Physics
Scientific paper
May 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsm24a..07m&link_type=abstract
American Geophysical Union, Spring Meeting 2008, abstract #SM24A-07
Physics
2723 Magnetic Reconnection (7526, 7835), 7526 Magnetic Reconnection (2723, 7835), 7835 Magnetic Reconnection (2723, 7526)
Scientific paper
Petschek reconnection describes how reconnection is able to proceed fast enough to explain observed energy release rates in eruptive events in the solar corona and Earth's magnetosphere. However, Petschek reconnection does not self-consistently occur in resistive magnetohydrodynamics (MHD). It was shown, for example, in the GEM Magnetic Reconnection Challenge [1] that the presence of the Hall effect is sufficient to set up (fast) Petschek reconnection. While it is well established that resistive MHD simulations without the Hall term give slow (Sweet-Parker) reconnection, the situation in hybrid simulations (particle ions, fluid electrons) is less clear, with some studies finding fast reconnection even without the Hall term[2]. In this study, we examine the role of the Hall term in allowing fast reconnection in hybrid simulations, with careful consideration of the chosen electron dissipation model. [1] J. Birn et al., J. Geophys. Res., 106, 3715 (2001). [2] H. Karimabadi, D. Krauss-Varban, J. D. Huba and H. X. Vu, J. Geophys. Res., 109, A09205 (2004).
Cassak Paul
Drake Jeremy J.
Malakit K.
Shay Meni
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