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Ionospheric foF2 storm forecasting using neural networks
Institution:1. Swedish Institute of Space Physics, Solar-Terrestrial Physics Division, Lund, Sweden;2. CLRC Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, OX11 0QX, England;1. Departamento de Ingeniería de Procesos e Hidráulica, Universidad Autónoma Metropolitana-Iztapalapa, Apartado Postal 55-534, Iztapalapa, 09340 México, Mexico;2. Departamento de Ingeniería Eléctrica, Área de Ingeniería Biomédica. Universidad Autónoma Metropolitana-Iztapalapa, Apartado Postal 55-534, Iztapalapa, 09340 México, Mexico;3. Departamento de Biotecnología, Universidad Autónoma Metropolitana-Iztapalapa, Apartado Postal 55-534, Iztapalapa, 09340 México, Mexico;4. Departamento de Ingeniería Eléctrica, Área de Computación y Sistemas. Universidad Autónoma Metropolitana-Iztapalapa, Apartado Postal 55-534, Iztapalapa, 09340 México, Mexico;1. University of Saint Petersburg, Saint Petersburg, Russia;2. Arctic and Antarctic Research Institute, Saint Petersburg, Russia;1. Facultad de Educación, Universidad Adventista de Chile, Casilla 7-D, Chillán, Chile;2. Instituto Nacional de Pesquisas Espaciais, Divisao de Aeronomia, Avenida dos Astronautas, 1758, Jardim da Granja, São José dos Campos, SP CEP 12227-010, Brazil;3. Departamento de Geofísica, Universidad de Concepción, Casilla 160-C, Correo 3, Concepción, Chile
Abstract:The ionosphere shows a large degree of variability on time scales from hours to the solar cycle length. This variation is associated with magnetospheric storms, the Earth's rotation, the season, and the level of solar activity. To make accurate predictions of key ionospheric parameters all these variations must be considered. Neural networks, which are data driven non-linear models, are very useful for such tasks. In this work we examine if the F2 layer plasma frequency, foF2, at a single ionospheric station can be predicted 1 to 24 hours in advance by using information of past foF2 observations, magnetospheric activity, and time as inputs to neural networks. Particular attention has been paid to periods when great geomagnetic storms were in progress with the aim to develop a successful ionospheric storm forecasting tool.
Keywords:
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