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排序方式: 共有150条查询结果,搜索用时 31 毫秒
91.
92.
A. Tříska Č. Barta F. Vodák 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1983,3(5):187-189
The creep of polycrystalline Hg2X2 (where X = Cl, Br, J) under the terrestrial and space conditions is studied in the present experiment. The authors suppose that the creep of the Hg2X2 cylindrical sample can be studied by the help of the theory of micropolar (non-Newtonian) fluids. In accordance with this theory we obtain the flux of fluid through any cross-section as functions of the radius, viscosity coefficients, the gradient of pressure and the gravity acceleration. In this paper a comparison of the theoretical results for normal and zero- gravity conditions is given. It is shown that the annealing of materials having a broad region of plasticity under microgravity conditions can lead to great improvement in optical as well as mechanical qualities of the crystal. Technical aspects of the experiment are also described. 相似文献
93.
R Marco J González-Jurado M Calleja R Garesse M Maroto E Ramírez M C Holgado E de Juan J Miquel 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1992,12(1):157-166
The results are presented of the exposure of Drosophila melanogaster to microgravity conditions during a 15-day biosatellite flight, Biokosmos 9, in a joint ESA-URSS project. The experimental containers were loaded before launch with a set of Drosophila melanogaster Oregon R larvae so that imagoes were due to emerge half-way through the flight. A large number of normally developed larvae were recovered from the space-flown containers. These larvae were able to develop into normal adults confirming earlier results that Drosophila melanogaster of a wild-type constitution can develop normally in the absence of gravity. However, microgravity exposure clearly enhances the number of growing embryos laid by the flies and possibly slows down the developmental pace of the microgravity-exposed animals. Due to some problems in the experimental set-up, this slowing down needs to be verified in future experiments. No live adult that had been exposed to microgravity was recovered from the experiment, so that no life span studies could be carried out, but adult males emerged from the recovered embyros showed a slight shortening in life span and a lower performance in other experimental tests of aging. This agrees with the results of previous experiments performed by our groups. 相似文献
94.
95.
J.A. Pyle A.M. Závody J.E. Harries P.H. Moffat 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,4(4):117-120
Stratospheric concentrations of OH have been derived from LIMS measurements of minor constituents. Two methods have been used. Assuming that HNO3 and NO2 are in photochemical steady state, LIMS measurements of these species, with knowledge of appropriate rate constants and a calculation of the HNO3 photolysis rate, allow nearly global fields of OH to be derived. The derived profiles show satisfactory agreement with observations. As a check on our method, OH has also been derived by calculations of its sources and sinks using LIMS measurements of H2O. The two methods agree extremely well in low latitudes. At higher latitudes the agreement is less satisfactory. This is discussed in terms of the diurnal behaviour of the species and the time constant of the HNO3/NO2 equilibrium. 相似文献
96.
Arnaud Masson Ondrej Santolík Donald L. Carpenter Fabien Darrouzet Pierrette M. E. Décréau Farida El-Lemdani Mazouz James L. Green Sandrine Grimald Mark B. Moldwin František Němec Vikas S. Sonwalkar 《Space Science Reviews》2009,145(1-2):137-191
This paper highlights significant advances in plasmaspheric wave research with Cluster and Image observations. This leap forward was made possible thanks to the new observational capabilities of these space missions. On one hand, the multipoint view of the four Cluster satellites, a unique capability, has enabled the estimation of wave characteristics impossible to derive from single spacecraft measurements. On the other hand, the Image experiments have enabled to relate large-scale plasmaspheric density structures with wave observations and provide radio soundings of the plasmasphere with unprecedented details. After a brief introduction on Cluster and Image wave instrumentation, a series of sections, each dedicated to a specific type of plasmaspheric wave, put into context the recent advances obtained by these two revolutionary missions. 相似文献
97.
A methodology based on point-like sources is discussed, enabling a reliable estimate of the acceleration of the Pioneer 10 and 11 probes caused by thermal effects. A sensitivity analysis of the several parameters of the model allows for a clear indication of the possible thermal origin of the so-called Pioneer anomaly. 相似文献
98.
M. A. Allodi R. A. Baragiola G. A. Baratta M. A. Barucci G. A. Blake P. Boduch J. R. Brucato C. Contreras S. H. Cuylle D. Fulvio M. S. Gudipati S. Ioppolo Z. Kaňuchová A. Lignell H. Linnartz M. E. Palumbo U. Raut H. Rothard F. Salama E. V. Savchenko E. Sciamma-O’Brien G. Strazzulla 《Space Science Reviews》2013,180(1-4):101-175
99.
J. R. Szalay A. R. Poppe J. Agarwal D. Britt I. Belskaya M. Horányi T. Nakamura M. Sachse F. Spahn 《Space Science Reviews》2018,214(5):98
Airless bodies are directly exposed to ambient plasma and meteoroid fluxes, making them characteristically different from bodies whose dense atmospheres protect their surfaces from such fluxes. Direct exposure to plasma and meteoroids has important consequences for the formation and evolution of planetary surfaces, including altering chemical makeup and optical properties, generating neutral gas and/or dust exospheres, and leading to the generation of circumplanetary and interplanetary dust grain populations. In the past two decades, there have been many advancements in our understanding of airless bodies and their interaction with various dust populations. In this paper, we describe relevant dust phenomena on the surface and in the vicinity of airless bodies over a broad range of scale sizes from \(\sim10^{-3}~\mbox{km}\) to \(\sim10^{3}~\mbox{km}\), with a focus on recent developments in this field. 相似文献
100.
Lucie M. Green Tibor Török Bojan Vršnak Ward ManchesterIV Astrid Veronig 《Space Science Reviews》2018,214(1):46
Coronal mass ejections (CMEs) were discovered in the early 1970s when space-borne coronagraphs revealed that eruptions of plasma are ejected from the Sun. Today, it is known that the Sun produces eruptive flares, filament eruptions, coronal mass ejections and failed eruptions; all thought to be due to a release of energy stored in the coronal magnetic field during its drastic reconfiguration. This review discusses the observations and physical mechanisms behind this eruptive activity, with a view to making an assessment of the current capability of forecasting these events for space weather risk and impact mitigation. Whilst a wealth of observations exist, and detailed models have been developed, there still exists a need to draw these approaches together. In particular more realistic models are encouraged in order to asses the full range of complexity of the solar atmosphere and the criteria for which an eruption is formed. From the observational side, a more detailed understanding of the role of photospheric flows and reconnection is needed in order to identify the evolutionary path that ultimately means a magnetic structure will erupt. 相似文献