Optimization of the neural-network geomagnetic model for forecasting large-amplitude substorm events
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[1] L. Lanzerotti. Geomagnetic induction effects in ground-based systems , 1983 .
[2] Tang,et al. Symbol sequence statistics in noisy chaotic signal reconstruction. , 1995, Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics.
[3] W. Horton,et al. A low‐dimensional energy‐conserving state space model for substorm dynamics , 1996 .
[4] Wendell Horton,et al. A Low-Dimensional Dynamical Model for the Solar Wind Driven Geotail-Ionosphere System , 1998 .
[5] R. Schunk,et al. Global ionosphere‐polar wind system during changing magnetic activity , 1997 .
[6] Konstantinos Papadopoulos,et al. Reconstruction of low‐dimensional magnetospheric dynamics by singular spectrum analysis , 1993 .
[7] P. Wintoft,et al. Prediction of geomagnetic storms from solar wind data with the use of a neural network , 1994 .
[8] Juan Alejandro Valdivia,et al. Spatiotemporal activity of magnetic storms , 1999 .
[9] Daniel N. Baker,et al. Magnetospheric Impulse Response for Many Levels of Geomagnetic Activity , 1985 .
[10] P. Palmadesso,et al. Plasma transport in the auroral return current region , 1987 .
[11] Daniel N. Baker,et al. A description of the solar wind-magnetosphere coupling based on nonlinear filters , 1995 .
[12] J. Takalo,et al. Correlation dimension and affinity of AE data and bicolored noise , 1993 .
[13] J. Timonen,et al. Properties of AE data and bicolored noise , 1994 .
[14] D. Prichard,et al. The non‐linear response of the magnetosphere: 30 October 1978 , 1993, comp-gas/9305003.
[15] J. Joselyn. Geomagnetic activity forecasting: The state of the art , 1995 .
[16] Patricia H. Reiff,et al. Effects of the March 1989 solar activity , 1989 .
[17] Geoffrey E. Hinton,et al. Learning representations by back-propagating errors , 1986, Nature.
[18] G. Ganguli,et al. Dispersive properties of a magnetized plasma with a field‐aligned drift and inhomogeneous transverse flow , 1996 .
[19] Toshiki Tajima,et al. Forecasting auroral electrojet activity from solar wind input with neural networks , 1999 .
[20] G. Ganguli,et al. Electrostatic oscillations due to filamentary structures in the magnetic-field-aligned flow: The ion-acoustic branch , 1999 .
[21] G. Ganguli,et al. Coupling of microprocesses and macroprocesses due to velocity shear: An application to the low-altitude ionosphere , 1994 .
[22] Charles F. Kennel,et al. Topside current instabilities , 1971 .
[23] R. A. Smith,et al. Prediction of geomagnetic activity , 1993 .
[24] J. Lyon,et al. Global numerical simulation of the growth phase and the expansion onset for a substorm observed by Viking , 1995 .
[25] V. Gavrishchaka,et al. Three‐dimensional simulations of the ionospheric plasma transport in the presence of the structured field‐aligned flows , 1999 .
[26] Daniel N. Baker,et al. Substorm recurrence during steady and variable solar wind driving: Evidence for a normal mode in the unloading dynamics of the magnetosphere , 1994 .
[27] H. Lundstedt,et al. Prediction of geomagnetic storms from solar wind data using Elman Recurrent Neural Networks , 1996 .
[28] W. Krueger,et al. Cross‐field transport due to low‐frequency oscillations in the auroral region: A three‐dimensional simulation , 1999 .
[29] Vadim M. Uritsky,et al. Low frequency 1/f-like fluctuations of the AE-index as a possible manifestation of self-organized criticality in the magnetosphere , 1998 .
[30] D. Baker,et al. Dst index prediction using data‐derived analogues of the magnetospheric dynamics , 1998 .
[31] José Carlos Príncipe,et al. The gamma model--A new neural model for temporal processing , 1992, Neural Networks.
[32] R. Schunk,et al. A three‐dimensional time‐dependent model of the polar wind , 1989 .
[33] Daniel N. Baker,et al. Indications of low dimensionality in magnetospheric dynamics , 1991 .
[34] G. Ganguli,et al. Kinetic theory for electrostatic waves due to transverse velocity shears , 1988 .
[35] H. Gleisner,et al. Response of the auroral electrojets to the solar wind modeled with neural networks , 1997 .
[36] C. Mobarry,et al. Topological structure of the magnetotail as a function of interplanetary magnetic field direction , 1995 .
[37] Tom Chang,et al. Self-organized criticality, multi-fractal spectra, sporadic localized reconnections and intermittent turbulence in the magnetotail , 1999 .
[38] Daniel N. Baker,et al. A nonlinear dynamical analogue model of geomagnetic activity , 1992 .
[39] P. Wintoft,et al. Neural network models predicting the magnetospheric response to the 1997 January Halo‐CME event , 1998 .
[40] K. Papadopoulos. A review of anomalous resistivity for the ionosphere , 1976 .
[41] J. Timonen,et al. Characteristic time scale of auroral electrojet data , 1994 .
[42] Konstantinos Papadopoulos,et al. Low-dimensional chaos in magnetospheric activity from AE time series , 1990 .
[43] H. Gleisner,et al. Predicting geomagnetic storms from solar-wind data using time-delay neural networks , 1996 .
[44] Daniel N. Baker,et al. The organized nonlinear dynamics of the magnetosphere , 1996 .
[45] Daniel N. Baker,et al. Satellite anomalies linked to electron increase in the magnetosphere , 1994 .
[46] Juan Alejandro Valdivia,et al. Prediction of magnetic storms by nonlinear models , 1996 .
[47] Tang,et al. Self-Organized Criticality: An Explanation of 1/f Noise , 2011 .
[48] Toshiki Tajima,et al. Neural net forecasting for geomagnetic activity , 1993 .
[49] C. Goertz,et al. Chaotic appearance of the AE index , 1991 .