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Resource Detailed View


  • Responsible Thematic Node: Plasmas
  • Short Name: PMM
  • Brief description: Paraboloid Model of the magnetosphere
  • URL: http://www.magnetosphere.ru/iso/
  • Type: DATA/Modeling & Simulation
  • English Language: YES
  • Restricted access: NO
  • Longer description:
    The model has been developed in SINP for the study of terrestrial magnetosphere. Its modifications are now widely applied for the magnetosphere study of different magnetized planets. The name of model is derived from its key simplifying assumption that the magnetopause can be represented by a paraboloid surface co-axial with the planet-Sun line. The PMM calculates the magnetic field generated by a variety of current systems located on the boundaries and within the boundaries of a planetís magnetosphere under a wide range of environmental conditions, quiet and disturbed, affected by the solar-planetary interactions simulated by solar activity such as solar flares and related phenomena which induce planetary magnetic disturbances such as terrestrial magnetic storms.

  • Status (static or active ?):
    active

  • Associated bibliographic resource 1: exeev, I.I., 1978, Geomagnetizm & Aeronomy, 18, 447.
  • Associated bibliographic resource 2: Alexeev, I.I., 1986, J. Geomagn. Geoelectr., 38, 1199.
  • EPN location (lab or institute):

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  • Contributor: Topf
  • Last updater: Topf
  • Other Responsible (name): Igor Alexeev
  • Other Responsible (email): alexeev@dec1.sinp.msu.ru
  • Other Contact (name): Igor Alexeev
  • Other Contact (email): alexeev@dec1.sinp.msu.ru
  • This is a copy (not an original): NO
  • Keywords (9):

    Scientific themes (1):



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