Abstract
Primary CR of galactic and solar origin (mostly protons and nuclei of different Z) undergo nuclear interactions with air atoms and generate a lot of secondary particles (secondary CR). As will be shown in Chapter 11, secondary relativistic positrons and electrons are responsible for lightning between clouds and ground, and between two clouds, as well as for discharges at great altitudes between clouds and the ionosphere (sprites). Primary CR (mostly protons, alpha—particles and heavier nuclei) and some part of secondary CR (nuclear active particles, mostly protons and neutrons) are important for the generation of stable and unstable cosmogenic nuclides in the atmosphere, in the oceans and underground (Chapters 10 and 17). Charged secondary particles such as protons, positive and negative pions, positive and negative muons, positrons and electrons (including re-entrant and splash albedo particles, see below Section 2.12) are important for the ionization of air and chemical processes in the atmosphere (particularly, formation of nitrates and influence on ozone layer — see Chapter 13). Ionization of air by primary and secondary charged CR particles is responsible for the effects of CR on ionosphere and radio wave propagation, for disruptions in radio communications during great solar flare events (Chapter 12). The ionization of air at altitudes higher than a few km caused by primary and secondary charged CR particles affects cloud formation as well, leading to long-term variation in global cloudiness, and consequently to global climate changes (Chapter 14).
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Aglietta M., B. Alpat, E.D. Alyea, et al. “Neutrino-induced and atmospheric single-muon fluxes measured over 5 decades of intensity by LVD at Gran-Sasso-Laboratory”, Astropart. Phys., 3 (4), 311–320 (1995).
Agrawal V., T.K. Gaisser, P. Lipari, and T. Stanev “Atmospheric neutrino flux above 1 GeV”, Phys.Rev., D53, 1314–1323, (1996).
Akhmedov E.Kh. and O.V. Bychuk “Resonant spin-flavor precession of neutrinos and the solar neutrino problem”, Zh. Éksp. Teor. Fiz. 95, 442–457 (1989).
Ambrosio M., R. Antolini, G. Auriemma, et al. “Vertical muon intensity measured with MACRO at the Gran Sasso laboratory”, Phys. Rev., D52, 3793–3802 (1995).
Andreev Yu.M., V.I. Gurentsov, and I.M. Kogai “Muon intensity from the Baksan underground scintillation telescope”, Proc. 20th Intern. Cosmic Ray Conf., Moscow, 6, 200–203 (1987).
Appleton I.C., M.T. Hogue, and B.C. Rastin “A study of the muon momentum spectrum and positive-negative ratio at sea-level”, Nucl. Phys., B26, No. 2, 365–389 (1971).
Bahcall J.N., M.H. Pinsonneault, and S. Basu “Solar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological Properties”, Astrophys. J., 555, 990–1012 (2001).
Bahcall J.N. and W.N. Press “Solar-cycle modulation of event rates in the chlorine solar neutrino experiment”, Astrophys. J., 370, 730–742 (1991).
Battistoni G. “A 3-D calculation of the atmospheric neutrino fluxes”, Astropart. Phys., 12, 315–333 (2000).
Battistoni G., A. Ferrari, T. Montaroli, and P. Sala “Improvements in the FLUKA calculations of the atmospheric neutrino fluxes”, Proc. 27th Intern. Cosmic Ray Conf., Hamburg, 3, 1166 (2001).
Baxendale J.M., C.J. Hume, and M.J. Thompson “Precise measurement of sea level muon charge ratio”, J. Phys., G1, No. 7, 781–788 (1975).
Bazilevskaya G.A., D.Sc. Thesis, Physical Lebedev Institute, Moscow (1985).
Bazilevskaya G.A., D.N. Korolkov, M.B. Krainev, A.K. Svirzhevskaya, and N.S. Svirzhevsky “On the angular distribution of cosmic ray intensity in the Earth ’s atmosphere”, Proc. 25th Intern. Cosmic Ray Conf., Durban, 7, 321–324 (1997).
