Modelling Quasi-Periodic Pulsations in Solar and Stellar Flares

Solar flare emission is detected in all EM bands and variations in flux density of solar energetic particles. Often the EM radiation generated in solar and stellar flares shows a pronounced oscillatory pattern, with characteristic periods ranging from a fraction of a second to several minutes. These...

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Veröffentlicht in:	Space science reviews 2018-02, Vol.214 (1), p.1-54, Article 45
Hauptverfasser:	McLaughlin, J. A., Nakariakov, V. M., Dominique, M., Jelínek, P., Takasao, S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Aerospace Technology and Astronautics Astronomical models Astrophysics and Astroparticles Coalescence Coalescing Dynamic stability Energetic particles Energy Flow stability Flux density Magnetohydrodynamics Observatories Oscillations Particle acceleration Periodicities Physics Physics and Astronomy Planetology Plasma Radiation Solar energetic particles Solar flares Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Stellar flares Stellar models
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