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11.
Shikha Raizada Christiano G.M. Brum John D. Mathews Cristina Gonzalez Efmi Franco 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(7):1850-1857
Electron concentration (Ne) inferred from Incoherent Scatter Radar (ISR) measurements has been used to determine the influence of solar flux and geomagnetic activity in the ionospheric E-region over Arecibo Observatory (AO). The approach is based on the determination of column integrated Ne, referred to as E-region total electron content (ErTEC) between 80 and 150 km altitude regions. The results discussed in this work are for the AO nighttime period. The study reveals higher ErTEC values during the low solar flux periods for all the seasons except for summer period. It is found that the E-region column abundance is higher in equinox periods than in the winter for low solar activity conditions. The column integrated Ne during the post-sunset/pre-sunrise periods always exceeds the midnight minima, independent of season or solar activity. This behavior has been attributed to the variations in the coupling processes from the F-region. The response of ErTEC to the geomagnetic variability is also examined for different solar flux conditions and seasons. During high solar flux periods, changes in Kp cause an ErTEC increase in summer and equinox, while producing a negative storm-like effect during the winter. Variations in ErTEC due to geomagnetic activity during low solar flux periods produce maximum variability in the E-region during equinox periods, while resulting in an increase/decrease in ErTEC before local midnight during the winter/summer periods, respectively. 相似文献
12.
S. Karakula W. Tkaczyk F. Giovannelli 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
In the spherical accretion onto massive objects, the matter may be heated up to temperatures as high as 1012 °K. In such a hot plasma, the thermal bremsstrahlung (e-e and e-p) and π° decay from inelastic collisions of protons are the main γ-ray sources. We determined the γ -ray production spectra from the π° decay and from bremsstrahlung for different temperatures. The expected γ-ray spectra were evaluated too in order to fit experimental data. We have fitted COS B data from 3C 273 using a two temperatures plasma model. The best fit is for
(M8 is the black hole mass in 108 M) which gives
. The hard X-ray measurements do not contradict the bremsstrahlung spectrum. 相似文献
Full-size image (1K)
13.
Miroslav Plavec R. Hoekstra C. De Jager Ji⋖´ Grygar J. Otterman H. M. van den Dool O. Namba C. J. Th. Gunsing Jean-Claude Pecker K. K. Kwee L. Perek D. Callebaut Jan Kuijpers W. de Graaff G. C. M. Reijnen B. Swanenburg N. Grevesse J. Kleczek P. P≙quet A. D. Fokker H. G. van Bueren D. Edgar Page R. J. van Duinen Franco Pacini 《Space Science Reviews》1978,21(4):469-483
14.
F. Giovannelli 《Space Science Reviews》1981,30(1-4):213-219
High speed photometry of the dwarf nova SS Cygni during an outburst reveals the presence of rapid oscillations detected over an interval of four days. The period of the oscillations ranged from a maximum of 9.91 s to a minimum of 8.96 s. The results are discussed from the view point of several current models. 相似文献
15.
D. E. Page M. Pick L. Kresák G. C. M. Reijnen A. G. W. Cameron Cornelius J. E. Schuurmans Mikhail Ya Marov B. Goldberg T. R. Kaiser J. Lemaire L. Sehnal H. Elsässer B. Valniček W. de Graaff Franco Pacini K. Rohlfs A. C. De Landtsheer I. D. Zhongolovich C. de Jager A. Greve J. Ruprecht R. J. Tayler G. Kockarts W. I. Axford H. Tabor H. J. Bolle E. Kaldis Gijsbertha C. M. Reijnen C. de Loore J. Kleczek C. A. Murray Åke Wallenquist 《Space Science Reviews》1981,28(1):105-118
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17.
F. Giovannelli M. Ferrari-Toniolo A. Giangrande P. Persi C. Bartolini A. Guarnieri A. Piccioni 《Space Science Reviews》1981,30(1-4):407-414
We present high and low dispersion UV spectra of HDE 245770, which is the optical counterpart of the recurrent transient X-ray pulsar A 0535+26,during a decay of an X-ray flare. UBV photometric measurements and medium dispersion optical spectra were simultaneously obtained.The energy distribution of the star in the 12 – 10 micron range is compared with the models of Kurucz and Poeckert and Marlborough.In this phase, HDE 245770 does not show evaluable variations with respect to the quiescent X-ray phase. 相似文献
18.
The technology of gallium arsenide field-effect transistors has advanced to the point where these devices can serve to replace traveling wave tubes in spaceborne communication transponders.This paper describes interim results of a C-band FET amplifier which is currently being developed by RCA for INTELSAT. The FETA is designed to provide a 6-W output with an efficiency greater than 25%, and a backed-off 1.5-W output level with low distortion and efficiency of 13%.The third order intermodulation () of a FETA at saturation is typically 15 dB as compared to 10 dB for a TWTA. At 10 dB input power back-off the improves to 24 dB while that of a TWTA is only 16 dB.We fabricated a breadboard 5-W FETA which demonstrates that a linear operation can be achieved at an output level of 1.5 W with 10% efficiency. By contrast the efficiency of a typical 5 W TWTA in the same linear region is no greater than 3–5%. 相似文献