On the Dependence of F2 Layer Critical Frequency on F10.7 Solar Flux at an Equatorial Station
暂无分享,去创建一个
[1] W. Wan,et al. Does the F10.7 index correctly describe solar EUV flux during the deep solar minimum of 2007-2009? , 2011 .
[2] I. Cnossen. Modelling of long-term trends in the middle and upper atmosphere , 2009 .
[3] P. Alken. A quiet time empirical model of equatorial vertical plasma drift in the Peruvian sector based on 150 km echoes , 2009 .
[4] Zhensen Wu,et al. A single-station spectral model of the monthly median foF2 over Chongqing, China , 2008 .
[5] R. Pektaş,et al. Examination of the solar cycle variation of foF2 for cycles 22 and 23 , 2008 .
[6] M. Goel,et al. Solar cycle variations of foF2 from IGY to 1990 , 2002 .
[7] Gary J. Rottman,et al. The SOLAR2000 empirical solar irradiance model and forecast tool , 2000 .
[8] P. Richards,et al. EUVAC: A solar EUV Flux Model for aeronomic calculations , 1994 .
[9] R. P. Kane. Sunspots, solar radio noise, solar EUV and ionospheric foF2. , 1992 .
[10] B. M. Reddy,et al. On the possible use of recent EUV data for ionospheric predictions , 1988 .
[11] L. M. Muggleton. Secular variation in F-region response to sunspot number , 1969 .
[12] M. rao,et al. The hysteresis variation in F2-layer parameters☆ , 1969 .
[13] R. Naismith,et al. Further evidence of a long term variation in the relationship of solar activity to the ionosphere , 1961 .
[14] R. Naismith,et al. A long term variation in the relationship of sunspot numbers to E-region character figures , 1961 .
[15] Dieter Bilitza,et al. International reference ionosphere , 1978 .