Abstract
For over 60 years, neutron monitors have been the main standard and high precision detectors for measuring cosmic rays with energy from 400 MeV to hundreds GeV. In order to obtain sufficiently complete information about the distribution of cosmic rays outside the magnetosphere, it is necessary to have a network of detectors spaced evenly enough around the globe. The ring of stations method is one of the most useful methods for studying the properties of the angular distribution of cosmic rays without expressing the cosmic ray intensity in terms of spherical harmonics. The method allows one to get the hourly longitude distribution of the cosmic ray intensity without modeling. The main objective of this work is to expand the use of the ring of stations method, as it is a convenient and useful method of studying cosmic ray variation. Using the ring of stations method, it is possible to study specific angular distributions of cosmic ray variation that are described poorly by the sum of the first spherical harmonics. The ring of stations method is primarily used to study Forbush decreases. Detailed descriptions of Forbush decrease investigation by the ring of stations method are presented in this study. The application of the method to the study of the precursors of Forbush decreases and cosmic rays behavior inside the solar wind disturbances is shown.
Similar content being viewed by others
References
Abunin, A.A., Abunina, M.A., Belov, A.V., Eroshenko, E.A., Oleneva, V.A., Yanke, V.G.: 2012, Geomagn. Aeron.52(3), 292. DOI.
Abunin, A.A., Abunina, M.A., Belov, A.V., Chertok, I.M.: 2020, Solar Phys.295(1), 7. DOI.
Asipenka, A., Belov, A.V., Eroshenko, E., Mavromihalaki, H., Papailiou, M., Papaioannou, A., Oleneva, V., Yanke, V.G.: 2009 In: Proc. 31st ICRC4, Lodz, Poland, 3100.
Belov, A.V.: 2008, In: Gopalswamy, N., Webb, D.F. (eds.) Universal Heliophysical Processes, Proc. IAU Symp.257, Cambridge Univ. Press, Cambridge, 439. DOI.
Belov, A.V., Dorman, L.I., Eroshenko, E.A., Iucci, N., Villoresi, G., Yanke, V.G.: 1995, In: Iucci, N., Lamanna, E. (eds.) Proc. 24th ICRC, Rome, Italy, Internat. Union Pure Appl. Phys.4, 888.
Belov, A.V., Bieber, J.W., Eroshenko, E.A., Evenson, P., Pyle, R., Yanke, V.G.: 2001, In: Droege, W., Kunow, H., Scholer, M. (eds.) Proc. 27th ICRC, Hamburg, Germany, Internat. Union Pure Appl. Phys.9, 3507.
Belov, A.V., Bieber, J.W., Eroshenko, E.A., Evenson, P., Pyle, R., Yanke, V.G.: 2003, Adv. Space Res.31(4), 919. DOI.
Belov, A., Baisultanova, L., Eroshenko, E., Mavromichalaki, H., Yanke, V., Pchelkin, V., Plainaki, C., Mariatos, G.: 2005a, J. Geophys. Res.110, A09S20. DOI.
Belov, A., Eroshenko, E., Mavromichalaki, H., Plainaki, C., Yanke, V.: 2005b, Ann. Geophys.23(6), 2281. DOI.
Belov, A., Abunin, A., Abunina, M., Eroshenko, E., Oleneva, V., Yanke, V., Papaioannou, A., Mavromichalaki, H., Gopalswamy, N., Yashiro, S.: 2014, Solar Phys.289, 3949. DOI.
Belov, A., Abunin, A., Abunina, M., Eroshenko, E., Oleneva, V., Yanke, V., Papaioannou, A., Mavromichalaki, H.: 2015, Solar Phys.290(5), 1429. DOI.
Belov, A., Abunina, M., Abunin, A., Eroshenko, E., Oleneva, V., Yanke, V.: 2017a, Geomagn. Aeron.57(4), 389. DOI.
Belov, A., Abunina, M., Abunin, A., Eroshenko, E., Oleneva, V., Yanke, V.: 2017b, Geomagn. Aeron.57(5), 541. DOI.
Belov, A., Eroshenko, E., Yanke, V., Oleneva, V., Abunin, A., Abunina, M., Papaioannou, A., Mavromichalaki, H.: 2018, Solar Phys.293(4), 68. DOI.
Bieber, J.W., Evenson, P.: 1995, In: Iucci, N., Lamanna, E. (eds.) Proc. 24th ICRC, Rome, Italy, Internat. Union Pure Appl. Phys.4, 1316.
Bothmer, V., Zhukov, A.: 2007, In: Bothmer, V., Daglis, I.A. (eds.) Space Weather — Physics and Effects, Springer, Berlin, 31. DOI.
Cane, H.V.: 2000, Space Sci. Rev.93, 55. DOI.
Dorman, L.I.: 1974, Cosmic Rays: Variations and Space Explorations, North-Holland, Amsterdam, 675.
Dorman, L.I.: 2005, Ann. Geophys.23, 2997.
Dorman, L., Kaminer, N., Kuzmicheva, A.: 1972, Geomagn. Aeron.12(5), 814.
Gopalswamy, N.: 2009, In: Tsuda, T., Fujii, R., Shibata, K., Geller, M.A. (eds.) Climate and Weather of the Sun-Earth System (CAWSES): Selected Papers from the 2007 Kyoto Symposium, TERRAPUB, Tokyo, 77.
