4. 地球磁気圏におけるプラズマフロー速度シア不安定の役割(<小特集>プラズマフロー速度シアの揺動・構造形成への効果)

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概要

• 論文の詳細を見る

• The plasma flow velocity shear instability, the so-called Kelvin-Helmholtz (K-H) instability has recently been recognized as an important process for the mass and energy transport of solar wind plasma into the earth magnetosphere. Even though this has been supported by many in-situ plasma observations, its physical mechanisms are still controversial. Recently, progress was made by a MHD simulation in which non-linear coupling with secondary instabilities results a turbulent and broad mixing layer. In the present paper, a new Sun-Earth connection model is proposed in which the K-H instability plays an important role.

• 社団法人プラズマ・核融合学会の論文
• 2004-04-25

著者

• 松本 洋介

  東京大学大学院

関連論文

• 4. 地球磁気圏におけるプラズマフロー速度シア不安定の役割(プラズマフロー速度シアの揺動・構造形成への効果)

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