Observations of bidirectional electrons in the distant tail lobes: GEOTAIL results

Research output: Contribution to journalArticleScientificpeer-review

Researchers

  • DN Baker
  • A. Nishida
  • T Mukai
  • T Yamamoto
  • Y Saito
  • Y Matsuno
  • S Kokubun
  • Tuija Pulkkinen

Research units

  • Institute of Space and Astronautical Science
  • Finnish Meteorological Institute
  • Nagoya University
  • University of Colorado Boulder

Abstract

ISEE-3 demonstrated the relatively frequent occurrence of low-energy (50 similar to 500 eV) electron flux enhancements within the distant magnetotail lobes. These electrons were found to be ''bidirectional'' in the sense that intensities were highest parallel (and antiparallel) to the lobe magnetic field lines. It was concluded that these electrons must enter the tail lobes along open field lines at the distant magnetopause and that this population would constitute the source for polar rain electrons at low altitudes in the polar cap regions. Similar plasma electron features have been found using the Low Energy Particle (LEP) sensor system onboard the GEOTAIL spacecraft. Remarkably close correspondences of low-energy (less than or similar to 2 keV) ion tailward flow enhancements are found to occur when bidirectional electron fluxes suddenly intensify. Such ion plasma measurements were not available with ISEE-3 and, thus, a new aspect of solar wind entry and overall plasma dynamics is revealed by these GEOTAIL measurements in the distant tail. Other ISTP data (e.g., IMP-8 and CANOPUS) are used to analyze selected periods.

Details

Original languageEnglish
Pages (from-to)959-962
Number of pages4
JournalGeophysical Research Letters
Volume24
Issue number8
Publication statusPublished - 15 Apr 1997
MoE publication typeA1 Journal article-refereed

ID: 3013635