Diffusive penetration of the IMF B(y) into the magnetosphere

Physics

Scientific paper

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Earth Magnetosphere, Interplanetary Magnetic Fields, Magnetic Field Reconnection, Solar Wind, Electric Fields, Geomagnetism

Scientific paper

A mechanism of the observed IMF B(y) penetration into the magnetosphere is discussed. It is argued that diffusion of the IMF through the magnetopause prevails when the IMF is sufficiently weak. The diffusive penetration coefficient defined as the ratio between the internal B(y) penetration and the IMF B(y) is estimated to be of order R(m) exp -1/4, where R(m) is the magnetic Reynolds number. A model is developed to describe quantitatively a magnetic field in the outer solar wind flow (within the diffusive magnetopause) and the IMF-related magnetic field in the magnetosphere. The calculated values of the diffusive penetration coefficient are consistent with the observational data. Some difference in the results is mainly due to the electric currents inside the magnetosphere which are caused by the penetration of the solar wind electric field into the magnetosphere along the open field lines. The further improvement of the model implies the incorporation of this current system.

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