Restoration of the meridional structure of geomagnetic pulsation fields from gradient measurements

Details Restoration of the meridional structure of geomagnetic pulsation fields from gradient measurements Restoration of the meridional structure of geomagnetic pulsation fields from gradient measurements

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989p%26ss...37..859b&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 37, July 1989, p. 859-864.

Physics

24

Geomagnetic Latitude, Geomagnetic Pulsations, Magnetohydrodynamic Waves, Earth Surface, Gradients, Magnetic Fields

Scientific paper

The usefulness of gradient measurements in the investigation of the resonance structure of geomagnetic pulsation fields along a meridian is extended. Starting with a simple resonance model and synchronous observations of Pc4 pulsations at five stations spaced about 100 km apart on a meridian, the gradient method is used to restore the structure of the pulsation field on a significant part of the meridian (about 1000 km) adjacent to the observation points.

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