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Re-Acceleration of Energetic Particles in Large-Scale Heliospheric Magnetic Cavities

Published online by Cambridge University Press:  24 July 2018

Olga V. Khabarova
Affiliation:
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of RAS (IZMIRAN), Moscow, Russia, email: [email protected]
Olga E. Malandraki
Affiliation:
IAASARS, National Observatory of Athens, Penteli, Greece, email: [email protected]
Gary P. Zank
Affiliation:
Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, AL, USA Department of Space Science, University of Alabama in Huntsville, AL, USA
Gang Li
Affiliation:
Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, AL, USA Department of Space Science, University of Alabama in Huntsville, AL, USA
Jakobus A. le Roux
Affiliation:
Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, AL, USA Department of Space Science, University of Alabama in Huntsville, AL, USA
Gary M. Webb
Affiliation:
Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, AL, USA
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Abstract

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Case studies show that some energetic particle flux enhancements up to MeV/nuc. observed at 1 AU cannot be treated as a consequence of particle acceleration at shocks or during flares. Atypical energetic particle events (AEPEs) are often detected during crossings of magnetic cavities formed by strong current sheets of various origins in the solar wind. Such cavities confine small-scale magnetic islands (SMIs) produced by magnetic reconnection. SMIs, in turn, trap and re-accelerate energetic particles according to predictions based on the theory of Zank et al. describing stochastic particle energization in the supersonic solar wind via numerous dynamically interacting SMIs. AEPEs possess energies that overlap SEP events and can be an important component in understanding space weather.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Jackson, B. V., Clover, J. M., Hick, P. P., et al. 2013, SoPh, 285, 151Google Scholar
Khabarova, O. V., Zank, G. P., Malandraki, O. E., et al. 2017, Sun and Geosphere, 12, 23Google Scholar
Khabarova, O. & Zank, G. P. 2017, ApJ, 843, 4, https://doi.org/10.3847/1538-4357/aa7686CrossRefGoogle Scholar
Khabarova, O., Zank, G. P., Li, G., et al. 2015, ApJ, 808, 181CrossRefGoogle Scholar
Lazarian, A., Vlahos, L., Kowal, G., et al. 2012, SSRv, 173, 557Google Scholar
le Roux, J. A., Zank, G. P., Webb, G. M. & Khabarova, O. 2015, ApJ, 801, 112CrossRefGoogle Scholar
le Roux, J. A., Zank, G. P., Webb, G. M. & Khabarova, O. 2016, ApJ, 827, 47CrossRefGoogle Scholar
Malova, H. V., Popov, V. Yu., Grigorenko, E. E., et al. 2017, ApJ, 834, 34CrossRefGoogle Scholar
Papaioannou, A., Malandraki, O. E., Dresing, N., et al. 2014, Astron. Astrophys., 569, A96, doi: 10.1051/0004-6361/201323336CrossRefGoogle Scholar
Wei, F., Hu, Q., Schwen, R. & Feng, X. 2000, Sci. China Ser. A-Math., 43, 629. https://doi.org/10.1007/BF02908775Google Scholar
Zank, G. P., Hunana, P., Mostafavi, P., et al. 2015, ApJ, 814, 137CrossRefGoogle Scholar
Zank, G. P., le Roux, J. A., Webb, G. M., Dosch, A. & Khabarova, O. 2014, ApJ, 797, 28CrossRefGoogle Scholar
Zank, G., Rice, W. K. M. & Wu, C. 2000, J. Geophys. Res., 105, 25079CrossRefGoogle Scholar
Zharkova, V. V. & Khabarova, O. V. 2015, AnGeo, 33, 457CrossRefGoogle Scholar