Hydromagnetic gradient waves in the dynamo region of the ionosphere

Details Hydromagnetic gradient waves in the dynamo region of the ionosphere Hydromagnetic gradient waves in the dynamo region of the ionosphere

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sogru.123...69k&link_type=abstract

Akademiia Nauk Gruzinskoi SSR, Soobshcheniia (ISSN 0132-1447), vol. 123, July 1986, p. 69-71. In Russian.

Computer Science

1

Atmospheric Circulation, Geomagnetism, Ionospheric Disturbances, Magnetohydrodynamic Waves, Planetary Waves, Dynamo Theory, Hall Effect

Scientific paper

It is demonstrated that both 'fast' and 'slow' planetary-scale hydromagnetic gradient waves may exist in the dynamo region of the ionosphere due to the inhomogeneity of the geomagnetic field with latitude. Large changes (by almost an order of magnitude) in the phase velocities and period of the 'fast' waves for the daytime and the nighttime ionosphere and also the direct connection between the waves and perturbations of the geomagnetic field provide a way for the experimental detection of these waves through a simultaneous analysis of the variation of ionospheric parameters in the E layer and geomagnetic field components.

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