'Turbulent reconnection' presentation slideshows

Smithsonian Astrophysical Observatory, April 22, 2002

Coronal Heating due to low frequency wave-driven turbulence W H Matthaeus Bartol Research Institute, University of Delaware Collaborators: P. Dmitruk, L. Milano, D. Mullan, G. Zank and S Oughton. Smithsonian Astrophysical Observatory, April 22, 2002. Overview.

455 views • 34 slides

Alex Lazarian

3D Reconnection of Weakly Stochastic Magnetic Field and its Implications. Alex Lazarian. Astronomy Department and Center for Magnetic Self-Organization in Astrophysical and Laboratory Plasmas. Collaboration: Ethan Vishniac, Grzegorz Kowal and Otminowska-Mazur.

451 views • 31 slides

MHD Turbulence: influences on transport and acceleration of energetic particles

MHD Turbulence: influences on transport and acceleration of energetic particles. W H Matthaeus Bartol Research Institute, University of Delaware Pablo Dmitruk Nirmal Seenu Gang Qin John Bieber. Huntsville Workshop 2002: Astrophysical Particle Acceleration in Geospace and Beyond

460 views • 29 slides

In-situ observations of magnetic reconnection in solar system plasma

316 views • 19 slides