Excitation of Magnetospheric Hydromagnetic Waves by Solar-Flare-Induced Change in Ionospheric Conductivity

T. J. Rosenberg, P. B. Morris, and L. J. Lanzerotti
Phys. Rev. Lett. 47, 1343 – Published 2 November 1981
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Abstract

Observations are reported of magnetospheric hydromagnetic (Alfvén) waves excited by rapid changes in ionospheric conductivity induced by solar flare x-ray and extreme-ultra-violet fluxes. The observed wave frequencies (∼0.01-0.02 Hz) are those expected for fundamental eigenoscillations of the geomagnetic field at middle latitudes. The measurements confirm a natural hydromagnetic wave generation mechanism not associated with the solar wind or geomagnetic storms. These results have implications for Alfvén wave generation in other cosmic plasmas.

  • Received 20 July 1981

DOI:https://doi.org/10.1103/PhysRevLett.47.1343

©1981 American Physical Society

Authors & Affiliations

T. J. Rosenberg and P. B. Morris

  • Institute for Physical Science and Technology, University of Maryland, College Park, Maryland 20742

L. J. Lanzerotti

  • Bell Laboratories, Murray Hill, New Jersey 07974

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Issue

Vol. 47, Iss. 18 — 2 November 1981

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