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831.
Korpela E. Forsten J. Hamalainen A. Ruoskanen J. Eskelinen P. 《Aerospace and Electronic Systems Magazine, IEEE》2005,20(11):19-22
A field programmable gate array-based computing platform for high-speed sensors such as short-range radars is presented. The circuit performs necessary A/D conversions, raw data stream compression and target detection, and constructs a message structure suitable for external displays. In the prototype, USB is the connecting path to a laptop computer. An elementary pulse radar is utilized as an application example. An application interest would be in collision avoidance systems. Observed data transfer rates with real radar input signals were 36 Mbytes/s when typical target detection algorithms were applied. 相似文献
832.
P Coll D Coscia M C Gazeau E de Vanssay J C Guillemin F Raulin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1995,16(2):93-103
Many experiments have already been carried out to simulate organic chemistry on Titan, the largest satellite of Saturn. They can provide fruitful information on the nature of minor organic constituents likely to be present in Titan's atmosphere, both in gas and aerosol phases. Indeed, all the organic compounds but one already detected in Titan's atmosphere have been identified in simulation experiments. The exception, C4N2, as well as other compounds expected in Titan from theoretical modeling, such as other N-organics, and polyynes, first of all C6H2, have never been detected in experimental simulation thus far. All these compounds are thermally unstable, and the temperature conditions used during the simulation experiments were not appropriate. We have recently started a new program of simulation experiments with temperature conditions close to that of Titan's environment. It also uses dedicated analytical techniques and procedures compatible with the analysis of organics only stable at low temperatures, as well solid products of low stability in the presence of O2 and H2O. Spark discharge of N2-CH4 gas mixtures was carried out at low temperature in the range 100-150 K. Products were analysed by FTIR, GC and GC-MS techniques. GC-peaks were identified by their mass spectrum, and, in most cases, by comparison of the retention time and mass spectrum with standard ones. We report here the first detection in Titan simulation experiments of C6H2 and HC5N. Their abundance is a few percent relative to C4H2 and HC3N, respectively. Preliminary data on the solid products indicate an elemental composition corresponding to (H11C11N)n. These results open new prospects in the modeling of Titan's haze making. 相似文献
833.
F.W. Taylor J.T. Schofield P.J. Valdes 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1985,5(9):5-23
The definitive data set for the mean thermal structure of the Venusian middle atmosphere is published for the first time. Some recent interim results on a modelling study to interpret the measured thermal field in terms of the global dynamics are also presented. These indicate that (a) the zonal winds on Venus fall to very low values above about 90 km, (b) there is a strong mid-latitude jet which circles the planet approximately every two days, (c) the observed solar tides are dominated by the semi-diurnal component, in agreement with theory. 相似文献
834.
Parsons P. Glendinning A. Angelidis D. 《Aerospace and Electronic Systems Magazine, IEEE》1992,7(7):45-48
A resonant-element transducer developed for aerospace applications using micromachined silicon technology is described. The sensor is a beam supported over a square diaphragm. The resonant frequency of the beam is proportional to the applied pressure on the diaphragm. Results presented show that the prototype's performance rivals that of current high-accuracy pressure transducers 相似文献
835.
L J DeLucas C D Smith D C Carter P Twigg X M He R S Snyder P C Weber J V Schloss H M Einspahr L L Clancy A McPherson S Koszelak M M Vandonselaar L Prasad J W Quail L T Delbaere C E Bugg 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1992,12(1):393-400
The first microgravity protein crystal growth experiments were performed on Spacelab I by Littke and John. These experiments indicated that the space grown crystals, which were obtained using a liquid-liquid diffusion system, were larger than crystals obtained by the same experimental system on earth. Subsequent experiments were performed by other investigators on a series of space shuttle missions from 1985 through 1990. The results from two of these shuttle flights (STS-26 and STS-29) have been described previously. The results from these missions indicated that the microgravity grown crystals for a number of different proteins were larger, displayed more uniform morphologies, and yielded diffraction data to significantly higher resolutions than the best crystals of these proteins grown on earth. This paper presents the results obtained from shuttle flight STS-32 (flown in January, 1990) and preliminary results from the most recent shuttle flight, STS-31 (flown in April, 1990). 相似文献
836.
Ramesh P. Singh 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,4(11):97-101
The importance of the dielectric properties of earth, ocean and snow surfaces in microwave remote sensing is reviewed. Data on dielectric properties of materials in the microwave frequency range are very scarce and their behaviour is not fully understood. In this paper the need for dielectric properties of ocean and snow surfaces, the earth's surface and subsurface materials is discussed for the quantitative and qualitative interpretation of microwave remote sensing data of developing countries. 相似文献
837.
P E Villeneuve E H Dunlop 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1992,12(5):237-245
The evolution of a phase-separated gravity-independent bioreactor is described. The initial prototype, a zero head-space manifold silicone membrane based reactor, maintained large diffusional resistances. Obtaining oxygen transfer rates needed to support carbon-recycling aerobic microbes is impossible if large resistances are maintained. Next generation designs (Mark I and II) mimic heat exchanger design to promote turbulence at the tubing-liquid interface, thereby reducing liquid and gas side diffusional resistances. While oxygen transfer rates increased by a factor of ten, liquid channeling prevented further increases. To overcome these problems, a Mark III reactor was developed which maintains inverted phases, i.e., media flows inside the silicone tubing, oxygen gas is applied external to the tubing. This enhances design through changes in gas side driving force concentration and liquid side turbulence levels. Combining an applied external pressure of four atmospheres with increased Reynolds numbers resulted in oxygen transfer intensities of 232 mmol O2/l/h (1000 times greater than first prototype and comparable to a conventional fermenter). A 1.0 liter Mark III reactor can potentially deliver oxygen supplies necessary to support cell cultures needed to recycle a 10 astronaut carbon load continuously. 相似文献
838.
P E Villeneuve K S Wenger B G Thompson T Kedar E H Dunlop 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1994,14(11):75-78
The gas exchange portion of a phase-separated loop bioreactor was tested with respect to oxygen mass transfer and micromixing in accelerations of 0.01g, 1g, and 2g. A plot of the overall mass transfer coefficient versus gravity indicates the rate of oxygen transfer does not change as a function of acceleration. Also, it was determined that the micromixing did not exhibit significant changes in the various gravitational fields. These observations indicate the loop bioreactor should function independent of acceleration. 相似文献
839.
K.B. Serafimov I.S. Kutiev Ts.P. Dachev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1985,5(10):33-36
With data of satellite INTERCOSMOS-BULGARIA-1300 northern and corresponding southern hemisphere plasma densities have been compared. Southern densities are greater in the ?90 to ?180 and +30 to +120° ranges. The opposite is true for ?60 to +30°. No asymmetry has been observed during daytime. These results are explained by the variations of the magnetic declination. 相似文献
840.
Sahraoui A.E.K. Romdhani M. Jeffroy A. Dechazelles P. 《Aerospace and Electronic Systems Magazine, IEEE》1996,11(5):33-38
This paper presents a new approach in the development of avionics at AEROSPATIALE. The approach is based on a selective use of specification languages. Its aim is to compose partial avionics specifications in a unified format which is used for later concurrent hardware/software design steps. A demonstrator of the approach is currently in progress. It deals with the re-design of an avionics on-board system that belongs to the family of AIRBUS A340. The multi-languages specification is achieved through three graphical specification languages: Harel's StateCharts, SDL and SAO. The status of work and future perspectives are outlined 相似文献