Results 161 to 170 of about 1,658,906 (207)

Flying through an Eruption-associated Magnetic Reconnection Current Sheet in the Solar Corona

Patel R, Niembro T, Xie X, Seaton D, Badman S, Roy S, Rivera Y, Reeves K, Stenborg G, Hess P, West M, Feller A, Hirzberger J, Suarez DO, Solanki S, Strecker H, Valori G.   +16 more
europepmc   +1 more source

Propagating slow-mode shocks discovered in dynamical solar flare loops. [PDF]

Nat Commun
Ye J, Shen C, Raymond JC, Cai Q, Mei Z, Hu J, Chen Y, Li Y, Lin J.   +8 more
europepmc   +1 more source

Back reaction of the untwisting solar corona scars sunspots. [PDF]

Sci Adv
Xing C, Cheng X, Aulanier G, Ding M.
europepmc   +1 more source

Potential Solar Precursors to Magnetic Switchbacks. [PDF]

Space Sci Rev
Tripathi D, Madjarska MS, Karpen J, Velli M, Froment C, Pariat E, Patsourakos S, Raouafi NE, Rouillard AP, Sterling AC, Tziotziou K, Wyper PF.   +11 more
europepmc   +1 more source

Miniature Dungey-like cycle at Mars. [PDF]

Nat Commun
Xu S, McFadden JP, Mitchell DL, Luhmann JG, Halekas JS, Hanley KG, Mazelle CX, Espley JR, Curry SM.   +8 more
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Magnetic Reconnection in Plasmas

Astrophysics and Space Science, 1996
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
openaire   +2 more sources

Magnetic Reconnection

2004
Magnetic reconnection is a fundamental dynamical process in highly conductive plasmas. It can be regarded as the process that removes the following difficulty. On typical dynamical time scales a sufficiently hot spatially extended PLASMA behaves approximately as an ideal fluid in the sense that resistive effects are ignorable.
Schindler, Karl, Hornig, Gunnar
openaire   +3 more sources

Reconnection rates in driven magnetic reconnection

Physics of Plasmas, 2007
Using resistive magnetohydrodynamic simulations, we investigate the influence of various parameters on the reconnection rate in two scenarios of magnetic reconnection. The first scenario consists of the “Newton Challenge” problem [Birn et al., Geophys. Res. Lett. 32, L06105 (2005)].
J. Birn, M. Hesse
openaire   +1 more source

Magnetic reconnection

Physics Reports, 1994
This lecture deals with the concept of magnetic field lines and with the conservation of magnetic flux. In high temperature fusion devices like tokamaks flux conservation can be violated and reconnection can occur at closed magnetic field lines. Reconnection processes lead to changes in the global topology of the magnetic field.
openaire   +3 more sources

Nonlinear collisionless magnetic reconnection

Physical Review Letters, 1993
Collisionless magnetic reconnection in regimes where the mode structure is characterized by global convection cells is found to exhibit a quasiexplosive time behavior in the early nonlinear stage where the fluid displacement is smaller than the equilibrium scale length. This process is accompanied by the formation of a current density sublayer narrower
M. OTTAVIANI, PORCELLI, Francesco
openaire   +4 more sources