Results 151 to 160 of about 1,699 (184)
Some of the next articles are maybe not open access.
Solar Flares and Magnetic Reconnection Experiments
Physica Scripta, 1984On the basis of dimensionless parameters a comparison has been made between the solar flares phenomena and special laboratory experiments.
S V Bulanov, V A Dogiel, A G Frank
openaire +1 more source
Solar Flares and Magnetic Reconnection
2005Abstract Recent studies by the author and his colleagues on solar flares based on the magnetic reconnection model are reviewed. The studies have been done mainly by using the data sets of space-craft observations and super-computer simulations. The covered topics are an EUV observation of reconnection inflows, MHD simulations of the reconnection ...
openaire +1 more source
Explosive events and magnetic reconnection in the solar atmosphere
AIP Conference Proceedings, 1992Explosive events are highly‐dynamic, small‐scale phenomena commonly observed in spectra of transition zone lines. Their velocities are near 100 km s−1, sizes near 1500 km, and time scales near 60 s. They occur at a height of 1000–2000 km, below typical transition zone structures.
openaire +1 more source
Magnetic Reconnection in Solar Flares
Hvar Observatory bulletin, 2004Various aspects of solar flares are considered in the framework of analytic solutions of the complete set of MHD equations describing the the 2.5-D Petchek's reconnection model. In particular, we compare the theoretical results with characteristics of two-ribbon flares since they provide spatially resolved measurements of various plasma parameters.
Skender, Marina, Vršnak, Bojan
openaire +2 more sources
Magnetic Reconnection in the Solar Wind: An Update
AIP Conference Proceedings, 2010Magnetic reconnection in the solar wind commonly occurs in a quasi‐stationary mode. It produces extensive Petschek‐like exhausts of roughly Alfvenic jetting plasma typically bounded by back‐to‐back rotational discontinuities that bifurcate a reconnecting current sheet. It occurs most frequently at current sheets associated with relatively small (
J. T. Gosling +5 more
openaire +1 more source
Solar Magnetic Topologies and Reconnection
2013A review is presented on the topology and eruption of twisted magnetic configurations in connection with eruptive flares, dynamical disparition brusque of prominences, and coronal mass ejections. A classical view of magnetic reconnection is mainly based on the MHD physics of 2-D configurations with an X-type neutral point, or on the extension of it to ...
openaire +1 more source
Solar magnetic reconnection seen in detail
Physics Today, 2013New observations provide the most complete picture yet for the most energetic explosions in the solar system.
openaire +1 more source
On the evolution of magnetic reconnection in the solar wind
Magnetic reconnection is a fundamental process in astrophysical plasma, as it enables the dissipation of energy at kinetic scales as well as large-scale reconfiguration of the magnetic topology. In the solar wind, its quantitative role in plasma dynamics and particle energization remains an open question that is starting to come into focus as more ...Naïs Fargette +8 more
openaire +1 more source
Analysis of Magnetic Reconnections and Compression of Magnetic Islands in the Solar Wind
Russian Journal of Mathematical Physics, 2018zbMATH Open Web Interface contents unavailable due to conflicting licenses.
openaire +1 more source
Magnetic reconnection and some solar applications
Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences, 2000Magnetic reconnection is a fundamental plasma–physics process that is of great importance for the Sun, the Earth9s magnetosphere and all astrophysical objects which have magnetic fields. It is a process central to the generation of magnetic fields in stars and also plays a major role in the heating of solar and stellar coronae.
openaire +1 more source