Bazilevskaya G.A. and V.S. Makhmutov “The electron precipitation into the atmosphere according to cosmic ray experiment in the stratosphere”, Izvestia Academy of Sciences USSR, Series Phys., 63, No. 8, 1670–1674 (1999).
Bazilevskaya G.A., A.M. Mukhamedzhanov, S.I. Nikolsky, Yu.I. Stozhkov, and T.N. Carakhchy’an “Cosmic rays and the neutrino flux in the Davis ’ experiment”, Soy. J. Nucl. Phys., 39, 543–550 (1984).
Berezinsky V. “Solar neutrino as highlight of Astroparticle Physics”, Proc. 25th Intern. Cosmic Ray Conf., Durban, 8, 59–79 (1997).
Berger Ch., M. Fröhlich, H. Mönch, et al. “Experimental study of muon bundles observed in the Fréjus detector”, Phys. Rev., D40, No. 7, 2163–2171 (1989).
Bleeker J.A.M., J.J. Burger, A. Scheepmaker, B.N. Swanenburg, and Y. Tanaka “A balloon observation of high energy electrons”, Proc. 9th Intern. Cosmic Ray Conf., London, 1, 327–329 (1965).
Bollinger L.M., Bull. Amer. Phys. Soc., 25, No. 3, 16 (1950).
Bower C.R., A.S. Beach, J.J. Beatty, et al. “The HEAT-pbar Cosmic Ray Antiproton Experiment”, Proc. 26th Intern. Cosmic Ray Conf., Salt Lake Sity, 5, 13–16 (1999).
Briesmeister J.F. “MNCP — A general Monte Carlo N-particle transport code version 4A”, LA-12625-M, pp. 693, Los Alamos Nat. Lab., Los Alamos, N.M. (1993).
Brun B. et al. “GEANT3 User ’s guide”, Rep. DD/EE/84–1, pp 584, Eur. Org. for Nucl. Res., Geneva (1987).
Bucik R., A. Dmitriev, K. Kudela, and S. Ryumin “Gamma-radiation of the Earth ’s atmosphere from the CORONAS-I data”, Proc. 26th Intern. Cosmic Ray Conf., Salt-Lake City, 7, 433–436 (1999).
Bykov A.A., V.Yu. Popov, A.I. Rez, V.B. Semikoz, and D.D. Sokoloff “Aperiodic spin-flavor conversions and electron-antineutrino from the Sun with random magnetic field”, Proc. of EU-Conference New Trends in Neutrino Physics, Ringberg Castle, Germany, 24–29 May 1998, World Scientific Publishing Company, 201–210 (1998).
Castagnoli G.C. and D. Lal “Solar modulation effects in terrestrial production of carbon 14”, Radiocarbon, 22, 133–158 (1980).
Clay J., C.G. Hooft, L.J. Dey, and J.T. Wiersma “An experimental test of the Super Nova hypothesis. Intensity of Cosmic rays in the Earth Crust”, Physica, 4, No. 2, 121–137 (1937).
Clay J. and A. Van Gemnert “Decrease of the intensity of cosmic rays in the earth down to 1380 m waterequivalent”, Physica, 6, No. 6, 497–510 (1939a).
Clay J. and A.G.M. Van Gemert “Absorption of the hard cosmic rays in different materials”, Physica, 6, No. 7, 649–655 (1939b).
Cleveland B.T., T. Daily, R.Jr. Davis, J.R. Distel, K. Lande, C.K. Lee, P.S. Wildenhain, J. Ullman “Measurement of the solar electron neutrino flux with the Homestake chlorine detector”, Astrophys. J., 496, No 1, pt.1, 505–526 (1998).
Cousins J.E., W.F. Nash, and A.J. Pointon “The Effect of the Angular Variation of the Intensity on Scattering Distribution of µ-Mesons Underground at a Depth of 40 m w.e.”, Il Nuovo Cimento, 6, 1113–1121 (1957).
