Abstract
Although the current Solar Cycle 24 is characterized by low solar activity, an intense geomagnetic storm (G4) was recorded in June 2015. It was a complex phenomenon that began on 22 June 2015 as the result of intense solar activity, accompanied by several flares and coronal mass ejections that interacted with the Earth’s magnetic field. A Forbush decrease was also recorded at the neutron monitors of the worldwide network, with an amplitude of 8.4%, and in its recovery phase, a second Forbush decrease followed, with an amplitude of 4.0% for cosmic rays of 10 GV obtained with the global survey method. The Dst index reached a minimum value of −204 nT that was detected on 23 June 2015 at 05:00 – 06:00 UT, while the Kp index reached the value eight. For our analysis, we used hourly cosmic-ray intensity data recorded by polar, mid-, and high-latitude neutron monitor stations obtained from the High Resolution Neutron Monitor Database. The cosmic-ray anisotropy variation at the ecliptic plane was also estimated and was found to be highly complex. We study and discuss the unusual and complex cosmic-ray and geomagnetic response to these solar events.
Similar content being viewed by others
References
Akasofu, S.I., Ahn, B.H., Kamide, Y., Allen, J.H.: 1983, A note on the accuracy of the auroral electrojet indices. J. Geophys. Res. 88, 5769. DOI .
Asipenka, A.S., Belov, A.V., Eroshenko, E.A., Klepach, E.G., Oleneva, V.A., Yanke, V.G.: 2009, Interactive database of cosmic ray anisotropy (DB-A10). Adv. Space Res. 43, 708. DOI .
Aslam, O.P.M., Badruddin: 2017, Study of the geoeffectiveness and galactic cosmic-ray response of VarSITI-ISEST campaign events in Solar Cycle 24. Solar Phys. 292, 17. DOI .
Bachelet, F., Balata, P., Iucci, N.: 1965, Some properties of the radiation recorded by the IGY cosmic-ray neutron monitors in the lower atmosphere. Nuovo Cimento A 40, 250. DOI .
Badruddin: 2006, Transient perturbations and their effects in the heliosphere, the geo-magnetosphere, and the Earth’s atmosphere: space weather perspective. J. Astrophys. Astron. 27, 209. DOI .
Bartels, J.: 1949, The standardized index Ks and the planetary index Kp. IATME Bull. 12b, 97.
Belov, A.V., Eroshenko, E.A., Oleneva, V.A., Struminsky, A.B., Yanke, V.G.: 2001, What determines the magnitude of Forbush decreases? Adv. Space Res. 27, 625. DOI .
Belov, A., Baisultanova, L., Eroshenko, E., Mavromichalaki, H., Yanke, V., Pchelkin, V., Plainaki, C., Mariatos, G.: 2005, Magnetospheric effects in cosmic rays during the unique magnetic storm on November 2003. J. Geophys. Res. 110, A09. DOI .
Cane, H.V.: 2000, Coronal mass ejections and Forbush decreases. Space Sci. Rev. 93, 55. DOI .
Davis, T.N., Sugiura, M.: 1966, Auroral electrojet activity index \(AE\) and its universal time variations. J. Geophys. Res. 71, 785. DOI .
Eroshenko, E., Belov, A., Mavromichalaki, H., Mariatos, G., Oleneva, V., Plainaki, C., Yanke, V.: 2004, Cosmic ray variations during the two great bursts of solar activity in the 23rd solar cycle. Solar Phys. 224, 345. DOI .
Gonzalez, W.D., Joselyn, J.A., Kamide, Y., Kroehl, H.W., Rostoker, G., Tsurutani, B.T., Vasyliunas, V.M.: 1994, What is a geomagnetic storm? J. Geophys. Res. 99, 5771. DOI .
Gromova, L.I., Kleimenova, N.L., Levitin, A.E., Gromov, S.V., Dremukhina, L.A., Zelinskii, N.R.: 2016, Daytime geomagnetic disturbances at high latitudes during a strong magnetic storm of June 21 – 23, 2015: the storm initial phase. Geomagn. Aeron. 56, 281. DOI .
Harrison, R.A.: 1995, The nature of solar-flares associated with coronal mass ejection. Astron. Astrophys. 304, 585.
Hundhausen, A.J.: 1999, Coronal mass ejections. In: Strong, K.T., Saba, J.L., Haisch, B.H., Schmelz, J.T. (eds.) The Many Faces of the Sun: A Summary of the Results from NASA’s Solar Maximum Mission, Springer, New York, 143. DOI .
Joselyn, J.A., Tsurutani, B.T.: 1990, Geomagnetic sudden impulses and storm sudden commencements: a note on terminology. Eos Trans. AGU 71, 1808. DOI .
Kamide Y., Kusano K.: 2015, No major solar flares but the largest geomagnetic storm in the present solar cycle. Space Weather 13, 365. DOI .
Kudela, K., Storini, M., Hofer, Y.M., Belov, A.: 2000, Cosmic rays in relation to space weather. Space Sci. Ser. ISSI 10, 153. DOI .
Kudela, K., Brenkus, R.: 2004, Cosmic ray decreases and geomagnetic activity: list of events 1982 – 2002. J. Atmos. Solar-Terr. Phys. 66, 112. DOI .
