Madeline Hubbard (Keene High School) Matthew Shindel (Stanwich High School) Advisors: Fathima Muzamil, Dr. Charles Farrugia, Dr. Roy Torbert Objective:
Kinetic properties of magnetic reconnection induced by the MHD-scale Kelvin-Helmholtz vortex: particle simulations 中村 琢磨 (T.K.M. Nakamura) Collaboraters:
Normal text - click to edit 1 August 2011 Auroral asymmetries in the conjugate hemispheres (and where KuaFu B can do better……) Nikolai Østgaard University.
Auroral Boundaries Model Validation – What has been done.
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.
Ørsted Results 5 Years in Space Geomagnetic Models, Publications and Conference Presentations Ørsted Initial Field Model (OIFM) Degree/order of main field.
Ørsted Results 5 Years in Space Geomagnetic Models, Publications and Conference Presentations
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,
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),
THEMIS Dayside
Chelpanov M. A., Zolotukhina N.A. Institute of Solar-Terrestrial Physics, Irkutsk, Russia
1. Introduction
