Direct contribution of oblique field-aligned currents to magnetic field variations on the ground

Attempt has been made to evaluate a direct contribution of the horizontal component of oblique field-aligned currents to surface magnetic variations in the auroral region associated with a localized electric potential distribution on the horizontal plane, in comparison with that of the ionospheric e...

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Bibliographic Details
Main Authors: Tsutomu Tamao, Haruyuki Taniguchi, Mitsuhiro Nambu, Akira Miura
Format: Report
Language:English
Published: Geophysics Research Laboratory, Faculty of Science, University of Tokyo/Geophysics Research Laboratory, Faculty of Science, University of Tokyo/College of General Education, Kyusyu University/Geophysics Research Laboratory, Faculty of Science, University of Tokyo 1985
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Online Access:https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=1766
http://id.nii.ac.jp/1291/00001766/
https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=1766&item_no=1&attribute_id=18&file_no=1
Description
Summary:Attempt has been made to evaluate a direct contribution of the horizontal component of oblique field-aligned currents to surface magnetic variations in the auroral region associated with a localized electric potential distribution on the horizontal plane, in comparison with that of the ionospheric eddy current. This direct effect is proportional to a product of two ratios, the Pedersen to Hall conductivities and the horizontal to vertical components of the local dipole magnetic intensity. In addition to these, the shorter the horizontal scale-length in the east-west direction compared with that in the north-south direction, the larger the direct effect of field-aligned currents. For the localized perturbation with an isotropic horizontal structure at 60° geomagnetic latitude, it attains to about 80% of the magnetic contribution of the Hall current at the earth's surface. It is also shown that only the vertical component of oblique field-aligned currents connects with the irrotational part of ionospheric currents, and that the effective conductance in the magnetosphere for three-dimensional current systems is reduced to a smaller value than that for the case of vertical field lines.