2011
DOI: 10.1029/2010rs004633
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Forecasting of low‐latitude storm‐time ionospheric foF2 using support vector machine

Abstract: .[1] An empirical model for predicting low-latitude storm-time ionospheric foF2 is developed using the support vector machine technique. Considering that the ionospheric disturbances are mainly caused by interplanetary disturbances, the solar wind data are introduced as model input, as well as the ionospheric observations of Haikou (HK, with geographic coordinates of 110.3°E and 20.0°N, and geomagnetic latitudes of 8.6°N) and Chongqing (CQ, 106.5°E, 29.6°N, and geomagnetic latitudes of 18.1°N) in China. Data f… Show more

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Cited by 26 publications
(14 citation statements)
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“…For instance, one can employ a time history of a given quantity, recorded with a certain time frequency. Examples of supervised regression in Space Weather are the forecast of a geomagnetic index, as function of solar wind parameters observed at L1 (Gleisner et al, ; Lundstedt & Wintoft, ; Macpherson et al, ; Uwamahoro & Habarulema, ; Valach et al, ; Weigel et al, ), the prediction of solar energetic particles (SEPs) (Fernandes, ; Gong et al, ; Li et al, ), of the F10.7 index for radio emissions (Ban et al, ; Huang et al, ), of ionospheric parameters (Chen et al, ), of sunspot numbers or, more in general, of the solar cycle (Ashmall & Moore, ; Calvo et al, ; Conway et al, ; Fessant et al, ; Lantos & Richard, ; Pesnell, ; Uwamahoro et al, ), of the arrival time of interplanetary shocks (Vandegriff et al, ), and of CMEs (Choi et al, ; Sudar et al, ).…”
Section: Machine Learning In Space Weathermentioning
confidence: 99%
“…For instance, one can employ a time history of a given quantity, recorded with a certain time frequency. Examples of supervised regression in Space Weather are the forecast of a geomagnetic index, as function of solar wind parameters observed at L1 (Gleisner et al, ; Lundstedt & Wintoft, ; Macpherson et al, ; Uwamahoro & Habarulema, ; Valach et al, ; Weigel et al, ), the prediction of solar energetic particles (SEPs) (Fernandes, ; Gong et al, ; Li et al, ), of the F10.7 index for radio emissions (Ban et al, ; Huang et al, ), of ionospheric parameters (Chen et al, ), of sunspot numbers or, more in general, of the solar cycle (Ashmall & Moore, ; Calvo et al, ; Conway et al, ; Fessant et al, ; Lantos & Richard, ; Pesnell, ; Uwamahoro et al, ), of the arrival time of interplanetary shocks (Vandegriff et al, ), and of CMEs (Choi et al, ; Sudar et al, ).…”
Section: Machine Learning In Space Weathermentioning
confidence: 99%
“…These very short-term predictions are generally referred to as nowcasts [34]. The most common ionospheric short-term fore-casting methods at present mainly include auto-correlation function method, multiple linear regression method, artificial neural network method, equivalent sunspot number method, Kalman filtering method, similar day method, storm time ionospheric forecasting method and so on [35][36][37]. Figure 3 shows a typical variation of LUF, MUF and FOT over a day.…”
Section: Hf Radio Propagation Prediction: Purposes and Approachesmentioning
confidence: 99%
“…Some literatures utilized the autoregression method, Muhtarov proposed a correlated autoregression ionospheric model driven by a synthetic geomagnetical index [16], Tsagouri presented an autoregression model for ionospheric short-term forecast based on the solar wind [17] [18], Tsagouri and Belehaki combined an autoregression forecasting algorithm with the empirical storm-time model [19]. In order to study the effects of the storm on the ionosphere, an empirical storm-time ionospheric correction model has been developed by Araujo Pradere [20] [21], and Ban introduced a forecasting model of low-latitude storm-time ionospheric f0F2 [22].…”
Section: Introductionmentioning
confidence: 99%