Abstract
Cosmic rays are the main source of ionization in the atmosphere at altitudes below 55–60 km. This circumstance, together with the fact that cosmic ray flux modulation closely mirrors the solar activity time history, makes cosmic rays a good candidate as a possible mediator in the solar variability – climate relationship. The observed cosmic ray flux variations are described with the aim of emphasizing the features which may be useful in the search of correlation between cosmic rays and atmospheric phenomena.
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Bazilevskaya, G. A., Krainev, M. B., Stozhkov, Yu. I., Svirzhevskaya, A. K., and Svirzhevsky, N. S.: 1991, ‘Long-Term Soviet Program for the Measurement of Ionizing Radiation in the Atmosphere’, J. Geomag. Geoelectr. Suppl. 43, 893–900.
Bazilevskaya, G. A. and Svirzhevskaya, A. K.: 1998, ‘On the StratosphericMeasurements of Cosmic Rays’, Space. Sci. Rev. 85, 431–521.
Bazilevskaya, G. A., Krainev, M. B., Makhmutov, V. S., Sladkova, A. I., Storini, M., and Flueckiger, E.: 1998, ‘The Gnevyshev Gap in Cosmic Ray Physics’, in: J. Medina (ed): rayos cosmicos 98, Proc. 16th European Cosmic Ray Symposium, Departamento de Fisica, Universidad de Alcala, Spain, 83–86.
Beer, J.: 2000, ‘Long Term, Indirect Indices of Solar Variability’. Space Sci. Rev., this volume.
Charakhchyan, A. N.: 1964, ‘Investigation of Stratosphere Cosmic Ray Intensity Fluctuations Induced by Processes on the Sun’, Soviet Physics Uspekhi 7(3), 358–374.
Charakhchyan, A. N., Bazilevskaya, G. A., Stozhkov, Yu. I., and Charakhchyan, T. N.: 1976, ‘Cosmic Rays in the Stratosphere and in the Near-Earth Space During 19th and 20th Cycles of Solar Activity’, Trudy FIAN, Nauka, Moscow, 88, 3–50, (in Russian).
Fisk, L. A. and Wenzel, K.-P., et al.:1998, ‘Global Processes that determine Cosmic Ray Modulation’, Space Sci. Rev. 83, 179–214.
Golenkov, A. E., Svirzhevskaya, A. K., Svirzhevsky, N. S., and Stozhkov, Yu. I.: 1990, ‘Cosmic Ray Latitude Survey in the Stratosphere During the 1987 Solar Minimum’, Proc. 21st Intern. Cosmic Ray Conf. Adelaide, 7, 14–17.
GOST, 1986, Galactic Cosmic Rays. Energy Spectra. Gosudarstvenny Standard 25645.122-85-25645.125-85, Moscow, 1986 (in Russian).
Hatton, C. J.: 1971, ‘The Neutron Monitor’. In: J. G. Wilson and S. A. Wouthuysen, (eds.):Processes in Elementary Particle and Cosmic Ray Physics, North-Holland Publ. Comp., Amsterdam-London, 3–100.
Makhmutov, V. S., Bazilevskaya, G. A., Podgorny, A. I., Stozhkov, Yu.I., Svirzhevsky, N. S.: 1995, ‘The precipitation of electrons into the Earth's atmosphere during 1994’, Proc. 24th Intern. Cosmic Ray Conf. Rome, 4, 1114–1117.
Neher, H. V.: 1967, ‘Cosmic Ray Particles That Changed from 1954 to 1958 to 1965’, J. Geophys. Res. 72(5), 1527–1539.
Neher, H. V.: 1971, ‘Cosmic Rays at High Latitudes and Altitudes Covering Four Solar Maxima’, J. Geophys. Res. 76(7), 1637–1651.
Simpson, J. A.: 1948, ‘The Latitude Dependence of Neutron Densities in the Atmosphere as a Function of Altitude’, Phys. Rev. 73, 1389–1391.
Simpson, J. A., Fonger, W. H., and Tremian, S. B.: 1953, ‘Cosmic Radiation Intensity-Time Variations and Their Origin: I. Neutron Intensity VariationMethod andMeteorological Factors’, Phys. Rev. 90, 934–950.
Stoker, P. H.: 1994, ‘Relativistic Solar Proton Events’, Space Sci. Rev. 73, 327–385.
Storini, M.: 1997, ‘Cosmic rays for solar-terrestrial physics’, Nuovo Cim. 20(6), 871–880.
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Bazilevskaya, G. Observations of Variability in Cosmic Rays. Space Science Reviews 94, 25–38 (2000). https://doi.org/10.1023/A:1026721912992
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DOI: https://doi.org/10.1023/A:1026721912992