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《中国航空学报》2022,35(9):35-48
In the past ten years, many high-quality datasets have been released to support the rapid development of deep learning in the fields of computer vision, voice, and natural language processing. Nowadays, deep learning has become a key research component of the Sixth-Generation wireless systems (6G) with numerous regulatory and defense applications. In order to facilitate the application of deep learning in radio signal recognition, in this work, a large-scale real-world radio signal dataset is created based on a special aeronautical monitoring system - Automatic Dependent Surveillance-Broadcast (ADS-B). This paper makes two main contributions. First, an automatic data collection and labeling system is designed to capture over-the-air ADS-B signals in the open and real-world scenario without human participation. Through data cleaning and sorting, a high-quality dataset of ADS-B signals is created for radio signal recognition. Second, we conduct an in-depth study on the performance of deep learning models using the new dataset, as well as comparison with a recognition benchmark using machine learning and deep learning methods. Finally, we conclude this paper with a discussion of open problems in this area. 相似文献
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A. N. Korzhavin V. M. Bogod V. N. Borovik G. B. Gelfreikh V. I. Makarov 《Space Science Reviews》1994,70(1-2):193-198
This paper presents a short summary of observations of coronal structures at microwaves using an instrument with high spatial resolution and good wavelength coverage. The comparison of the RATAN-600 data with optical observations of coronal loops in the green line and with the Very Large Array maps at 21 cm has shown that the loops represent only a small part of coronal matter, although their role may be of great importance in the physics of the solar corona. Prominence (filament) associated sources, especially peculiar ones, are also reviewed. 相似文献
125.
多数传电台信息传输的设计和实现 总被引:3,自引:0,他引:3
应用星形结构思想,提出了建立“一对多”数传电台信息传输的技术途径及实现方案,并开发出了具体的应用软件。提出的方法可应用于无通信基础情况下静止或低动态多目标间的信息交换,具有很大的实际应用价值。 相似文献
126.
M. Pandey A.P. Rao R. Manchanda P. Durouchoux C.H. Ishwara-Chandra 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2820-2823
We present the results of low frequency radio observations of the X-ray binaries, Cygnus X-1 and Cygnus X-3, during different X-ray states. The low frequency observations were made for the first time for these sources at 0.61 and 1.28 GHz using the Giant Meter-wave Radio Telescope (GMRT) between 2003 and 2004. Both Cyg X-1 and Cyg X-3 are highly variable at low radio frequencies. We also compare our data with the observations at 15 GHz conducted by the Ryle telescope. Spectral turnover is seen for both the sources below 2 GHz. The data suggest that the change in the radio flux density in both the sources is correlated to the X-ray hardness ratio and follows a similar behavior pattern. 相似文献
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G. J. Molina-Cuberos J. Porti B. P. Besser J. A. Morente J. Margineda H. I. M. Lichtenegger A. Salinas K. Schwingenschuh H. U. Eichelberger 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,33(12):2309-2313
Among the multiple questions that the CASSINI/HUYGENS mission tries to answer is the likelihood of electric discharges in Titan's atmosphere. The instruments “Huygens Atmospheric Structure Instrument” and “Radio and Plasma Wave Science” will probe the electromagnetic emissions during the Huygens descent and Cassini flybys, respectively. Although no lightning was observed during Voyager's encounters with Titan in 1980 and 1981, this does not exclude the existence of lightning phenomena. Recent investigations show that lightning discharges could occur in the lower atmosphere, such as the detection of methane condensation clouds in the troposphere and the theoretical prediction of an electric field that would be sufficient enough to cause lightning. We present a numerical model of Titan's atmosphere with the aim of calculating the resonance frequencies and the atmospheric transparency to electromagnetic waves. The detection and measurement of these resonances, Schumann frequencies, by the Huygens probe, would show the existence of electric activity connected with lightning discharges in the atmosphere. As it happens with the Schumann frequencies of Earth, losses associated with the electric conductivity will make these frequencies to be lower than the theoretically predicted, the fundamental one being located between 11 and 15 Hz. An analytical study shows that the strong losses associated with the high conductivity make it impossible that an electromagnetic wave generated near the surface with a frequency of 10 MHz or lower reaches the outer part of Titan's atmosphere. Therefore the detection of electromagnetic waves coming from Titan's lower atmosphere by the RPWS instrument is very unlikely. 相似文献
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基于多个不同权重与时延的doublet脉冲叠加,提出一种新的多带通超宽带( MB-UWB)信号光学产生与传输的方法。射频( RF)信号对光载波进行强度调制后,电高斯脉冲对光信号进行相位调制并利用标准单模光纤( SMF)进行传输。 SMF实现相位调制-强度调制( PM-IM)转换,产生doublet脉冲;实现多个doublet信号的时延差,产生叠加的UWB信号。通过调节RF信号源的频率可以实现UWB信号中心频率和带宽的改变;通过调节RF信号源的幅度可以实现边带抑制比的改变。仿真实现了边带抑制比大于25dB,中心频率5~8GHz,带宽2.9~3.8GHz的UWB的信号产生。 相似文献
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