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Open AccessArticle10.11728/cjss2010.04.312

Observations of magnetic reconnection in the magnetotail associated with substorms

Yukinaga Miyashita-2010-01-01-Chinese Journal of Space Science

TL;DRAbstract

Magnetic reconnection is one of the most important, dynamic phenomena in the magnetotail in terms of magnetic field line configuration change and energy release. It is believed to occur in the distant magnetotail mainly during southward interplanetary magnetic field periods and in the near-Earth magnetotail in association with substorms. In the present paper, we discuss several important issues concerning magnetic reconnection in the magnetotail associated with substorms, such as reconnection signatures, location, timing, spatial scale, and behavior, from the macroscopic, observational point of view.

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Magnetic reconnection is one of the most important, dynamic phenomena in the magnetotail in terms of magnetic field line configuration change and energy release. It is believed to occur in the distant magnetotail mainly during southward interplanetary magnetic field periods and in the near-Earth magnetotail in association with substorms. In the present paper, we discuss several important issues concerning magnetic reconnection in the magnetotail associated with substorms, such as reconnection signatures, location, timing, spatial scale, and behavior, from the macroscopic, observational point of view.

Keywords

Magnetic reconnectionPhysicsSubstormInterplanetary magnetic fieldGeophysicsPlasma sheetMagnetic fieldMagnetosphere

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