Three-Dimensional MHD Simulation of Interplanetary Magnetic Field Changes at 1 AU Caused by a Simulated Solar Disturbance and a Tilted Heliospheric Current/plasma Sheet

Details Three-Dimensional MHD Simulation of Interplanetary Magnetic Field Changes at 1 AU Caused by a Simulated Solar Disturbance and a Tilted Heliospheric Current/plasma Sheet Three-Dimensional MHD Simulation of Interplanetary Magnetic Field Changes at 1 AU Caused by a Simulated Solar Disturbance and a Tilted Heliospheric Current/plasma Sheet

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997soph..173..391w&link_type=ejournal

Solar Physics, v. 173, Issue 2, p. 391-408.

Physics

10

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