Grigoryev, V.G., Starodubtsev, S.A.: 2015, Bull. Russ. Acad. Sci., Phys.79(5), 649. DOI.
Gvozdevsky, B., Belov, A., Gushchina, R., Eroshenko, E., Yanke, V.: 2019, J. Phys. Conf. Ser.1181(1), 012008. DOI.
Hatton, C.J., Carmichael, H.: 1964, Can. J. Phys.42(12), 2443. DOI.
Kaminer, N.S., Kuzmicheva, A.E., Mymrina, N.V.: 1981, Geomagn. Aeron.21(2), 358.
Korotkov, V., Berkova, M., Belov, A., Eroshenko, E., Yanke, V., Pyle, R.: 2013, J. Geophys. Res.118(11), 6852. DOI.
Kryakunova, O., Belov, A., Abunin, A., Abunina, M., Eroshenko, E., Malimbayev, A., Tsepakina, I., Yanke, V.: 2015, J. Phys. Conf. Ser.632, 012062. DOI.
Krymsky, G.F., Altukhov, A.M., Kuzmin, A.I., Skripin, G.V.: 1966, A New Method for Studying the Anisotropy of Cosmic Rays – Investigation of Geomagnetism and Aeronomy, Nauka, Moscow, 105.
Krymsky, G.F., Kuzmin, A.I., Krivoshapkin, P.A., Samsonov, I.S., Skripin, G.V., Transkii, I.A., Chirkov, N.P.: 1981, Cosmic Rays and Solar Wind, Nauka, Novosibirsk, 224.
Kudela, K., Storini, M.: 2006, Adv. Space Res.37(8), 1443. DOI.
Kuwabara, T., Bieber, J.W., Clem, J., et al.: 2006, Space Weather4, S08001. DOI.
Leerungnavarat, K., Ruffolo, D., Bieber, J.W.: 2003, Astrophys. J.593(1), 587. DOI.
Lingri, D., Mavromichalaki, H., Belov, A., Abunina, M., Eroshenko, E., Abunin, A.: 2019, Solar Phys.294(6), 70. DOI.
Lockwood, J.A.: 1971, Space Sci. Rev.12(5), 658. DOI.
Mavromichalaki, H., Papaioannou, A., Gerontidou, M., Papailiou, M., Plainaki, C., Belov, A., Eroshenko, E., Abunin, A., Abunina, M., Yanke, V.: 2013, J. Phys. Conf. Ser.409, 012206. DOI.
Moraal, H., Belov, A., Clem, J.: 2000, Space Sci. Rev.93, 285. DOI.
Nagashima, K., Fujimoto, K., Morishita, I.: 1994, J. Geophys. Res.99(A11), 21419. DOI.
Nagashima, K., Sakakibara, S., Fujimoto, K., Tatsuoka, R., Morishita, I.: 1990, Nuovo Cimento C13C, 551. DOI.
Okike, O., Collier, A.B.: 2011, J. Atmos. Solar-Terr. Phys.73(7–8), 796. DOI.
Papailiou, M., Mavromichalaki, H., Belov, A., Eroshenko, E., Yanke, V.: 2012a, Solar Phys.276(1–2), 337. DOI.
Papailiou, M., Mavromichalaki, H., Belov, A., Eroshenko, E., Yanke, V.: 2012b, Solar Phys.280(2), 641. DOI.
Papailiou, M., Mavromichalaki, H., Abunina, M., Belov, A., Eroshenko, E., Yanke, V., Kryakunova, O.: 2013, Solar Phys.283(2), 557. DOI.
Parsons, N.R.: 1960a, Tellus12(4), 450. DOI.
Parsons, N.: 1960b, J. Geophys. Res.65(10), 3159. DOI.
Shah, G., Kaul, C., Razdan, H., Kaul, S.: 1981 In: Proc. 17th ICRC4, Paris, France, 21.
Shea, M.A., Smart, D.F.: 1975 In: Proc. 14th ICRC4, Munchen, Germany, 1298.
Shea, M.A., Smart, D.F.: 2012, Space Sci. Rev.171(1–4), 161. DOI.
Shea, M.A., Smart, D.F., Humble, J.E., Fluckiger, E.O., Gentile, L.C., Nichol, M.R.: 1987 In: Proc. 20th ICRC3, Moscow, USSR, 171.
Simpson, J.A.: 1957, Ann. Int. Geophys. Year4, 351.
Acknowledgements
This research was partially supported by the Russian Foundation of Basic Research under grants 18-52-34004 and 18-02-00451, experimentally and methodologically supported by the project UNU. We also acknowledge the NMDB database (www.nmdb.eu), founded under the European Unions FP7 program (contract No. 213007), for providing the data.
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Disclosure of Potential Conflicts of Interest
The authors declare that they have no conflicts of interest.
Additional information
Publisher’s Note
Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
Rights and permissions
About this article
Cite this article
Abunina, M.A., Belov, A.V., Eroshenko, E.A. et al. Ring of Stations Method in Cosmic Rays Variations Research. Sol Phys 295, 69 (2020). https://doi.org/10.1007/s11207-020-01639-7
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s11207-020-01639-7