2014
DOI: 10.1186/bf03352454
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Prediction of the Dst index from solar wind parameters by a neural network method

Abstract: Using the Elman-type neural network technique, operational models are constructed that predict the Dst index two hours in advance. The input data consist of real-time solar wind velocity, density, and magnetic field data obtained by the Advanced Composition Explorer (ACE) spacecraft since May 1998 (http://www2.crl.go.jp/uk/uk223/service/nnw/index.html). During the period from February to October 1998, eleven storms occurred with minimum Dst values below −80 nT. For ten of these storms the differences between t… Show more

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Cited by 27 publications
(14 citation statements)
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“…Yu et al (2006) proposed a chaos game representation of Dst index while Drezet et al (2002) presented a Kernel based technique. The most notable prediction is achieved by Artificial Neural Network method (Elman 1990;Kugblenu et al 1999;Lundstedt and Wintoft 1994;Lundstedt et al 2002;Pallocchia et al 2006a;Stepanova and Pérez 2000;Watanabe et al 2002;Wu and Lundstedt 1996). All these methods have their own advantages and disadvantages.…”
Section: Introductionmentioning
confidence: 97%
“…Yu et al (2006) proposed a chaos game representation of Dst index while Drezet et al (2002) presented a Kernel based technique. The most notable prediction is achieved by Artificial Neural Network method (Elman 1990;Kugblenu et al 1999;Lundstedt and Wintoft 1994;Lundstedt et al 2002;Pallocchia et al 2006a;Stepanova and Pérez 2000;Watanabe et al 2002;Wu and Lundstedt 1996). All these methods have their own advantages and disadvantages.…”
Section: Introductionmentioning
confidence: 97%
“…Other techniques for Dst-index predictions include the usage of neural networks, with delayed inputs, with feed-back connections (e.g., Lundstedt and Wintoft 1994;Lundstedt et al 2001;Watanabe et al 2002;Pallocchia et al 2006;Bala and Reiff 2012;Dolenko et al 2014;Lu et al 2016). Bala and Reiff (2012) use the solar wind-magnetosphere coupling function, the Boyle index (Boyle et al 1997), which is an empirical approximation for the polar cap potential dependent on solar wind parameters, as basis functions to train an artificial neural network to predict the Dst-index.…”
Section: Dst-index As a Storm Indicator Measure And Predictormentioning
confidence: 99%
“…Caswell () used B x , B y , and B z components of the IMF, solar wind proton density, solar wind plasma speed, and plasma flow pressure to predict the Dst index 1 hr in advance. Similarly, Watanabe et al () used the solar wind velocity, density, and IMF B x , B y , B z , and B t to predict the Dst index 2 hr in advance.…”
Section: Introductionmentioning
confidence: 99%