Results 191 to 200 of about 4,329,863 (238)

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

Sci Adv
Xing C, Cheng X, Aulanier G, Ding M.
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

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

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Magnetic Reconnection

, 2006
Christopher A. Jennings
semanticscholar   +4 more sources

Observations of Particle Acceleration in Magnetic Reconnection–driven Turbulence

Astrophysical Journal, 2020
The Magnetospheric Multiscale Mission observes, in detail, charged particle heating and substantial nonthermal acceleration in a region of strong turbulence ( , where is the magnetic field) that surrounds a magnetic reconnection X-line.
R. Ergun, N. Ahmadi, L. Kromyda, S. Schwartz, A. Chasapis, S. Hoilijoki, F. Wilder, J. Stawarz, K. Goodrich, D. Turner, I. Cohen, S. Bingham, J. Holmes, R. Nakamura, F. Pucci, R. Torbert, J. Burch, P. Lindqvist, R. Strangeway, O. le Contel, B. Giles   +20 more
semanticscholar   +1 more source

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