[PDF] Top 20 Steady models for magnetic reconnection

... and magnetic field strength do show some difference and o f course there is now a density gradient in the æ-direction, b u t the va ria tio n o f the solutions w ith changes in the reconnection regime (or ... See full document

... a steady-state two-phase picture instead of the cooling-flow scenario, we must ex- plain how the two phases are thermally insulated from each other, and what prevents the cool phase from the radiative ...chaotic ... See full document

... Numerical models must take a Large Eddy Simulation (LES) approach, explicitly computing only a fraction of the active dynamical ...of magnetic fields in a turbulent, electrically conducting fluid flow can ... See full document

... examined magnetic reconnection, not as an isolated pro- cess that occurs in idealized, controlled conditions, but as a necessary ingredient in the complex nonlinear dynamical process that we call ... See full document

... of magnetic recon- nection are naturally much more complicated than studies of the large-scale ...of magnetic reconnection, however, restricts modeling to simpler geometries, usually, as in our case, ... See full document

... diffusion models of particle propagation in the ...wide magnetic field polarity domains generated by the 11 yr ...Where magnetic field do- mains converge on each other due to solar wind gradient, ... See full document

... ing magnetic fields that involves a force normal to the re- connection ...the reconnection layer through its wide surface rather than through its narrow ends, as is the case in traditional magnetic ... See full document

... 4. Steady-state magnetic reconnection. The steady-state, incompressible MHD equations are reduced to two non-linear coupled partial differential ...equations. Reconnection solutions are ... See full document

... why magnetic reconnec- tion in nature proceeds on faster time scale than the resistive diffusion timescale predicted by the Sweet-Parker model in the magnetohydrodynamics (MHD) ...simulation models ... See full document

... netic reconnection between two flux ropes through a moving reconnection site is ...single magnetic field null at its center. The ini- tial magnetic field configuration is embedded into a ... See full document

... fast reconnection phase (t = 193 - 194 µs) as “phase 1” to focus on the energy of electromagnetic fluctu- ...fast reconnection and the generation of large fluctuations clearly occur simulta- neously as ... See full document

... heating models such as the nanoflare ...role magnetic reconnection plays in producing solar flares (impulsive events that produce intense extreme-ultraviolet, X-ray, and sometimes gamma radiation) ... See full document

... Magnetic reconnection in partially ionized plasmas was experimentally investigated using the RMF ...quasi-steady magnetic reconnection was induced by contacting their poloidal ...of ... See full document

... a steady state soon after the experiment was started and so transient waves soon damped out or left the ...imposed magnetic field on the boundary; without this, the results from Chapter 4 show that tearing ... See full document

... the magnetic null is included by the tetrahedron at 6-time points, corresponding to N1 (a), N2 (b - d), N3 (e and f) ...single magnetic null included by the Cluster tetrahe- dron, which well matches the ... See full document

... of magnetic fields with complex field line mappings, for example, magnetic ...complex magnetic field, a pair of field lines traced from nearby starting points may take very different paths through ... See full document

... the magnetic field vector increment using a time lag τ and h i denotes an appropriate time ...identifying reconnection exhausts and current sheets, a time lag τ ¼ 3 s is ...identifying reconnection ... See full document

... Figure 2. The solar wind and local conditions surrounding the aurora enhancement shown in Figure 1 are shown. (left) The IMF components are plotted in the top panel. The solar wind velocity is plotted in the second ... See full document

... dayside magnetic reconnection has only been identified at the ...near-noon reconnection within Saturn’s magnetodisc using measurements from the Cassini ...the reconnection region are ... See full document

... the reconnection physics for an X-point [5, ...initial magnetic stress, determined by the ini- tial X-point magnetic field configuration, causes the sys- tem to ...The magnetic stress is ... See full document