The Role of Space-Time Dependent Ionospheric Conductivity in the Evolution of Field Line Resonances: Relation to Auroral Arc

  1. Shin-Ichi Ohtani,
  2. Ryoichi Fujii,
  3. Michael Hesse and
  4. Robert L. Lysak
  1. Manju Prakash1 and
  2. Robert Rankin2

Published Online: 18 MAR 2013

DOI: 10.1029/GM118p0165

Magnetospheric Current Systems

Magnetospheric Current Systems

How to Cite

Prakash, M. and Rankin, R. (2000) The Role of Space-Time Dependent Ionospheric Conductivity in the Evolution of Field Line Resonances: Relation to Auroral Arc, in Magnetospheric Current Systems (eds S.-I. Ohtani, R. Fujii, M. Hesse and R. L. Lysak), American Geophysical Union, Washington, D. C.. doi: 10.1029/GM118p0165

Author Information

  1. 1

    Department of Physics and Astronomy, SUNY at Stony Brook, New York

  2. 2

    Department of Physics, University of Alberta, Edmonton

Publication History

  1. Published Online: 18 MAR 2013
  2. Published Print: 1 JAN 2000

ISBN Information

Print ISBN: 9780875909769

Online ISBN: 9781118669006

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Keywords:

  • Magnetospheric currents—Congresses

Summary

  • Introduction

  • The Field Line Resonance Wave Model

  • The Role of Space-Time Dependent Conductivity On The Evolution of FLRs

  • Nonlinear Evolution of FLRs in the Presence of Inhomogeneous and Time-Dependent Conductivity

  • Summary and Conclusions