Propagation of plasmoids generated by fast reconnection in the geomagnetic tail

Author:

Ugai M.

Funder

Grant-in-Aids

Ministry of Education in Japan

Mitsubishi Foundation, RISH of Kyoto University

Solar-Terrestrial Environment Laboratory of Nagoya University

Publisher

Elsevier BV

Subject

Space and Planetary Science,Atmospheric Science,Geophysics

Reference37 articles.

1. Geospace environmental modeling (GEM) magnetic reconnection challenge;Birn;Journal of Geophysical Research,2001

2. Substorm processes in the magnetotail;Hones;Journal of Geophysical Research,1977

3. Statistical analysis of the plasmoid evolution with Geotail observations;Ieda;Journal of Geophysical Research,1998

4. Experimental test of the Sweet-Parker model of magnetic reconnection;Ji;Physical Review Letters,1998

5. Potential plasma instabilities for substorm expansion onsets;Lui;Space Science Review,2004

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1. Magnetospheric Substorm Onset by Current Disruption Processes;Auroral Dynamics and Space Weather;2015-11-20

2. The Monge–Ampère trajectory correction for semi-Lagrangian schemes;Journal of Computational Physics;2014-10

3. Solar flares: radio and X-ray signatures of magnetic reconnection processes;Research in Astronomy and Astrophysics;2014-07

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