Full Wave Analysis of the Australian Omega Signal Observed by the Akebono Satellite (Special Issue on 1992 International Symposium on Antennas and Propagation)
スポンサーリンク
概要
- 論文の詳細を見る
The Akebono satellite observed the Australian Omega signals when it passed about 1000km over the Omega station. In this paper, we compare the observed Omega signal intensities with the values obtained using a full wave calculation and we discuss a mechanism of modulation of the signals. The relative spatial variations of the calculated Omega intensities are quite consistent with those observed, but the absolute calculated intensities themselves are several dB larger than the observed intensities. This difference in intensity may be due to the horizontal inhomogeneity of the D region, which is not modeled in the full wave calculation, or to an incorrect assumption about radiation characteristics of the Omega antenna. It is found that modulation of the observed signals is caused by the interference between the waves with different k vectors.
- 社団法人電子情報通信学会の論文
- 1993-12-25
著者
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YAGITANI Satoshi
Kanazawa University
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Rosen P
Jet Propulsion Lab. Ca Usa
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Kimura Iwane
Faculty of Engineering, Kyoto University
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Rosen P.
Jpl
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Yagitani S
Graduate School Of Natural Science & Technology Kanazawa University Kakuma-machi Kanazawa 920-11
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Yagitani Satoshi
Faculty Of Engineering Kanazawa University
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Kimura Iwane
Faculty Of Engineering Kyoto University
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Kimura Iwane
Faculty Of Technology Kyoto University
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Nagano Isamu
Kanazawa University Kakuma-machi Kanazawa 920-1192 Japan
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Nagano Isamu
Faculty Of Engineering Kanazawa University
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Rosen PaulA.
Jet Propulsion Laboratory
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Hata Minoru
Faculty of Technology, Kanazawa University
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Miyamura Kazutoshi
PFU
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Hata Minoru
Faculty Of Technology Kanazawa University
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Nagano I
Kanazawa University Kakuma-machi Kanazawa 920-1192 Japan.
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