Crouch M. “An improved world survey expression for cosmic ray vertical intensity vs. depth in standard rock”, Proc. 20th Intern. Cosmic Ray Conf., Moscow, 6, 165–168 (1987).
Daniel R.R. and S.A. Stephens “Cosmic ray produced electrons and gamma rays in the atmosphere”, Rev. Geophys. Space Sci., 12, No. 2, 233–258 (1974).
Davis R. Jr. “A half-century with solar neutrinos”. Nobel Lecture in Physics, 1–21 (2002)
Davis R Jr, A.K. Mann, L. Wolfenstein “Solar neutrinos”, Annu. Rev. Nucl. Part. Sci., 39, 467–506 (1989).
De Nolfo G.A., S.W. Barwick, J.J. Beatty et al. “Secondary and re-entrant albedo electrons in the atmosphere”, Proc. 25th Intern. Cosmic Ray Conf., Durbin, 2, 373–376 (1997).
Desorgher L., E.O. Flückiger, M.R. Moser, and R. Bütikofer “Geant Simulation of the Propagation of Cosmic Rays through the Earth ’s Atmosphere”, Proc. 28th Intern. Cosmic Ray Conf., Tsukuba, 7, 4277–4280 (2003).
Dorman L.I. “Solar-Neutrino Variations: A Manifestation of Nonzero Neutrino Mass and Magnetic Moment, and Mixing”, Physics ofAtomic Nuclei, 63, No. 6, 984–988 (2000a).
Dorman L.I. “The Asymmetry of Solar-Neutrino Fluxes” Physics of Atomic Nuclei, 63, No. 6, 989–992 (2000b).
Dorman L.I., V.L. Dorman, and A.W. Wolfendale “North-South asymmetry in solar neutrino fluxes and in correlation coefficients”, Proc. 23th Intern. Cosmic Ray Conf.. Calgary, 4. 873–876 (1993).
Dorman L.I., V.L. Dorman, and A.W. Wolfendale “The solar cycle variations of solar neutrino flux and heliolatitude anisotropy”, Proc. 24th Intern. Cosmic Ray Conf., Rome, 4, 1239–1242 (1995).
Dorman L.I. and A.W. Wolfendale “The correlation of the solar neutrino rate with solar activity”, J. Phys. G: Nucl. Part. Phys., 17, 769–778 (1991a).
Dorman L.I. and A.W. Wolfendale “Solar neutrino rate and solar activity”, Geophys. Astrophys. Fluid Dynamics, 62, 173–182 (1991b).
Dorman L.I. and A.W. Wolfendale “Relationship between the solar neutrino counting rate in the Homestake experiment, solar activity, cosmic ray intensity and the Earth ’s heliolatitude”, Proc.22th Intern. Cosmic Ray Conf., Dublin, 3, 736–739 (1991c).
Dorman L.I. and A.W. Wolfendale “The solar neutrino problem: connection with elementary particle physics and the physics of the solar interior”, Proc.22th Intern. Cosmic Ray Conf., Dublin, 3, 740–743 (1991d).
DuVernois M.A., A.S. Beach, J.J. Beatty et al. “Splash and reentrant albedo observations of electrons and positrons at a 4.2 GV vertical magnetic cutoff”, Proc. 27th Intern. Cosmic Ray Conf., Hamburg, 10, 4003–4006 (2001a).
DuVernois M.A., J.J. Beatty, C. Bower et al. “Absolute rigidity spectra of protons and helium from 16 to 250 GV”, Proc. 27th Intern. Cosmic Ray Conf., Hamburg, 5, 1618–1621 (2001b).
Ehmert A. “Die Absorptionkurve der harten component der kosmichen ultrasrahlung”, Zs. Phys., 106, No. 11–12. 751–772 (1937).
Engel R., T.K. Gaisser, and T. Stanev “The flux of atmospheric muons”, Proc. 27th Intern. Cosmic Ray Conf., Hamburg, 3, 1029–1032 (2001).
Follet D.H. and I.D. Crawskaw “Cosmic ray measurements under thirty meters of clay”, Proc. Roy. Soc., A155, 546–558 (1936).
