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The top documents tagged [northward imf]
Madeline Hubbard (Keene High School) Matthew Shindel (Stanwich High School) Advisors: Fathima Muzamil, Dr. Charles Farrugia, Dr. Roy Torbert Objective:
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Kinetic properties of magnetic reconnection induced by the MHD-scale Kelvin-Helmholtz vortex: particle simulations 中村 琢磨 (T.K.M. Nakamura) Collaboraters:
218 views
Normal text - click to edit 1 August 2011 Auroral asymmetries in the conjugate hemispheres (and where KuaFu B can do better……) Nikolai Østgaard University
212 views
Auroral Boundaries Model Validation – What has been done
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ESS 200C Lecture 18. An isolated substorm is caused by a brief (30-60 min) pulse of southward IMF. Magnetospheric storms are large, prolonged disturbances
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Ørsted Results 5 Years in Space Geomagnetic Models, Publications and Conference Presentations Ørsted Initial Field Model (OIFM) Degree/order of main field
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Ørsted Results 5 Years in Space Geomagnetic Models, Publications and Conference Presentations
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Lecture 3 Introduction to Magnetic Storms. An isolated substorm is caused by a brief (30-60 min) pulse of southward IMF. Magnetospheric storms are large,
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Cluster observations of a reconnection site at high- latitude magnetopause Y. Khotyaintsev (1), A. Vaivads (1), Y. Ogawa (1,2), M. André(1), S. Buchert(1),
217 views
THEMIS Dayside
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Chelpanov M. A., Zolotukhina N.A. Institute of Solar-Terrestrial Physics, Irkutsk, Russia
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1. Introduction
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