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  • Magnetic clouds have been defined as special regions in the solar wind with higher magnetic field magnitude, lower proton temperature, and large rotation of the magnetic field vector. In some cases, the rotation exceeds 180° and it is interpreted as a signature that a magnetic cloud/flux rope is curved. It corresponds to common understanding that magnetic clouds are large interplanetary flux ropes, which have loop-like shapes in the heliosphere. In such cases, magnetic clouds are fitted by approximate linear force-free toroidal solutions (derived for large aspect ratios). Here an exact constant-alpha force-free toroidal solution is compared with approximate ones and it is found a reasonable agreement even for low aspect ratios.
  • Magnetic clouds have been defined as special regions in the solar wind with higher magnetic field magnitude, lower proton temperature, and large rotation of the magnetic field vector. In some cases, the rotation exceeds 180° and it is interpreted as a signature that a magnetic cloud/flux rope is curved. It corresponds to common understanding that magnetic clouds are large interplanetary flux ropes, which have loop-like shapes in the heliosphere. In such cases, magnetic clouds are fitted by approximate linear force-free toroidal solutions (derived for large aspect ratios). Here an exact constant-alpha force-free toroidal solution is compared with approximate ones and it is found a reasonable agreement even for low aspect ratios. (en)
Title
  • Magnetic Clouds Fitted by a Constant-Alpha Force-Free Toroidal Solution
  • Magnetic Clouds Fitted by a Constant-Alpha Force-Free Toroidal Solution (en)
skos:prefLabel
  • Magnetic Clouds Fitted by a Constant-Alpha Force-Free Toroidal Solution
  • Magnetic Clouds Fitted by a Constant-Alpha Force-Free Toroidal Solution (en)
skos:notation
  • RIV/67985815:_____/10:00355336!RIV15-GA0-67985815
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(1QS300120506), P(GA205/09/0170), P(ME09032), Z(AV0Z10030501)
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
  • 269156
http://linked.open...ai/riv/idVysledku
  • RIV/67985815:_____/10:00355336
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • interplanetary; magnetic fields; particle emission (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [ED02239D62D5]
http://linked.open...v/mistoKonaniAkce
  • Saint-Malo
http://linked.open...i/riv/mistoVydani
  • New York
http://linked.open...i/riv/nazevZdroje
  • Twelfth International Solar Wind Conference. Proceedings Paper
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...iv/tvurceVysledku
  • Vandas, Marek
  • Romashets, E. P.
http://linked.open...vavai/riv/typAkce
http://linked.open...ain/vavai/riv/wos
  • 000281438100095
http://linked.open.../riv/zahajeniAkce
http://linked.open...n/vavai/riv/zamer
issn
  • 0094-243X
number of pages
http://bibframe.org/vocab/doi
  • 10.1063/1.3395888
http://purl.org/ne...btex#hasPublisher
  • Melville
https://schema.org/isbn
  • 978-0-7354-0759-6
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