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991.
O.A. Molchanov O.A. Maltseva E.E. Titova V.I. Di F. Jirˇi´cˇek P. Trˇi´ska 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1982,2(10):227-229
Signals of VLF transmitters of the Omega navigation system located in the auroral zone (66.4°N, 13.2°E, L= 5) were recorded by the VLF receiving equipment of the Interkosmos 19 satellite. Signals at frequencies between 10.2 and 13.6 kHz were received in a region above the transmitters, frequently with whistler-type echoes. An analysis of these echoes has shown their predominating occurrence in periods of low geomagnetic activity (Kp<2+). The occurrence region of these phenomena in the outer ionosphere has the dimension of about 1000 km and its position is betweenL= 2.5 and L= 4.4. The delay of echo-signals is practically the same during one satellite pass but its values for different satellite revolutions lie between 2.5 and 3.5 s. The frequency spectrum of these signals can be broadened up to 100 Hz. On the basis of calculations made, it can be shown that the experimental results are generally in accordance with the hypothesis of nonlinear ducting of VLF waves in the magnetosphere. 相似文献
992.
The effect of spectral bandwidth and spectral shape upon laser binary communication systems is investigated. The probability of error is plotted as a function of bandwidth for Lorentzian and Gaussian shaped spectra. The results show that even when the average noise power and the signal-to-noise ratio are held constant, the probability of error varies considerably as a function of spectral bandwidth. 相似文献
993.
994.
D. J. Lennon Paolo A. Mazzali F. Pasian P. Bonifacio V. Castellani 《Space Science Reviews》1993,66(1-4):169-172
Medium resolution (2A/px) but high s/n spectra of approximately twenty of the brightest blue stars in the young open cluster NGC 330 in the SMC have been analyzed in order to determine their atmospheric parameters and the evolutionary status. Stellar parameters are determined by comparison with LTE and NLTE model atmosphere calculations and an HR diagram constructed. Luminosities of the sample stars lie in the range 4.0L
*/L
)<5.0 and spectral types between O9 and late-B. The stars in our sample appear to define 4 groups: main-sequence B-stars (B2-B4), B-supergiants (B4) in a blue-loop phase of evolution, a small number of blue stragglers (O9-B0 near main-sequence stars) and a group of luminous giants (B1-B2) which reside in the so-called post main-sequence gap of the HR diagram. Furthermore, we have confirmed spectroscopically the very high incidence of Be stars in this cluster. Finally the almost complete absence of metal lines (at this resolution) is in keeping with the expected very low metallicity of the SMC. 相似文献
995.
R. Viotti A. Cassatella V. F. Polcaro G. B. Baratta A. Damineli Neto C. Rossi M. Barylak 《Space Science Reviews》1993,66(1-4):215-218
After many years of permanence at minimum, the luminous blue variable AG Car started in mid 1990 a new brightening phase. We review the spectroscopic variations of the star since 1949, and discuss the nature of the circumstellar nebula. We give evidence that, like in Car, also in AG Car dust is continuously condensing from the stellar wind. We suggest that the star could be partially reddened by the circumstellar dust, which could affect the estimates of the stellar distance. An extended HII
halo is present outside the ring nebula, which should be associated with the wind of a previous cooler evolutionary stage of AG Car. 相似文献
996.
Following our previously proposed technique, we have used the recent -ray observations of Mkr421 to place theoretically significant constraints on the magnitude of the intergalactic infrared radiation field (IIRF). Our 2 upper limits are consistent with normal IR production by stars and dust in galaxies. They rule out exotic mechanisms proposed to produce a larger IIRF. Although they are still subject to revision and are unconfirmed, the data on the spectrum of Mkr421 hint at a possible absorption cutoff which could be produced by an IIRF of the magnitude expected from stellar emission and reprocessing in galaxies. Using models for the low energy intergalactic photon spectrum from microwave to ultraviolet energies, we calculate the opacity of intergalactic space to -rays as a function of energy and redshift. These calculations indicate that the GeV -ray burst recently observed by the CGRO EGRET detector originates at a redshift less than 1.5. 相似文献
997.
Haupt GF 《Acta Astronautica》1991,25(11):733-736
The methods presently applied in the psychological training of astronauts are based on the principle of ensuring maximum performance of astronauts during missions. The shortcomings are obvious since those undergoing training provide nothing but the best ability to cope with Earth problem situations and add simply an experience of space problem situations as they are presently conceived. Earth attitudes and Earth behaviour remain and are simply modified. Through the utilization of interdisciplinary space knowledge a much higher degree of problem anticipation could be achieved and the astronaut be psychologically transformed into a space-being. This would at the same time stimulate interdisciplinary space research. The interdisciplinary space knowledge already available suggests that space requires not only physical and mental adjustments, but a profoundly new relationship with life. 相似文献
998.
The objective of this investigation was to evaluate the effect of a daily intake of fluid and salt supplementation (FSS) on bone mineralization in physically healthy male volunteers after exposure to hypokinesia (decreased number of steps taken/day) over a period of 364 days. The studies were performed after exposure to 364 days of hypokinesia (HK) on 18 physically healthy male volunteers who had an average VO2max of 65 ml/kg/min and were aged between 19 and 24 years. For the simulation of the hypokinetic effect the volunteers were kept under an average of 1000 steps/day. The subjects were divided into three equal groups of 6: 6 underwent a normal ambulatory life (control group), 6 were placed under HK (hypokinetic group) and the remaining 6 were subjected to HK and consumed a daily FSS (water 26 ml/kg body wt and NaCl 0.10 mg/kg body wt) (hyperhydrated group). The density of the ulnar, radius, tibia, fibular, lumbar vertebrae and calcenous was measured. Calcium and phosphorus changes, plasma volume, blood pressure and body weight were determined. Calcium content in the examined skeletal bones decreased more in the hypokinetic subjects than in the hyperhydrated subjects. Urinary calcium and phosphorus losses were more pronounced in hypokinetic than hyperhydrated subjects. Plasma volume and body weight increased in hyperhydrated subjects, while it decreased in hypokinetic subjects. It was concluded that a daily intake of FSS may be used to neutralize bone demineralization in physically healthy subjects during prolonged restriction of motor activity. 相似文献
999.
CROCODILE (CROissance de Cristaux Organiques par DIffusion Liquide dans l'Espace) is a space instrument dedicated to crystal growth from solution. The selected material N (4 nitrophenyl) (L) prolinol (NPP) is the result of studies on organic crystal in the frame of an extended program initiated by CNES for many years. The apparatus was flown aboard PHOTON, an automatic satellite, in April 1990, for a flight duration of more than 15 days. This paper describes the instrument design, with emphasis on specific and original technology well adapted to crystal growth from solution, and extendable to any space experiment on fluids. Preliminary details of the flight campaign will also be discussed. 相似文献
1000.
M. A. Barstow F. Wesemael J. B. Holberg K. Werner D. A. H. Buckley R. S. Stobie G. Fontaine S. R. Rosen S. Demers R. Lamontagne M. J. Irwin P. Bergeron S. O. Kepler S. Vennes 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1993,13(12):281-285
We report the discovery of two hot white dwarfs which have the lowest line-of-sight neutral hydrogen column densities yet measured. The stars were found independently by the ROSAT EUV, Montreal-Cambridge-Tololo, and Edinburgh-Cape surveys. Follow-up observations made using the Voyager 2 ultraviolet spectrometer reveal strong continua shortward of the 912Å Lyman limit from which we deduce that the neutral hydrogen column densities are 1.3 × 1017 and 2.0 × 1017 atoms cm−2. 相似文献