Kumar, A., Badruddin: 2014, Interplanetary coronal mass ejections, associated features, and transient modulation of galactic cosmic rays. Solar Phys. 289, 2177. DOI .
Lingri, D., Mavromichalaki, H., Belov, A., Eroshenko, E., Yanke, V., Abunin, A., Abunina, M.: 2016, Solar activity parameters and associated Forbush decreases during the minimum between Cycles 23 and 24 and the ascending phase of Cycle 24. Solar Phys. 291, 1025. DOI .
Liu, Y.D., Hu, H., Wang, R., Yang, Z., Zhu, B., Liu, Y.A., Luhmann, J.G., Richardson, J.D.: 2015, Plasma and magnetic field characteristics of solar coronal mass ejections in relation to geomagnetic storm intensity and variability. Astrophys. J. Lett. 809, L34. DOI .
Livada, M., Lingri, D., Mavromichalaki, H.: 2015, Galactic cosmic ray spectrum of the Forbush decreases of March 2012. In: Proc. 12th Hel.A.S. Conf., vol. 1, p. 12.
Lockwood, J.A.: 1971, Forbush decreases in the cosmic radiation. Space Sci. Rev. 12, 658. DOI .
Mavromichalaki, H., Papaioannou, A., Mariatos, G., Papahliou, M., Belov, A., Eroshenko, E., Yanke, V., Stassinopoulos, E.G.: 2007, Cosmic ray radiation effects on space environment associated to intense solar and geomagnetic activity. IEEE Trans. Nucl. Sci. 54, 1089. DOI .
Mavromichalaki, H., Eroshenko, E., Belov, A., Yanke, V., Mariatos, G., Laoutaris, A., Kontiza, A.: 2013, Magnetospheric cut-off rigidity variations recorded by neutron monitors in the events from 2001 to 2010. Proc. 23rd ECRS. J. Phys. Conf. Ser. 409. DOI .
Papaioannou, A., Belov, A., Mavromichalaki, H., Eroshenko, E., Oleneva, V.: 2009, The unusual cosmic ray variations in July 2005 resulted from western and behind the limb solar activity. Adv. Space Res. 43, 582. DOI .
Papaioannou, A., Souvatzoglou, G., Paschalis, P., Gerontidou, M., Mavromichalaki, H.: 2014, Solar Phys. 289, 423. DOI .
Papailiou, M., Mavromichalaki, H., Eroshenko, E., Belov, A., Yanke, V.: 2012, Precursor effects in different cases of Forbush decreases. Solar Phys. 276, 337. DOI .
Piersanti, M., Alberti, T., Bemporad, A., Berrilli, F., et al.: 2017, Comprehensive analysis of the geoeffective solar event of 21 June 2015: effects on the magnetosphere, plasmasphere, and ionosphere systems. Solar Phys. 292, 169. DOI .
Plainaki, C., Belov, A., Eroshenko, E., Mavromichalaki, H., Yanke, V.: 2007, Modeling ground level enhancements: the event of 20 January 2005. J. Geophys. Res. 112, A04. DOI .
Plainaki, C., Mavromichalaki, H., Belov, A., Eroshenko, E., Yanke, V.: 2009, Neutron monitor asymptotic directions of viewing during the event of 13 December 2006. Adv. Space Res. 43, 518. DOI .
Sugiura, M.: 1964, Hourly Values of Equatorial Dst for IGY, Annals of the International Geophysical Year 35, Pergamon Press, Oxford, 945.
Tsurutani, B., Lakhina, G.: 2014, An extreme coronal mass ejection and consequences for the magnetosphere and Earth, EGU General Assembly, Vienna, id. 3064.
Tsyganenko, N.A., Stern, D.P.: 1996, Modeling the global magnetic field of the large-scale Birkeland current systems. J. Geophys. Res. 101, 27187. DOI .
Venkatesan, D., Badruddin: 1990, Cosmic-ray intensity variations in the 3-dimensional heliosphere. Space Sci. Rev. 52, 121. DOI .
Wanliss, J.A., Showalter, K.M.: 2006, High-resolution global storm index: Dst versus SYM-H. J. Geophys. Res. 111, A02202. DOI .
Acknowledgements
Special thanks to the colleagues of the NM stations ( http://www.nmdb.eu ) for kindly providing the cosmic-ray data used in this study in the frame of the high-resolution neutron monitor database NMDB, funded under the European Union’s FP7 Program (contract no. 213007). Thanks are due to the IZMIRAN group of the Russian Academy of Sciences for kindly providing Forbush decrease data. The co-author D. Lingri thanks the General Secretariat for Research and Technology (GSRT) and the Hellenic Foundation for Research and Innovation (HFRI) of the Greek Ministry of Education for supporting her PhD fellowship. Thanks are also due to the anonymous referee for useful suggestions that improved this manuscript significantly.
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Conflict of Interest
The authors declare that they have no conflicts of interest.
Rights and permissions
About this article
Cite this article
Samara, E., Smponias, A., Lytrosyngounis, I. et al. Unusual Cosmic Ray Variations During the Forbush Decreases of June 2015. Sol Phys 293, 67 (2018). https://doi.org/10.1007/s11207-018-1290-9
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s11207-018-1290-9