يعرض 1 - 9 نتائج من 9 نتيجة بحث عن '"Single station model"', وقت الاستعلام: 0.43s تنقيح النتائج
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    Academic Journal
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    Academic Journal
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    Academic Journal

    المؤلفون: Xu, T., Wu, Z., Wu, J., Wei, G., Feng, J.

    المساهمون: Xu, T., School of Science, Xidian University, Xi’an, China, Wu, Z., Wu, J., National Key Laboratory of Electromagnetic Environment, China Research Institute of Radiowave Propagation, Beijing, China, Wei, G., School of Science, Southwest Petroleum University, Chengdu, China, Feng, J., China Research Institute of Radiowave Propagation, Qingdao, China

    Relation: Annals of Geophysics; 4/51 (2008); APOSTOLOV, E., L. ALBERCA and D. PANCHEVA (1994): Longterm prediction of the foF2 on the rising and falling parts of the solar cycle, Adv. Space. Res. 14, 47-50. BALAN, N., G.J. BAILEY, B. JENKINS, P.B. RAO and R.J. MOFFETT (1994): Variations of ionospheric ionization and related solar fluxes during an intense solar cycle, J. Geophys. Res., 99, 2243-2253. BILITZA, D. (2000): The importance of EUV indices for the International Reference Ionosphphere, Phys. Chem. Earth., 25, 515-521. BILITZA, D. (2001): International reference ionosphere 2000, Radio Sci., 36, 261-275. BILITZA, D. (2002): Ionospheric models for radiao propagation studies, in the review of Radio Science 1999-2002 edited by W. R. STONE, IEEE Press, 625-679. CARUANA, J. (1990): The IPS monthly T-index, Proc. of the solar-Terrestrial Prediction Workshop, Leura, Australia, 2, 257-263. DE FRANCESCHI G. and A. DESANTIS (1994): PASHA: regional long term predictions ionospheric parameters by ACHA, Ann. Geophysics, 37, 209-220. DOMINICI, P. and B. ZOLESI (1987): A model for the normal ionosphere over Rome, II Nuovo Cimento, 10C, 191- 208. DICK, M. and P. BRADLEY (1992): The RAL multi-quasiparabolic model ionosphere, Porc. of PRIME Workshop, Roquetes, Memoria, 16, 67-83. FORBES, J. M., S. E. PALO and X.L. ZHANG (2000): Variability of the ionosphere, J. Atmos. Terr. Phys., 62, 685- 693. HOLT, J. M., S. R. ZHANG and M. J. BUONSANTO (2002): Regional and local ionospheric models based on Millstone Hill incoherent scatter radar data, Geophys. Res. Lett. 29, 1027. HUANG, Y.N. (1963): The hysteresis variation of the semithickness of the F2-layer and its relevant phenomena at Kokubunji, Japan, J. Atmos. Terr. Phys., 25, 647-658. KANE, R.P. (1992): Solar cycle variation of foF2, J. Atmos. Terr. Phys., 54, 1201-1205. KOURIS, S.S., Th.D. XENOS, and S. GOUTZAMANIS (1993): Proposals for the solar-cycle variations of foF2, Porc. of PRIME Workshop, Graz. Wissenschaftlucher Bericht, 2, 79-88. KOURIS, S.S. and J.K. NISSOPOULOS (1994): Variation of foF2 with solar activity, Adv. Space Res., 14, 163-166. KOURIS, S.S., P.A. BRADLEY and P. DOMINICI (1998): Solarcycle variation of the daily foF2 and M(3000)F2, Ann. Geophysicae, 16, 1093-1042. LIU, J. Y., Y. I. CHEN and J. S. LIN (2003): Statistical investigation of the saturation effect in the ionospheric foF2 versus sunspot, solar radio noise, and solar EUV radiation, J. Geophys. Res., 108, 1067-1073. LIU, L.B., W.X. WAN and B.Q. NING (2004): Statistical modeling of ionospheric foF2 over Wuhan, Radio Sci., 39, 2013. LIU, R., P. SMITH and J. KING (1983): A new solar index to improve foF2 prediction using the CCIR, Altas. Telecomm. J. 50, 408-413. MIKHAILOV, A. and V. MIKHAILOV (1995): A new ionospheric index MF2, Adv. Space. Res., 15, 93-97. MORAITIS, G., Z. KECIC and L. CANDER (1991): Ionospheric modeling at single stations, Porc. of PRIME Workshop, Rome, 154-160. PANCHEVA, D. and P. MUKHTAROV (1996): A single-station spectral model of the monthly median F-region critical frequency, Ann. Geophysics, 39, 807-818. PANCHEVA, D. and P. MUKHTAROV (1998): A single-station spectral model of the monthly median foF2 and M(3000) F2, Studia geoph. et geod., 42, 183-196. RAO, M.S. and R.S. RAO (1969): The hysteresis variation in F2 layer parameters, J. Atmos. Terr. Phys., 31, 1119- 1125. RICHARDS, P.G. (2001): Seasonal and solar cycle variations of the ionospheric peak electron density: Comparison of measurement and models, J. Geophys. Res., 106, 12803-12819. SETHI, N.K., M.K. GOEL and K. K. MAHAJAN (2002): Solar cycle variations of foF2 from IGY to 1990, Ann. Geophysicae, 20, 1677-1685. SIZUN, H. (1991): foF2 variation with R12 solar index, Proc. of PRIME Workshop, Rome, 87-91. SIZUN, H. (1992): F2-layer critical frequency modelization as a function of upward and downward phase of solar activity cycle, Proc. of PRIME/URSI Workshop, Roquetes, Memoria, 16, 205-217. SOLÉ, J.G. (1988): Relations between hourly monthly median values of foF2 and some geophysical indices. Their application to an ionospheric single station model, Acta Geophys. Polonica, 17, 77-88. XENOS, Th.D., S.S. KOURIS and B. ZOLESI (1996): Assessment of the solar–cycle dependence of foF2, Ann. Geophysics, 6, 1157-1166. ZHANG, M.L., J.K. SHI, X. WANG and M. RADICELLA (2004): Ionospheric variability at low latitude station: Hainan, China, Adv. Space. Res., 34, 1860-1868. ZOLESI, B., Lj.R. CANDER and G.D. FRANCESCHI (1993): Simplified ionospheic regional model for telecommunication application, Radio Sci., 28, 603-612. ZOLESI, B. and Lj.R. CANDER (2000): Evolution of the ionospheric mapping and modeling during the last four decades, Fisica de la Tierra, 12, 127-154.; http://hdl.handle.net/2122/4974

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    Academic Journal
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    Academic Journal
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    Academic Journal
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    Academic Journal

    المؤلفون: Stanislawska, I.

    المساهمون: Stanislawska, I., Space Research Centre, Polish Academy of Sciences, Warszawa, Poland

    وصف الملف: 1233760 bytes; application/pdf

    Relation: 2/37 (1994); http://hdl.handle.net/2122/1868

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