Solar wind-magnetosphere coupling during an isolated substorm event
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Solar wind-magnetosphere coupling during an isolated substorm event a multispacecraft ISTP study

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Published by National Aeronautics and Space Administration, National Technical Information Service, distributor in [Washington, DC, Springfield, Va .
Written in English

Subjects:

  • Solar wind.,
  • Earth magnetosphere.,
  • Magnetic storms.,
  • Interplanetary magnetic fields.,
  • Satellite imagery.

Book details:

Edition Notes

Other titlesSolar wind magnetosphere coupling during an isolated substorm event., Multispacecraft ISTP study.
StatementT.I. Pulkkinen ... [et al.].
Series[NASA contractor report] -- NASA-CR-205242., NASA contractor report -- NASA CR-205242.
ContributionsPulkkinen, T. I., United States. National Aeronautics and Space Administration.
The Physical Object
FormatMicroform
Pagination1 v.
ID Numbers
Open LibraryOL15495025M

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Solar wind—magnetosphere coupling: A review of recent results. Fig. 3a and b shows the energy input through the magnetopause and ionospheric dissipation in a simulation run of a substorm event (Pulkkinen et al., ). Energy transfer during a substorm on Aug 15, Cited by: Coupling between the solar wind and the magnetosphere: CDAW 6 Energy budget during an isolated substorm using measurements of multi satellites and geomagnetic indices, Astrophysics Edward J. Smith, Frances Tang and Syun‐I. Akasofu, Solar wind‐magnetosphere coupling during intense magnetic storms ( ‐), Journal. Feb 01,  · Also of interest to this topic is the review of Milan which describes our present understanding of solar wind–magnetosphere–ionosphere coupling, that is the dynamics of the magnetosphere in response to solar wind driving, which in turn are responsible for many of the current systems within the academyrealtor.com by: Sep 19,  · Lecture: Solar Wind - Magnetosphere Coupling Dr. Brian Walsh - NASA Goddard Space Flight Center. Dr. Ed Dowdye: Solar Gravitation and Solar Plasma Wave Propagation Interaction.

(). Solar wind-magnetosphere coupling during an isolated substorm event: A multispacecraft ISTP study. Geophysical Research Letters, 24(8), doi: /97GL This Article is brought to you for free and open access by the Physics and Astronomy Department at Digital Commons @ Trinity. Ground signatures indicative of substorm activity were also observed by the THEMIS ground-based observatories during this interval. Prior to the substorm, none of the solar-wind monitoring missions (Geotail, OMNI, ACE) observed a significant southward Bz which could have initiated the academyrealtor.com: Miles Thomas Bengtson. Magnetospheric substorms represent a global interaction between the solar wind, the magetosphere, and the ionosphere. This article gives an overview of the solar wind - magnetosphere- ionosphere coupling processes with emphasis on the nonlinear particle dynamics in the academyrealtor.com by: Two Major Processes of The Solar Wind-Magnetosphere-Ionosphere Coupling is found to be significant during substorm expansion phases. event on 18 April and an isolated substorm .

Observations of the solar wind-magnetosphere-ionosphere coupling Abstract In this thesis, the solar wind-magnetosphere-ionosphere coupling is studied observationally, with the main focus on the ionospheric currents in the auroral region. The thesis consists of five research articles and an introductory part that summa-. to the output from the Solar Wind Magnetosphere-Ionosphere System (WINDMI) model through the ring candidate input solar wind-magnetosphere coupling func-tions in section 3. The December storm and substorm event is discussed in more detail in section 4. In section 5 discussions and future model uses and enhance-. Solar-wind–magnetosphere coupling, including relativistic electron energization, during high-speed streams is the type expected for wave excitation that is associated with the electrons transported by the enhanced convection during the substorm growth phase; 2. A.J. SmithSolar wind–magnetosphere coupling leading to relativistic Cited by: We discuss the energy input from the solar wind and its dissipation in the nightside ionosphere, as a form of Joule heating, during both isolated and storm-time substorms.