A prediction model of foF2 over periods of severe geomagnetic activity

被引:13
作者
Perrone, L. [1 ]
Pietrella, M. [1 ]
Zolesi, B. [1 ]
机构
[1] Ist Nazl Geofis & Vulcanol, I-00143 Rome, Italy
关键词
ionosphere; ionospheric storms; F2; layer; prediction model; geomagnetic index;
D O I
10.1016/j.asr.2006.08.008
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
A prediction procedure of the hourly values of the critical frequency of the F2 ionospheric layer, foF2, based on the geomagnetic index, is presented. The geomagnetic index used in this study is the time-weighted accumulation magnetic index ap(tau) based on the recent past history of the planetary index ap. The procedure is based on an empirical relationship between the ratio log(NmF2(t)/NmF2M(t)) and ap(tau), where NmF2(t) is the hourly maximum electron density at the F2 peak layer and NmF2M(t) is its 'quiet' value. The prediction of foF2 has been calculated during periods of severe magnetic activity in the current solar cycle 23 using data processed at the Rome ionospheric observatory. The performance of the model, during negative ionospheric storms, can be considered satisfactory, given that the root mean square (r.m.s.), calculated between measured and forecasted foF2, ranged between 0.74-2.0 MHz. (c) 2006 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:674 / 680
页数:7
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