Krainev, M. B., and G. A. Bazilevskaya (2004), The structure of the solar cycle maximum phase in the galactic cosmic ray 11-year variation, Adv. Space Res., 35, doi:10.1016/j.asr.2004.11.007.
Krainev, M. B., and W. R. Webber (2003), On the galactic cosmic ray behavior during the maximum phase of the current (23rd) solar cycle, in: The Climatic and Ecological Aspects of the Solar Activity, Proceedings of the Pulkovo International Conference on Solar Physics (in Russian), p. 249, GAO, Pulkovo, St. Petersburg.
Krainev, M. B., and W. R. Webber (2004), The solar cycle in the heliospheric parameters and galactic cosmic ray intensity, in: Multi-wavelength Investigations of Solar Activity, Proc. IAU Symp., 223, p. 81, Cambridge Univ. Press, New York.
Krainev, M. B., and W. R. Webber (2005), The medium energy galactic cosmic rays according to the spacecraft and stratospheric data, Bulletin of the Lebedev Physics Institute (in Russian), 11, 18.
Krainev, M. B., M. Storini, G. A. Bazilevskaya, E. O. Fluckiger, V. S. Makhmutov, A. I. Sladkova, and S. A. Starodubtsev (1999a), The Gnevyshev gap effect in galactic cosmic rays, in: Proc. 26th Int. Cosmic Ray Conf., p. 155, High Energy Astro Physics Institute, University of Utah under the auspieces of the International Union of Pure and Applied Physics (IUPAP), Salt Lake City, Utah, USA.
Krainev, M. B., G. A. Bazilevskaya, and V. S. Makhmutov (1999b), On the large scale solar magnetic fields and the double peak structure of solar activity during the maximum phase of solar cycle, in: The Large-Scale Structure of Solar Activity, Proceedings of the Pulkovo International Conference on Solar Physics (in Russian), p. 121, Pulkovo, St. Petersburg.
Krainev, M. B., G. A. Bazilevskaya, and V. S. Makhmutov (2001), The general features of the galactic cosmic ray intensity in the maximum phase of solar cycles 19-23, in: Proc. 27th Int. Cosmic Ray Conf. (in Russian), p. 3847, Copernicus Gesellschaft e.V., Katlenburg-Lindau under the auspieces of IUPAP, Hamburg, Germany.
Krainev, M. B., G. A. Bazilevskaya, and V. S. Makhmutov (2002), Solar magnetic field and dynamic phenomena in cosmic rays, Adv. Space Res., 29, (3), 331.
Krimigis, S. M., R. B. Decker, E. C. Roelof, and D. Lario (2003), Energetic particle intensity increases at Voyagers 1 and 2 during 2002-03, in: Proc. 28th Int. Cosmic Ray Conf., p. 3769, Institute for Cosmic Ray Research, University of Tokyo, under the auspieces of IUPAP, Tsukuba, Japan.
McDonald, F. B., A. C. Cummings, E. C. Stone, B. Heikkila, N. Lal, and W. R. Webber (2003), Unusual enhancements of MeV ions and electrons as Voyager 1 approaches the heliospheric termination shock, in: Proc. 28th Int. Cosmic Ray Conf., p. 3765, Institute for Cosmic Ray Research, University of Tokyo, under the auspieces of IUPAP, Tsukuba, Japan.
Svirzhevsky, N. S. (2003), The temporal and space variations of the charged radiation in the Earth's atmosphere, Doctor of Science thesis (in Russian), Lebedev Phys. Inst., Russ. Acad. of Sci., Moscow.
Zeldovich, M. A., A. V. Dmitriev, K. Kescemety, Ju. I. Logachev, and I. S. Veselovsky (2000), On the possible detection of the outer heliospheric boundary signatures in accelerated ions seen by Voyager 1 beginning from July 2002, in: Proc. 28th Int. Cosmic Ray Conf., p. 3785, Institute for Cosmic Ray Research, University of Tokyo, under the auspieces of IUPAP, Tsukuba, Japan.
Citation: 2005), The development of the maximum phase of solar cycle 23 in the galactic cosmic ray intensity, Int. J. Geomagn. Aeron., 5, GI3008, doi:10.1029/2004GI000067.
Copyright 2005 by the American Geophysical Union (