Acceleration of Solar Energetic Particles Rami Vainio University of Helsinki, Department of Physics, Finland University of Turku, Department of Physics and Astronomy, Finland SPACECAST.
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Acceleration of Solar Energetic Particles Rami Vainio University of Helsinki, Department of Physics, Finland University of Turku, Department of Physics and Astronomy, Finland SPACECAST Stakeholder Meeting, BAS, 7 February 2014 Solar energetic particle events Lario (2005) Flares or shocks? Large gradual SEP events nearly always accompanied with both! –30 min Solar energetic particle events Lario (2005) Present paradigm of SEP acceleration in gradual events CME-driven shocks are the main source of deka-MeV protons during the largest SEP events CME driven shocks Diffusive shock acceleration u2 SW frame u1 ∆u = u2 – u1 Turbulent foreshock Outward-streaming ions scattering off turbulence lead to amplification of fluctuations Bootstrapping! Modeling in SPACECAST Alfvén wave intensity [G2] Proton intensity [cm–2 sr–1 s–1 MeV–1] Distance of the shock from the Sun = 14 – 22 R Mathematical model (—) developed for turbulent region explains simulations (- - -) Three different initial particle distributions 1a 2a 3a 4a 1b 2b 3b 4b 1c R = 5.8–11 R θBn = 2.8° Vs = 1920 km/s R = 14–22 R θBn = 5.4° Vs = 1820 km/s R = 25–36 R θBn = 8.7° Vs = 1620 km/s R = 40–60 R θBn = 14° Vs = 1430 km/s 2c 3c 4c New tool for space weather modelling Summary • Solar energetic particles are accelerated in flares and CMEdriven shocks – CME-driven shocks responsible for large gradual events • SPACECAST project has developed models for particle acceleration in CME-driven shocks – First steps taken towards operational direction by analyzing simulations and developing a semi-analytical description of ion foreshocks in CMEs • Next steps: integration of SPACECAST results to a state-of-theart transport code (see Angels Aran’s presentation) Acknowledgements • The research leading to these results has received funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement no 262468, and is supported in part by the University of Helsinki