Cusp Ion Composition as an Indicator of Non-Steady Reconnection

  1. James L. Burch,
  2. Robert L. Carovillano and
  3. Spiro K. Antiochos
  1. S. A. Fuselier and
  2. K. J. Trattner

Published Online: 19 MAR 2013

DOI: 10.1029/GM109p0161

Sun-Earth Plasma Connections

Sun-Earth Plasma Connections

How to Cite

Fuselier, S. A. and Trattner, K. J. (1999) Cusp Ion Composition as an Indicator of Non-Steady Reconnection, in Sun-Earth Plasma Connections (eds J. L. Burch, R. L. Carovillano and S. K. Antiochos), American Geophysical Union, Washington, D. C.. doi: 10.1029/GM109p0161

Author Information

  1. Lockheed Martin Advanced Technology Center

Publication History

  1. Published Online: 19 MAR 2013
  2. Published Print: 1 JAN 1999

ISBN Information

Print ISBN: 9780875900926

Online ISBN: 9781118664469

SEARCH

Keywords:

  • International Solar-Terrestrial Physics Program Congresses;
  • Sun Congresses;
  • Solar magnetic fields Congresses;
  • Space plasmas Congresses;
  • Magnetosphere Congresses;
  • Astrophysics Congresses

Summary

This chapter contains sections titled:

  • Introduction

  • Sample CUSP Encounter

  • Survey of Selected Southward IMF Events

  • Interpretation

  • Conclusions