Results 21 to 30 of about 2,611,112 (157)
Extreme ultraviolet imaging of three-dimensional magnetic reconnection in a solar eruption [PDF]
X.C., J.Q.S., M.D.D., Y.G., P.F.C. and C.F. are supported by NSFC through grants 11303016, 11373023, 11203014 and 11025314, and by NKBRSF through grants 2011CB811402 and 2014CB744203. C.E.P. and S.J.E. are supported by the UK STFC. J.Z.
Sun, J.Q. +11 more
core +1 more source
Differences in the response to CME and CIR drivers of geomagnetic disturbances
Utilizing 1-minute resolution data on the geomagnetic indices SYM-H, AE, solar wind parameters (velocity Vsw and density Np), and z-component Bz of the interplanetary magnetic field (IMF) during solar cycles 23 and 24, we have statistically analyzed the ...
Namuun B. +3 more
doaj +1 more source
Aspects of three-dimensional MHD : magnetic reconnection and rotating coronae [PDF]
Solutions of the magnetohydrodynamic (MHD) equations are very important for modelling laboratory, space and astrophysical plasmas, for example the solar and stellar coronae, as well as for modelling many of the dynamic processes that occur in these ...
Al-Salti, Nasser S.
core +2 more sources
Coronal heating is a longstanding issue in solar physics as well as plasma physics in general. In recent years, significant resolution improvements of satellite observations have contributed to a deeper understanding of small-scale physics, e.g ...
Jitong Zou +4 more
doaj +1 more source
Does Magnetic Reconnection Occur in the Near Lunar Surface Environment?
The near lunar surface contains small‐scale magnetic field structures that provide a natural test bed for observing plasmas with a non‐zero Hall electric field, as well as potentially facilitating electron‐only reconnection.
R. P. Sawyer +7 more
doaj +1 more source
Magnetic reconnection drives the ejection of plasmas during solar flares through changes in the magnetic fields. Here, the authors use a laboratory-based experiment to create magnetic reconnection in a regime in which the plasma on one side of the ...
Zhonghai Zhao +17 more
doaj +1 more source
Pickup Ion–Mediated Magnetic Reconnection in the Outer Heliosphere
Pickup ions (PUIs) play a crucial role in the heliosphere, contributing to the mediation of large-scale structures such as the distant solar wind, the heliospheric termination shock, and the heliopause.
M. Nakanotani, G. P. Zank, L.-L. Zhao
doaj +1 more source
The acceleration and heating of solar wind particles by magnetic reconnection are important mechanisms in space physics. Although alpha particles ( ^4 He ^2+ ) are the second most abundant population of solar wind ions, their kinetic behavior in solar ...
Die Duan +12 more
doaj +1 more source
Magnetopause reconnection across wide local time [PDF]
During April to July 2007 a combination of 10 spacecraft provided simultaneous monitoring of the dayside magnetopause across a wide range of local times.
Volwerk, M. +21 more
core +6 more sources
The investigation of quasi-separatrix layers in solar magnetic fields [PDF]
The structure of the magnetic field is often an important factor in many energetic processes in the solar corona. To determine the topology of the magnetic field features such as null points, separatrix surfaces, and separators must be found.
Restante, Anna Lisa
core +2 more sources

