Chaotic collisionless reconnection in Jupiter's nightside magnetosphere

Details Chaotic collisionless reconnection in Jupiter's nightside magnetosphere Chaotic collisionless reconnection in Jupiter's nightside magnetosphere

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ncimc..15..645z&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 15 C, no. 5, p. 645-655.

Computer Science

Chaos, Jupiter Atmosphere, Magnetic Field Reconnection, Neutral Sheets, Planetary Magnetospheres, Charged Particles, Larmor Radius, Night

Scientific paper

The Buechner and Zelenyi theory is applied to Jupiter's magnetosphere. The instability parameters of this theory are computed by using a magnetic-field model, and the chaotic collisionless reconnection is shown to be possible. The results obtained are compared with the available experimental data, and possible consequences of the collisionless reconnection on the dynamics of Jupiter's magnetotail are discussed.

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