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记者:请您介绍一下罗克韦尔·柯林斯公司在ARJ21-700项目中的参与情况。
丹尼·海格森:作为ARJ21-700项目的19家供应商之一,我们负责为ARJ21-700飞机提供一整套的航电设备,其中涵盖了通信、导航、飞控以及监视各个子系统。 相似文献
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Kenneth E.Gazzola Former Executive VP 《国际航空》2007,(9):56-57
20 years ago, in September 1987, an adventure began which was unique in aviation/aerospace publishing. That adventure led to a multimedia partnership which has grown stronger every year since 1987 and developed into a lasting friendship and global business alliance that continues today. 相似文献
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I.A. Nesterov V.E. Kunitsyn 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
We discuss the specific features of the spatiotemporal radio tomography of ionospheric electron density based on the data from high orbiting global navigational satellite system (GNSS). The main peculiarities are four-dimensionality of the problem and essential incompleteness of input data. The approach suggested for the solution of this problem is based on the search for the solution with minimal Sobolev’s norm (the most smooth solution), which provides, in particular, smooth extension of the solution to the area where no input data is available. Methods and algorithms for the solution of the problem are developed, and the resolution of the proposed technique is estimated. Examples of global and regional radio tomographic imaging based on GNSS data are presented. The obtained results are compared with the data of ionosondes and with the results of radio tomography based on the radio transmissions from low-orbiting satellites. 相似文献
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V. V. Akimov V. G. Afanassyev I. D. Blokhintsev N. G. Leikov V. E. Nesterov A. M. Galper Y. V. Ozerov V. A. Rugki V. M. Zemskov M. I. Fradkin N. P. Topchiev E. I. Chuiken E. Barouch I. Grenier M. Gros A. R.Bazer-Bachi J. -M. Lavigne J. -F. Olive A. Buczkowska J. Grygorczuk J. Juchniewicz P. McCulloch 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1993,13(12):657-664
Two observations of the Vela Pulsar in the energy range 50–5000 MeV performed with the GAMMA-1 telescope in 1990 and 1991 allowed us to study time variability of the pulsar light curve and energy spectra. The light curve for Eγ > 50 MeV shows definite variations in the first interpeak phase interval. The energy spectra of the two main peaks and first interpeak in the lightcurve vary significantly below 200 MeV. 相似文献
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The effect of a 20-day space flight on water, Na+, K+, Mg2+, Ca2+ and glycogen contents as well as on activities of glycogen metabolism enzymes--glycogen synthetase and glycogen phosphorylase--of rat skeletal muscles was studied. This data is regarded as an integral test characterizing the state of contractile tissue of the animals at the final stage of flight aboard biosatellites. The measurements indicate that there were no significant changes of cations and glycogen contents nor of the enzymic activities in fast-twitch muscles during the 20-day spaceflight. At the same time dehydration in these muscles was observed, which disappeared on the 25th postflight day. In slow-twitch antigravitational skeletal muscle (m. soleus) there was a decrease of K+ and increase of Na+ in the tissue contents. The changes disappeared at the end of the on-earth readaptation period. From the pattern of these observations, we can conclude that the 20-day space flight leads to some reversible biochemical changes of the rat skeletal muscles. A conclusion can be drawn about necessity of creating, aboard the spaceship, an artificial load on antigravitational skeletal muscles. 相似文献
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V. V. Akimov V. G. Afanassyev I. D. Blokhintsev L. F. Kalinkin N. G. Leikov V. E. Nesterov A. M. Galper Y. V. Ozerov V. A. Rudko M. F. Runtso V. M. Zemskov M. I. Fradkin L. V. Kurnosova M. A. Russakovitch N. P. Topchiev E. I. Chuikin V. Y. Tugaenko M. Gros A. R. Bazer-Bachi J. -M. Lavigne J. -F. Olive 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1993,13(12):739-742
The Geminga light curve obtained with the “Gamma-1” telescope features two peaks separated by 0.5 ± 0.03 period. The light curve is pronounced for γ-quanta energies higher than 400 MeV. The pulsed flux upper limit (1σ) in the energy interval 50 – 300 MeV is 6·10−7 cm−2sec−1. For energies >300 MeV the pulsed component power law spectrum has an exponent 1.1 −0.3+1.1 and an integral flux (1.1±0.3)·10−6 cm−2sec−1. 相似文献
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