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In addition, the interaction between solar wind and the magnetosphere leads to substorms, which are manifestations of the explosive energy release processes.
Nonthermal electrons propagate along the coronal magnetic field thereby exciting dm- and m-wave radio burst emission after acceleration during reconnection or other energy release processes in heights of some Mm to ⩾700 Mm.
We also review a selection of new models that illustrate the current state of the art, as well as highlighting the complexity of energy release processes mediated by reconnection in complicated three-dimensional magnetic fields.
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We discuss the energy release process in a solar flare.
Here, we discuss various numerical approaches that attempt to uncover the dynamical energy release process.
The NCER value is also important to understand how the energy release process varies depending on seismicity patterns such as mainshock aftershock, foreshock mainshock aftershock, and swarm types.
This may provide a new clue to understand the coronal magnetic field structure involved in the energy release process of flares.
Radio bursts with fine structures in decimetric centimetric wave range are generally believed to manifest the primary energy release process during flare/CME events.
Results of thermal analyses reveal that the polymer or carbon coatings have little negative effect on the energy release process of the Zr powder.
In other words, our estimations are probably the lower bound of the rupture process, revealing the first-order rupture features for the 2008 Wenchuan earthquake, namely, the main energy release process.
Period of nighttime Pc3 waves is to be determined either by the periodicity of energy release process, or by band-pass filtering which can occur during the wave trapping and propagation along the magnetotail waveguide (Mazur et al. 2010).
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