Results 11 to 20 of about 2,458,506 (201)
The Astrophysical Journal, 2023 Although magnetic reconnection plays a key role in the formation of a solar filament, the detailed formation process is still ambiguous. Combining the observational data from the New Vacuum Solar Telescope and the Solar Dynamics Observatory, we analyzed ...
Liping Yang +9 more
doaj +1 more source
Magnetic Reconnection and Intermittent Turbulence in the Solar Wind [PDF]
Physical Review Letters, 2014 5 pages, 3 figures, submitted to Physical Review ...
K. T. Osman +7 more
openaire +4 more sources
Open magnetic flux and magnetic flux closure during sawtooth events [PDF]
, 2008 peer reviewedWe use IMAGE-FUV observations of the polar aurora and measurements of the ionospheric convection from the SuperDARN radar network to study several sawtooth events previously reported in the literature. We estimate the amount of open magnetic
Hubert, Benoît +6 more
core +6 more sources
Solar Flares as Cascades of Reconnecting Magnetic Loops [PDF]
Physical Review Letters, 2003 A model for the solar coronal magnetic field is proposed where multiple directed loops evolve in space and time. Loops injected at small scales are anchored by footpoints of opposite polarity moving randomly on a surface. Nearby footpoints of the same polarity aggregate, and loops can reconnect when they collide.
Hughes, D. +4 more
openaire +3 more sources
Differences in the response to CME and CIR drivers of geomagnetic disturbances
Solar-Terrestrial Physics, 2023 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
Extreme ultraviolet imaging of three-dimensional magnetic reconnection in a solar eruption [PDF]
, 2015 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. +9 more
core +1 more source
Aspects of three-dimensional MHD : magnetic reconnection and rotating coronae [PDF]
, 2010 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
The Astrophysical Journal, 2023 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?
Geophysical Research Letters, 2023 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 in Strongly Magnetized Regions of the Low Solar Chromosphere [PDF]
The Astrophysical Journal, 2018 Abstract Magnetic reconnection in strongly magnetized regions around the temperature minimum region of the low solar atmosphere is studied by employing MHD-based simulations of a partially ionized plasma within a reactive 2.5D multi-fluid model.
Lei Ni +3 more
openaire +2 more sources