Gaisser T.K. and T. Stanev “Cosmic Rays”, Phys. Rev., D54, No. 1, 122–127 (1996).
Gavryusev V., J. Provost, E. Gavryuseva, and G. Berthomieu “The Spectrum of Gravity Modes as a Function of the Solar Structure — Model with a Mixed Core”, Sol. Phys., 133, 139–161 (1991).
George E.P. “Observations of cosmic rays underground and their interpretation”, in Progress in Cosmic Ray Physics, ed. By J.G. Wilson, North Holland Publ. Co., Amsterdam, 1, 395–454 (1952).
Golenkov A.E., A.K. Svirzhevskaya, N.S. Svirzhevsky, and Yu.I. Stozhkov “Cosmic ray latitude survey in the stratosphere during the 1987 solar minimum”, Proc. 21st Intern. Cosmic Ray Conf., Adelaida, 7, 14–17 (1990).
Gonzales W.D., B.T. Tsurutani, P.S. McIntosh, and A.L. Clua de Gonzalez “Coronal hole-active regioncurrent sheet (CHARCS) association with intense interplanetary and geomagnetic activity”, Geophys. Res. Lett., 23, No. 19, 2577–2580 (1996).
Hansen P., M. Ambriola, S. Bartalucci, et al. “A new measurement of muon spectra in the atmosphere”, Proc. 27th Intern. Cosmic Ray Conf., Hamburg, 3, 921–924 (2001).
Hebbeker T. and C. Timmermans, Preprint hep-ph/0102042 (2001).
Hirata K.S., T. Kajita, M. Koshiba et al. “Observation of a neutrino burst from the supernova SN 1987A”, Phys. Rev. Lett., 58, No. 14, 1490–1493 (1987).
Hirata K.S., T. Kajita, M. Koshiba et al. “Experimental-study of the atmospheric neutrino flux”, Phys. Lett., B 205, No. 2–3, 416–420 (1988).
Hirata K.S., T. Kajita, K. Kifune et al. “Observation of 8B-solar neutrinos in the Kamiokande-II detector”, Phys. Rev. Lett., 63, No. 1, 16–19 (1989).
Honda M., T. Kajita, K. Kasahara, and S. Midorikawa “Calculation of the flux of atmospheric neutrinos”, Phys. Rev. D52, 4985–5005 (1995).
Hovestadt D. and P. Meyer “The geomagnetic cut-off at Ft. Churchill and the primary cosmic ray electron spectrum from 10 MeV to 12 GeV in 1968”, Acta Phys. Acad. Scient. Hungaricae, 29, suppl. 2, 525–531 (1970).
Israel M.H. “Cosmic-Ray Electrons between 12 MeV and 1 GeV in 1967”, J. Geophys. Res., 74, No. 19, 4701–4713 (1969).
Kajita T. “Muons and neutrinos”, Proc. 27th Intern. Cosmic Ray Conf., Hamburg, Vol. Invited, Rapporteur, and Highlight Papers, 194–205 (2001).
Kasahara K., E. Mochizuki, S. Torii, et al. “Atmospheric gamma-ray observations with BETS for calibrating atmospheric neutrino flux calculations”, Proc. 27th Intern. Cosmic Ray Conf., Hamburg, 3, 966–969 (2001).
Kolhörster W. “Intensitates und Richtungsmessungen der durchdringenden Strahlung”, Berl. Ber., 24, 366–377 (1923).
Kolhörster W. “The Hardest Cosmic Rays and the Electric Charge of the Earth”, Nature, 132, No. 3332, 407–407 (1933).
Koshiba M. “Observational Neutrino Astrophysics”, Phys. Rep., 220, No. 5–6, 229–381 (1992).
Koshiba M. “Birth of Neutrino Astrophysics”, Nobel Lecture in Physics, 1–15 (2002).
Letaw J.R., G.H. Share, R.L. Kinzer, R. Silberberg, and E.L. Chupp “Satellite observation of atmospheric nuclear gamma radiation”, J. Geophys. Res., 94, 1211–1221 (1989).
