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A model of the magnetosheath structure\udproposed in a recent paper from the authors is extended to estimate the\udmagnetopause stand-off distance from solar wind data. For this purpose, the\udrelationship of the magnetopause location to the magnetosheath and solar wind\udparameters is studied. It is shown that magnetopause erosion may be explained in\udterms of the magnetosheath magnetic field penetration into the magnetosphere.\udThe coefficient of penetration (the ratio of the magnetospheric magnetic field\uddepression to the intensity of the magnetosheath magnetic field Bm⊥z=–Bmsin2&#x0398;/2,\udis estimated and found approximately to equal 1. It is shown that having\udcombined a magnetosheath model presented in an earlier paper and the\udmagnetosheath field penetration model presented in this paper, it is possible to\udpredict the magnetopause stand-off distance from solar wind parameters. Key words. Magnetospheric physics · Magnetopause ·\udCusp and boundary layers-Magnetosheath</p

Magnetopause stand-off distance in dependence on the magnetosheath and solar wind parameters