Total pressure variations in the magnetotail as a function of the position and the substorm magnitude

R. Yamaguchi, H. Kawano, S. Ohtani, S. Kokubun, K. Yumoto

研究成果: Contribution to journalArticle査読

11 被引用数 (Scopus)

抄録

The present study investigates the energy storage and release processes of substorms as a function of both position and substorm intensity in a model-independent manner. As an index of the substorm intensity, we use the amplitude of the positive bay observed at middle and low latitudes. As an index of the energy storage and release in the magnetotail, we use the total pressure measured by Geotail. We have performed a superposed epoch analysis of the total pressure for each substorm group binned in terms of the position and the substorm intensity. We have found that (1) both the magnitude and the increasing rate of the total pressure (i.e., energy density) in the near-tail region (-15 RE < XGSM < -6 RE and -8 RE < YGSM <8 RE) are highly correlated with the substorm intensity, while those in the midtail (-25 RE < X GSM < -15 RE and - 10 RE < Y GSM <10 RE) are not correlated with the substorm intensity. We have also found that (2) the start of the energy release of small substorms in the near-tail region tends to be delayed from the first Pi2 onset.

本文言語英語
ページ(範囲)A03206
ジャーナルJournal of Geophysical Research: Space Physics
109
A3
DOI
出版ステータス出版済み - 3 2004

All Science Journal Classification (ASJC) codes

  • Geophysics
  • Space and Planetary Science

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