Ling J.C. “A semiempirical model for atmospheric gamma rays from 0.3 to 10 MeV at a geomagnetic latitude of 400”, J. Geophys. Res., 80, 3241–3252 (1975).
Lingenfelter R.E. “Production of carbon 14 by cosmic ray neutrons”, Reviews of Geophysics, 1, No. 1, 35–55 (1963)
Mahoney W.A., J.C. Ling, and A.S. Jacobson “HEAO 3 measurements of the atmospheric positron annihilation line”, J. Geophys. Res., 86, 11098–11104 (1981).
Makhmutov V.S., G.A. Bazilevskaya, A.I. Podgorny, Yu.I. Stozhkov, and N.S. Svirzhevsky “The precipitation of electrons into the Earth ’s atmosphere during 1994”, Proc. 24th Intern. Cosmic Ray Conf., Rome, 4, 1114–1117 (1995).
Makhmutov V.S., G.A. Bazilevskaya, and M.B. Krainev “Characteristics of energetic electron precipitation into the Earth ’s polar atmosphere and geomagnetic conditions”, Adv. Space. Res. 2001a (in press).
Makhmutov V.S., G.A. Bazilevskaya, M. B. Krainev, and M. Storini “Long-term cosmic ray experiment in the atmosphere: energetic electron precipitation events during 20–23 solar activity cycles”, Proc. 27th Intern. Cosmic Ray Conf., Hamburg, 10, 4196–4199 (2001b).
Makhmutov V.S., G.A. Bazilevskaya, M.B. Krainev, Y.I. Stozhkov, A.K. Svirzhevskaya, N.S. Svirzhevsky, S.Y. Malin “Semiannual variation in the number of energetic electron precipitation events recorded in the polar atmosphere”, Proc. 28th Intern. Cosmic Ray Conf., Tsukuba, 7, 4233–4236 (2003).
Masarik J. and J. Beer “Simulation of particle fluxes and cosmogenic nuclide production in the Earth ’s atmosphere”, J. Geophys. Res., 104, No. D10, 12099–12111 (1999).
Massetti S. “Is there a North-South asymmetry in the Homestake neutrino data connected with solar activity?”, Proc. 24th Intern. Cosmic Ray Conf., Rome. 4. 1251–1254 (1995)
Massetti S., M. Storini, and N. Lucci “Summary of correlative analyses between Homestake neutrino data and related to solar activity”, Proc. 24th Intern. Cosmic Ray Conf., Rome, 4, 1243–1247 (1995).
Menon M., P.V. Ramanamurthy, B.V. Sreekantan, and S. Miyake “Cosmic Ray Intensity at Great Depth and Neutrino experiments”, Nuovo Cimento, 30, No. 5, 5766–5777 (1963).
Mikheyev S.P. and A.Yu. Smirnov “Resonance enhancement of oscillations in matter and solar neutrino spectroscopy”, Soy. J. Nucl. Phys. 42, No. 6, 1441–1448 (1985).
Mikheyev S.P. and A.Yu. Smirnov “Resonant amplification of v oscillations in matter and solar-neutrino spectroscopy”, Nuovo Cimento, 9C, Ser. 1, No 1. 17–26 (1986).
Millikan R.A. “High Frequency Rays of Cosmic Origin”, Nature, 116, No.2927, 823–826 (1925).
Millikan R.A. and G.H. Cameron “High Frequency Rays of Cosmic Origin III. Measurements in Snow-Fed Lakes at High Altitudes”, Phys. Rev., 28. No. 5. 851–868 (1926).
Millikan R.A. and G.H. Cameron “New Precision in Cosmic Ray Measurements; Yielding Extension of Spectrum and Indications of Bands”, Phys. Rev., 31, No. 6, 921–930 (1928).
Millikan R.A. and G.H. Cameron “A More Accurate and More Extended Cosmic-ray Ionization-Depth Curve, and the Present Evidence for Atom-Building”, Phys. Rev., 37, No. 3, 235–252 (1931).
