Abstract
Solar proton events possess a wide variety of features that reflect the conditions of solar proton acceleration and propagation. Relevant investigations rely on statistical methods that make it possible to classify events with the aim of obtaining deeper insight into physical processes leading to the generation of solar cosmic rays. In classifying events in power, the intensity of particles with energy above 10MeV at the maximum of the event time profile or the fluence of particles throughout the event time is usually used. A new parameter, Eqm, that characterizes the proton event power and which is some kind of approximation of the maximum energy of accelerated particles is analyzed in the present study. Correlations of Eqm with properties of x-ray flares on the Sun and with the velocity of coronal mass ejections are examined.
Similar content being viewed by others
References
M. Desai and J. Giacalone, Living Rev. Sol. Phys. 13, 3 (2016).
L. I. Miroshnichenko and J. A. Perez-Peraza, Int. J.Mod. Phys. A 23, 1 (2008).
Catalog of Solar Particle Events 1955–1969, Ed. by Z. Svestka and P. Simon (Reidel, Dordrecht, Boston, 1975).
Series of Catalogues of Solar Proton Events in 1970–1997, Ed. by Yu. I. Logachev (1982, 1986, 1989, 1990, 1998). https://doi.org/www.wdcb.ru/stp/data/SPE.
Yu. I. Logachev, G.A. Bazilevskaya, E. V. Vashenyuk, E. I. Daibog, V. N. Ishkov, L. L. Lazutin, L. I. Miroshnichenko, M.N. Nazarova, I. E. Petrenko, A. G. Stupishin, G. M. Surova, and O. S. Yakovchuk, Catalogue of Solar Protonic Events of 23rd Solar Activity Cycle in 1996–2008 (Geofiz. Tsentr RAN, Moscow, 2016) [in Russian]. doi 10.2205/ESDBSAD-001
G. A. Bazilevskaya, J. Phys.: Conf. Ser. 798, 012034 (2017).
GOST (State Stand ard) No. 25645.150-90, Cosmic galactic rays, model of particle fluxes changes (1991).
D. V. Reames, Space Sci. Rev. 175, 53 (2013).
I. M. Chertok, V. V. Grechnev, and N. S. Meshalkina, Astron. Rep. 53, 1059 (2009).
I. G. Richardson, T. T. von Rosenvinge, H. V. Cane, E. R. Christian, C. M. S. Cohen, A. W. Labrador, R. A. Leske, R. A. Mewaldt, M. E. Wiedenbeck, and E. C. Stone, Sol. Phys. 289, 3059 (2014).
M. Dierckxsens, K. Tziotziou, S. Dalla, I. Patsou, M. S. Marsh, N. B. Crosby, O. Maland raki, and G. Tsiropoula, Sol. Phys. 290, 8414 (2015).
V. V. Grechnev, V. I. Kiselev, N. S. Meshalkina, and I. M. Chertok, Sol. Phys. 290, 2827 (2015).
H. V. Cane and D. Lario, Space Sci. Rev. 123, 45 (2006).
A. Papaioannou, I. Sand berg, A. Anastasiadis, A. Kouloumvakos, M. K. Georgoulis, K. Tziotziou, G. Tsiropoula, P. Jiggens, and A. Hilgers, J. Space Weather Space Clim. 6, A42 (2016).
R. Miteva, K.-L. Klein, O. Maland raki, and G. Dorrian, Sol. Phys. 282, 579 (2013).
G.M. Simnett, Astron. Astrophys. 445, 715 (2006).
M. Laurenza, G. Consolini, M. Storini, and A. Damiani, Astrophys. Space Sci. Trans. 8, 19 (2012).
N. Gopalswamy, Geosci. Lett. 3, 8 (2016).
D. F. Webb and T. A. Howard, Living Rev. Sol. Phys. 9, 3 (2012).
A. Belov, Adv. Space Res. 43, 467 (2009).
G. Le and X. Zhang, PoS(ICRC2017)131.
S.W. Kahler and A. Vourlidas, Astrophys. J. 769, 143 (2013).
N. Gopalswamy, H. Xie, S. Yashiro, S. Akiyama, P. Mäkelä, and I. G. Usoskin, Space Sci. Rev. 171, 23 (2012).
C. Salas-Matamoros and K.-L. Klein, Sol. Phys. 290, 1337 (2015).
Author information
Authors and Affiliations
Corresponding author
Additional information
Original Russian Text © Yu.I. Logachev, G.A. Bazilevskaya, E.I. Daibog, V.N. Ishkov, L.L. Lazutin, G.M. Surova, 2018, published in Yadernaya Fizika, 2018, Vol. 81, No. 3, pp. 371–376.
Rights and permissions
About this article
Cite this article
Logachev, Y.I., Bazilevskaya, G.A., Daibog, E.I. et al. New Parameter in the Description of Solar Cosmic Ray Events—Energy of Balance between Solar and Galactic Protons. Phys. Atom. Nuclei 81, 384–389 (2018). https://doi.org/10.1134/S106377881803016X
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S106377881803016X