Titlebook: Energy Conversion and Particle Acceleration in the Solar Corona; Karl-Ludwig Klein Book 2003 Springer-Verlag Berlin Heidelberg 2003 Chromo

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0075-8450 he current theoretical and experimental status in the field. Paying attention to both the details and the broader picture, this book addresses both the experienced researcher as well as non-specialist researchers from related areas and postgraduate students..978-3-642-05546-1978-3-540-36242-5Series ISSN 0075-8450 Series E-ISSN 1616-6361

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Theoretical Models of Magnetic Configurations Relevant to Energy Release the results mostly obtained by the BEM and compare the reconstructed 3D coronal magnetic structures with Hα, soft X-ray, UV/EUV images and/or radio observations so as to understand the triggering and energy release processes in these flare events.

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Signature of Energy Release and Particle Acceleration Observed by the Nobeyama Radioheliographthat flares start in a small loop and also shown that hot plasmas and high-energy electrons are fed into a nearby larger loop from the small one. Based on these and other observations, it is proposed that “high-beta disruption” is the cause of solar flare phenomena.

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0075-8450 in the Sun‘s interior creates its hot corona and a wealth of dynamical phenomena such as flares and mass ejections. Based on recent significant progress in understanding magnetic reconnection and a wealth of new observations of energetic particle signatures from the sun, the present volume reviews t

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https://doi.org/10.1007/978-1-4614-5348-2eractions between plasmas and magnetic fields. The manner in which magnetically stored energy is converted to other forms, and prominently to energetic particle populations, is clearly of central importance for coronal physics.

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Janos Abonyi,Janos Madar,Ferenc Szeifertfield and flow variations. To these one can apply conservation laws and verify whether boundaries, like the magnetopause, have a normal magnetic field component, i.e., are rotational discontinuities. In the magnetotail the magnetic field structure can be deduced from the temporal variation of the magnetic field during high speed flow events.

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