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  • Solar energetic particle (SEP) modelling has gained great interest in the community, specifically in connection with the safety of crews and the protection of technological systems of spacecraft situated outside the shielding of Earth's magnetosphere. Two models for the prediction of SEP events are presented in this paper. The models are based on a linear filter and on a special type of dynamic artificial neural network known as the layer-recurrent neural network. In this work they use as input the following parameters: the X-ray flare class for flares originating close to the centre of the solar disk; observed type II or IV radio bursts; and of the position angle, width, and linear speed of observed full or partial halo CMEs.
  • Solar energetic particle (SEP) modelling has gained great interest in the community, specifically in connection with the safety of crews and the protection of technological systems of spacecraft situated outside the shielding of Earth's magnetosphere. Two models for the prediction of SEP events are presented in this paper. The models are based on a linear filter and on a special type of dynamic artificial neural network known as the layer-recurrent neural network. In this work they use as input the following parameters: the X-ray flare class for flares originating close to the centre of the solar disk; observed type II or IV radio bursts; and of the position angle, width, and linear speed of observed full or partial halo CMEs. (en)
Title
  • Predictions of SEP events by means of a linear filter and layer-recurrent neural network
  • Predictions of SEP events by means of a linear filter and layer-recurrent neural network (en)
skos:prefLabel
  • Predictions of SEP events by means of a linear filter and layer-recurrent neural network
  • Predictions of SEP events by means of a linear filter and layer-recurrent neural network (en)
skos:notation
  • RIV/67985530:_____/11:00365304!RIV12-AV0-67985530
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(IAA300120608), P(OC09070), Z(AV0Z30120515)
http://linked.open...iv/cisloPeriodika
  • 9-10
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 222749
http://linked.open...ai/riv/idVysledku
  • RIV/67985530:_____/11:00365304
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • coronal mass ejection; X-ray flare; solar energetic particles; artificial neural network (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • GB - Spojené království Velké Británie a Severního Irska
http://linked.open...ontrolniKodProRIV
  • [CEA9B8A444D5]
http://linked.open...i/riv/nazevZdroje
  • Acta Astronautica
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 69
http://linked.open...iv/tvurceVysledku
  • Hejda, Pavel
  • Bochníček, Josef
  • Revallo, M.
  • Valach, F.
http://linked.open...ain/vavai/riv/wos
  • 000295069600002
http://linked.open...n/vavai/riv/zamer
issn
  • 0094-5765
number of pages
http://bibframe.org/vocab/doi
  • 10.1016/j.actaastro.2011.06.003
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