Motoki M., T. Sanuki, S. Orito, et al. “Precise measurement of atmospheric muon fluxes at sea level”, Proc. 27th Intern. Cosmic Ray Conf.. Hamburg 3, 927–930 (2001)
Myssowsky L. and L. Tuwim “Versuche uber die Absorption der Hohenstrahlung im Wasser”, Ztschr. Phys., 35, No. 4, 299–305 (1925).
Nandi B.C. and M. Sinha “Charge ratio of muons at sea level in range 5–600 GeV/c”, Nucl. Phys., B40, No. 1, 289–297 (1972)
Oakley D.S., H.B. Snodgrass, R.K. Ulrich, and T.L. VanDeKop “On the correlation of solar surface magnetic flux with solar neutrino capture rate”. Astrophys. Lett., 437, L63–L66 (1994)
Oakley D.S. and H.B. Snodgrass “Correlation Studies of Solar Magnetic with Solar Neutrino Flux”, Bull. Am. Phys. Soc., 40, No. 7, 1511 (1995).
Oakley D.S. and H.B. Snodgrass, Technical Progress Report No. 65, University of Colorado Nuclear Physics Laboratory (1996).
Oakley D.S. and H.B. Snodgrass “Interactions between solar neutrinos and solar magnetic fields”, Astropart. Phys., 7, No. 4, 297–306 (1997).
Ramaty R., B. Kozlovsky, and R.E. Lingenfelter “Nuclear Gamma Rays from Energetic Particle Interactions”, Astrophys. J. Suppl., 40,487–495 (1979).
Randell C.A. and W.E. Hazen “The ratio of electrons to mesons 1100 feet underground”, Phys. Rev., 81, No. 1, 144–145 (1951).
Rastin B.C. “A study of the muon charge ratio at sea level within the momentum range 4 to 2000 GeV/c”, J. Phys., G10, No. 11, 1629–1638 (1984).
Raychaudhuri P. “Time variations in Kamiokande solar neutrino data”, Mod. Phys. Lett., A6, No.22, 2003–2007 (1991).
Reedy R.C. “Nuclide production by primary-ray protons”, J Geophys. Res., 92, Sunni.. E697–E702, 1987.
Reedy R.C. and J. Masarik “Cosmogenic-nuclide depth profiles in the lunar surface”, Lunar Planet. Sci, 25, 1119–1120 (1994).
Reeves G.D. “Relativistic electrons and magnetic storms: 1992–1995”, Geoph. Res. Lett., 25, No. 11, 1817–1820 (1998).
Regener E. “Spectrum of cosmic rays”, Nature, 127, 233–234 (1931).
Rivin Yu.R. “Temporal variations in the flux of high-energy solar neutrinos based on data from the detector in South Dakota”, Astron. Reports, 37, 202–208 (1993).
Rivin Yu.R. and V.N. Obridko “Cyclic variation of the high-energy solar neutrino flux”, Astron. Reports, 41, 76–84 (1997).
Rockstroh J. and W.R. Webber “A measurement of the spectrum of cosmic ray electrons between 20 Me V and 3 GeV in 1968 — Further evidence for extensive time variations of this component”, J. Geophys. Res., 74, No. 21, 5041–5053 (1969).
Sanuki T., Y. Yamamoto, M. Motoki, et al. “Atmospheric muons at various altitudes”, Proc. 2/th Intern. Cosmic Ray Conf., Hamburg, 3, 950–953 (2001).
Schmoker J.W. and J.A. Earl “Magnetic-Cloud-Chamber Observations of Low Energy Cosmic-Ray Electrons”, Phys. Rev., 138, No. 1B, B300–B302 (1965)
Share G.H., R.J. Murphy, and E. Rieger “Atmospheric gamma-ray lines produced by cosmic rays and solar energetic particles”, Proc 26th Intern. Cosmic Ray Conf., Salt-Lake City, 7, 329–332 (1999).
