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AGU: Geophysical Research Letters

 

Keywords

  • geomagnetic
  • ionosphere
  • Meteor Ridge

Index Terms

  • Ionosphere: Electric fields
  • Ionosphere: Ionospheric disturbances
  • Ionosphere: Ionospheric dynamics
  • Ionosphere: Ionospheric irregularities
  • Ionosphere: Meteor-trail physics

Abstract

GEOPHYSICAL RESEARCH LETTERS, VOL. 33, L24105, 5 PP., 2006
doi:10.1029/2006GL028267

Meteor induced ridge and trough formation and the structuring of the nighttime E-region ionosphere

Meers M. Oppenheim

Center for Space Physics, Boston University, Boston, Massachusetts, USA

Yakov Dimant

Center for Space Physics, Boston University, Boston, Massachusetts, USA

When meteor-generated plasma trails diffuse into the ionosphere they create large ambipolar electric fields mainly perpendicular to the Earth's geomagnetic field (B) and extending many kilometers from the trail along B. These fields will cause ionospheric plasma to collect into ridges extending from the trail along B, enhancing the density by as much as a factor of 2, and they will also remove up to 90% of the plasma on each side of the ridge. We predict that meteor-induced density perturbations may fill as much as 20% of the ionosphere between 95 and 120 km altitude. This paper presents simulations and theory to show how meteors produce plasma ridges and troughs. We estimate the extent of these as a function of altitude and meteor density. This process may explain observations of extensive nighttime E-region density structures made by rockets and radars.

Received 22 September 2006; accepted 21 November 2006; published 28 December 2006.

Citation: Oppenheim, M. M., and Y. Dimant (2006), Meteor induced ridge and trough formation and the structuring of the nighttime E-region ionosphere, Geophys. Res. Lett., 33, L24105, doi:10.1029/2006GL028267.

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