GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS |
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Correlations between Strong Range Spread-F and GPS L-Band Scintillations Observed in Hainan in 2004 |
WANG Guo-Jun, SHI Jian-Kui, SHANG She-Ping, WANG Xiao |
State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100190 |
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Cite this article: |
WANG Guo-Jun, SHI Jian-Kui, SHANG She-Ping et al 2009 Chin. Phys. Lett. 26 019401 |
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Abstract Data from the DPS-4 digisonde and the GPS L-band ionospheric scintillation monitor are employed to study the correlations between strong range spread-F (SSF) and GPS L-band scintillations observed in the ionosphere over Hainan Island, China (19.5°N, 109.1°E geogr., dip lat. 9°N) in 2004. The SSF in the ionogram is different from the general range spread-F because it extends in frequency well beyond FoF2 and makes FoF2 difficult to be determined. The observations show that the SSF phenomenon is frequently accompanied by the occurrence of GPS L-band scintillations. The SSF and GPS L-band scintillations occur frequently in the equinoctial months (March, April, September, and October), but rarely in the winter (January, February, November, and December) and summer (May-August); especially, occurrence variations of the SSF and GPS L-band scintillations nearly have a same trend. The SSF and scintillations may be associated with the occurrence of topside plasma bubbles and could be explained by the generalized Rayleigh-Taylor instability.
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Keywords:
94.20.Vv
98.58.Ay
94.20.-y
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Received: 04 August 2008
Published: 24 December 2008
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PACS: |
94.20.Vv
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(Ionospheric disturbances, irregularities, and storms)
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98.58.Ay
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(Physical properties (abundances, electron density, magnetic fields, scintillation, scattering, kinematics, dynamics, turbulence, etc.))
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94.20.-y
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(Physics of the ionosphere)
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[1] Booker H G and Wells H W 1938 Terr. Magn. Atmos.Electron. 43 249 [2] Fejer B G and Kelley M C 1980 Rev. Geophys. SpacePhys. 18 401 [3] Basu Su and Basu S 1985 J. Atmos. Terrest. Phys. 47 753 [4] Mathews J D et al 2001 Geophys. Res. Lett. 284167 [5] Aarons J 1993 Space Sci. Rev. 63 209 [6] Abdu M A et al 1983 J. Geophys. Res. 88 9197 [7] Abdu M A, Medeiros R T and Nakamura Y 1983b J.Ceophys. Res. 88 4861 [8] Kil H and Heelis R A 1998 J. Geophys. Res. 103407 [9] Wang G J et al 2008 Adv. Space Res. 41 639 [10] de Medeiros R T et al 1983 J. Geophys. Res. 88 6253 [11] Rastogi R G et al 1989 Ann. Geophys. 7 281 [12] Iyer K N et al 2003 Adv. Space Res. 31 735 [13] Beach T L and Kintner P M 2001 IEEE Trans. Geosci.Remote Sens. 39 918 [14] Piggott W R and K Rawer 1972 URSI Handbook ofIonogram Interpretation and Reduction, Rep. UAG-23A, Boulder, COpp 68-73 [15] Sales G S et al 1996 J. Geophys. Res. 10126819 [16] Kil H et al 2002 Radio Sci. 37 1006 [17] Thomas R M et al 2001 Radio Sci. 36 1545 [18] Whalen J A 1997 Radio Sci. 32 1559 [19] Kelley M C 1989 The Earth's Ionosphere(San Diego,CA: Academic) p 121 |
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