Shea M.A., D.F. Smart, and L.C. Gentile “Estimating cosmic ray vertical cutoff rigidities as a function of the Mcllwain L-parameter for different epochs of the geomagnetic field”, Phys. of the Earth and Planet. Interiors, 48, 200–205 (1987).
Snodgrass H.B. and D.S. Oakley “Comment on Absence of Correlation between the Solar Neutrino Flux and the Sunspot Number”, Phys. Rev. Letters, 83, No. 9, 1894 (1999)
Sreekantan B.V., S. Naranan, and P.V. Ramanamurthy “On the angular distribution of penetrating cosmic-ray particles at a depth 103 mwe below ground”, Proc. Indian Academy of Sciences, Ser. A, 43, No. 2, 113–129 (1956).
Stephens S.A. “Atmospheric electron spectrum over Hyderabad and a study of re-entrant albedo electrons”, Acta Phys. Acad. Scient. Hungaricae, 29, suppl. 2, 727–732 (1970)
Stozhkov Y.I., N.S. Svirzhevsky, and V.S. Makhmutov “Cosmic ray measurements in the atmosphere”, Preprint No. 8, FIAN, Moscow, 1–21, 2001.
Sturrock P.A., G. Walther and M.S. Wheatland “Apparent Latitudinal Modulation of the Solar Neutrino Flux”, Astrophys. J., 507, 978–983 (1998).
Tsuji S., K. Himei, T. Katayama, et al. “Atmospheric muon measurements I: Vertical measurements”, Proc. 27th Intern. Cosmic Ray Conf., Hamburg, 3, 931–934 (2001).
Vannuccini E., Grimani C., Papini P., and Stephens S.A. “The Secondary Proton Spectrum at Small Atmospheric Depths”, Proc. 28th Intern. Cosmic Ray Conf., Tsukuba, 7, 4287–4290 (2003)
Verma S.D. “Measurement of the charged splash and re-entrant albedo of the cosmic radiation”, J. Geophys. Res., 72, No.3, 915–925 (1967).
Verma S.D. and S.P. Bhatnagar “Observation of Energy Spectrum of Electron Albedo in Low Latitude Region at Hyderabad, India”, Proc. 19th Intern. Cosmic Ray Conf., La Jolla, 5, 316–319 (1985).
Walther G. “On the Solar-Cycle Modulation of the Homestake Solar Neutrino Capture Rate and the Shuffle Test”, Astrophys. J. 513, 990–996 (1999).
Willett J.B. and W.A. Mahoney “High spectral resolution measurement of gamma ray lines from the earth ’s atmosphere”, J. Geophys. Res., 97, 131–139(1992).
Wilson V.C. “Cosmic-Ray Intensities at Great Depths”, Phys. Rev., 53, No. 5, 337–343 (1938a).
Wilson V.C. “On the Nature of the Penetrating Cosmic Rays”, Phys. Rev., 53, No. 11, 908–909 (1938b).
Wolfenstein L. “Neutrino oscillations in matter”, Phys. Rev. D17, 2369–2374 (1978).
Zanini A., C. Ongaro, E. Durisi, L. Visca, S. DeAgostini, F. Fasolo, M. Pelliccioni, and O. Saavedra “Differential Neutron Flux in Atmosphere at Various Geophysical Conditions”, Proc. 28th Intern. Cosmic Ray Conf., Tsukuba, 7, 4291–4294 (2003)
Author information
Authors and Affiliations
Rights and permissions
Copyright information
© 2004 Springer Science+Business Media New York
About this chapter
Cite this chapter
Dorman, L.I. (2004). Secondary Cosmic Rays Underground and in the Atmosphere. In: Cosmic Rays in the Earth’s Atmosphere and Underground. Astrophysics and Space Science Library, vol 303. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-2113-8_2
Download citation
DOI: https://doi.org/10.1007/978-1-4020-2113-8_2
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-015-6987-3
Online ISBN: 978-1-4020-2113-8
eBook Packages: Springer Book Archive