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81.
ISO performed a large variety of observing programmes on comets, asteroids and zodiacal light – covering about 1% of the archived
observations – with a surprisingly rewarding scientific return. Outstanding results were related to the exceptionally bright
comet Hale–Bopp and to ISO's capability to study in detail the water spectrum in a direct way. But many other results were
broadly recognised: Discovery of new molecules in comets, the studies of crystalline silicates, the work on asteroid surface
mineralogy, results from thermophysical studies of asteroids, a new determination of the asteroid number density in the main-belt
and last but not least, the investigations on the spatial and spectral features of the zodiacal light. 相似文献
82.
P. Lukáč A. Meňovský Z. Trojanová J. Krumpos 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(5):73-76
The crystal growth under near-zero gravity conditions may lead to materials of better crystalline and compositional perfection [1]. Unidirectional solidification of metals is a part of Czechoslovak programme on space research within the framework of Interkosmos [2]. On the model-like systems of metals grown in the space we want to study the effect of foreign atoms on the surface tension and the lattice defects density. The objectives of our ground-based and space experiments are discussed. 相似文献
83.
J. Eró K. Kecskeméty T. Kovács G. Kozma I. Náday A. Somogyi L. Szabó I. T-Szücs A. Zarándy 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(3):173-176
A charged particle semiconductor-telescope is under construction in the CRIP, Budapest, to measure fluxes of 4–30 MeV/AMU protons, alphas, and M nuclei in interplanetary space. Identification and counting of particles are made on-board using microprocessor techniques. Details including some new ideas on economical coding of information and design of electronics are given. 相似文献
84.
85.
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
86.
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
87.
88.
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
89.
K. Watanabe R.P. Lin S. Krucker R.J. Murphy G.H. Share M.J. Harris M. Gros Y. Muraki T. Sako Y. Matsubara T. Sakai S. Shibata J.F. Valds-Galicia L.X. Gonzlez A. Hurtado O. Musalem P. Miranda N. Martinic R. Ticona A. Velarde F. Kakimoto Y. Tsunesada H. Tokuno S. Ogio 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009,44(7):789-793
Relativistic neutrons were observed by the neutron monitors at Mt. Chacaltaya and Mexico City and by the solar neutron telescopes at Chacaltaya and Mt. Sierra Negra in association with an X17.0 flare on 2005 September 7. The neutron signal continued for more than 20 min with high statistical significance. Intense emissions of γ-rays were also registered by INTEGRAL, and during the decay phase by RHESSI. We analyzed these data using the solar-flare magnetic-loop transport and interaction model of Hua et al. [Hua, X.-M., Kozlovsky, B., Lingenfelter, R.E. et al. Angular and energy-dependent neutron emission from solar flare magnetic loops, Astrophys. J. Suppl. Ser. 140, 563–579, 2002], and found that the model could successfully fit the data with intermediate values of loop magnetic convergence and pitch-angle scattering parameters. These results indicate that solar neutrons were produced at the same time as the γ-ray line emission and that ions were continuously accelerated at the emission site. 相似文献
90.
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