consists of a balloon for scientific observations and a relay balloon for a data-relay terminal between a ground station and the balloon for observation. The system was successfully applied to the observation of electric-power fields (50 and 60 Hz) over the Pacific ocean. The maiximum distance between two balloons was about 1100 km and that between the Sanriku Balloon Center and the main balloon for the observation was about 1300 km. 相似文献
998.
H. Elliot 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1983,3(7):45-52
Space research in Western Europe began in the form of independent national space programmes confined in the first instance to the use of sounding rockets. These early steps were soon supplemented by bilateral collaborative projects with the USA and USSR whose agencies provided the satellite launch vehicles that Europe lacked at that time.In 1962 as a result of an agreement between ten member states the European Space Research Organisation (ESRO) was established for the purpose of carrying out a programme of space science. ESRO was succeeded in 1974 by the European Space Agency (ESA) with a much broader range of activities covering both scientific research and the application of space technology together with the development of launch vehicles.At the present time the totality of space activities of the ESA member states is made up of national programmes and collaborative projects with other nations and agencies together with participation in the agreed ESA programme. Because of its essentially non-military character, its relatively modest level of funding and its multinational nature the European experience with ESA may provide some useful guidance in the development of space science and technology elsewhere in the world. 相似文献
999.
W.D. Carter T.H. Kiilsgaard 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1983,3(2):113-123
The Yangjiatan tungsten district at latitude 27°28′ N. and longitude 111°54′E. is located about 140 km southwest of the city of Changsha and 35 km northeast of the town of Shaoyang, southeast Hunan Province, People's Republic of China. The deposits, consisting largely of scheelite in veins (Wang, 1975), are contained in highly folded and faulted sedimentary rocks of Paleozoic, Mesozoic, and Cenozoic age intruded by granitic plutons that are circular in plan view. The major faults and folds trend in a northeasterly direction; whereas, the plutons are clustered in a more easterly trending band across the Landsat image.Landsat image E-2338-02202, acquired December 26, 1975, is number 470 in the “Landsat Image Atlas of the People's Republic of China” printed by the Publishing House of Geology in 1979. A computer-compatible tape of the image was analyzed and used as a demonstration project under a United Nations technical assistance program. Supervised classification of soils, rocks, and vegetation; band ratioing to detect limonite alteration; and edge enhancement were all conducted to demonstrate the flexibility and capability of interactive computer systems. Field evaluation of the results of this work will be conducted by colleagues of the Remote Sensing Center for Geology, Ministry of Geology, in China. 相似文献
1000.
Lawrence C. Rowan Alexander F.H. Goetz Marguerite J. Kingston 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1983,3(2):125-132
The Shuttle Multispectral Infrared Radiometer (SMIRR) is a spectroradiometer covering the region from 0.5 to 2.5 μm in 10 channels that acquired data from spots 100 m in diameter along the subspacecraft ground track. It was flown aboard the second flight of the space shuttle Columbia, November 12–14, 1981. Data collected during orbit 16 over southern Egypt show that carbonate rocks, kaolinite, and possibly montmorillonite can be identified by their SMIRR spectral signatures and limited knowledge of the lithologic units present. Detailed analysis of SMIRR data for this area indicates that calcite, kaolinite, and montmorillonite rocks give rise to absorption features that result in characteristic 10 channel spectra. 相似文献