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Is the magnetosphere a lens for MHD waves?
Author(s) -
Papadopoulos K.,
Sharma A. S.,
Valdivia J. A.
Publication year - 1993
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/93gl03011
Subject(s) - magnetopause , magnetosphere , physics , magnetohydrodynamics , geophysics , substorm , solar wind , current sheet , ring current , computational physics , earth radius , magnetosphere of saturn , alfvén wave , magnetic field , quantum mechanics
A novel viewpoint of the magnetosphere as a lens for MHD waves is presented. Using a simple model of the variation of the Alfven speed as proportional to the local magnetic field value given by the Earth's dipole field and that due to the magnetopause currents represented by a current loop, it is found that the near‐Earth magnetotail, in the range 8–16 R E , is the focus of the magnetospheric lens. This location is found to be quite insensitive to a wide variation of parameters. By using simple diffraction theory analysis it is found that the focal region extends about 1 R E about the neutral sheet in the north‐south plane and 0.2–0.5 R E along the Sun‐Earth line. Compressive MHD waves carried by the solar wind or created by the interaction of the wind with the magnetopause can be amplified by a factor of about 100 in the focal region and this has potentially important implications to substorm activity.