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1

Dorman, Lev I. Cosmic Ray Interactions, Propagation, and Acceleration in Space Plasmas. Dordrecht: Springer Netherlands, 2006. http://dx.doi.org/10.1007/1-4020-5101-8.

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2

International, Symposium on Very High Energy Cosmic Ray Interactions (9th 1996 Karlsruhe Germany). Very High Energy Cosmic Ray Interactions: Proceedings of the 9th International Symposium on Very High Energy Cosmic Ray Interactions, Karlsruhe, Germany, 19-23 August 1996. [Netherlands]: North-Holland, 1997.

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3

France) International Symposium on Very High Energy Cosmic Ray Interactions (15th 2008 Paris. Very high energy cosmic ray interactions: Proceedings of the XV International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI 2008) : Paris, France, 1-6 September 2008. Amsterdam: Elsevier, 2008.

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4

International Symposium on Very High Cosmic Ray Interactions (10th 1998 Laboratori Nazionali del Gran Sasso, Assergi, Italy). Very high energy cosmic ray interactions: Proceedings of the 10th International Symposium on Very High Energy Cosmic Ray Interactions, Laboratori Nazionali del Gran Sasso, Assergi, Italy, 12-17 July 1998. [Amsterdam]: North-Holland, 1999.

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5

Guzik, T. Gregory. [The systematic interpretation of cosmic ray data (the transport project)]. [Washington, DC: National Aeronautics and Space Administration, 1997.

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6

Cucinotta, Francis A. Description of alpha-nucleus interaction cross sections for cosmic ray shielding studies. Hampton, Va: Langley Research Center, 1993.

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7

International Symposium on Very High Energy Cosmic Ray Interactions (11th 2000 Campinas, São Paulo, Brazil). Very high energy cosmic ray interactions: Proceedings of the 11th International Symposium on Very High Energy Cosmic Ray Interactions : 'Gleb Wataghin' Institute of Physics, State University of Campinas, Campinas, Brazil, 17-21 July 2000. [Amsterdam, Netherlands]: North-Holland, 2001.

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8

Abunina, Maria, Rolf Bütikofer, Karl-Ludwig Klein, Olga Kryakunova, Monica Laurenza, David Ruffolo, Danislav Sapundjiev, Christian T. Steigies, and Ilya Usoskin, eds. NMDB@Home 2020. Kiel: Universitätsverlag Kiel | Kiel University Publishing, 2021. http://dx.doi.org/10.38072/2748-3150/v1.

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With the 'Proceedings of the 1st virtual symposium on cosmic ray studies with neutron detectors' launches the new open access series 'Cosmic ray studies with neutron detectors'. The volume comprises the papers presented at the online meeting held in July 2020. The contributions show that neutron detectors on the ground provide significant results for studying the interaction of galactic cosmic rays with magnetic fields in the heliosphere, for accelerating energetic particles, and for a growing number of applications, including geophysics and space weather. The easily accessible databases around the project 'Real-Time database for high resolution Neutron Monitor measurements' (NMDB) make the original data readily available to a large user community.
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9

Murzin, V. S. Fizika adronnykh prot͡s︡essov. Moskva: Ėnergoatomizdat, 1986.

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10

A search for muon neutrino to electron neutrino oscillations in the MINOS experiment. New York: Springer, 2011.

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11

Cucinotta, Francis A. Energy-loss cross sections for inclusive charge-exchange reactions at intermediate energies. Hampton, Va: Langley Research Center, 1993.

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12

Cucinotta, Francis A. Abrasion-ablation model for neutron production in heavy ion reactions. Hampton, Va: Langley Research Center, 1995.

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13

Jones, Lawrence. Very High Energy Cosmic Ray Interactions VIIth International Symposium. American Institute of Physics, 1993.

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14

Cosmic Ray Interactions, Propagation, and Acceleration in Space Plasmas. Springer, 2006.

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15

1925-, Jones Lawrence W., and American Institute of Physics, eds. Very high energy cosmic-ray interactions: VIIth International Symposium, Ann Arbor, MI, June 21-27, 1992. New York: American Institute of Physics, 1993.

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16

W, Townsend Lawrence, Wilson J. W, and United States. National Aeronautics and Space Administration. Scientific and Technical Information Program., eds. Description of alpha-nucleus interaction cross sections for cosmic ray shielding studies. [Washington, DC]: National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Program, 1993.

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17

W, Townsend Lawrence, Wilson J. W, and United States. National Aeronautics and Space Administration. Scientific and Technical Information Program., eds. Description of alpha-nucleus interaction cross sections for cosmic ray shielding studies. [Washington, DC]: National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Program, 1993.

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18

W, Townsend Lawrence, Wilson J. W, and United States. National Aeronautics and Space Administration. Scientific and Technical Information Program., eds. Description of alpha-nucleus interaction cross sections for cosmic ray shielding studies. [Washington, DC]: National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Program, 1993.

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19

Skobel'tsyn, D. V. Cosmic Rays and Nuclear Interactions at High Energies. Springer, 2012.

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20

F, Burlaga L., and Goddard Space Flight Center, eds. Cosmic ray modulation and turbulent interaction regions near 11 AU. Greenbelt, MD: National Aeronautics and Space Administration, Goddard Space Flight Center, 1985.

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21

Sano, Hidetoshi. Shock-Cloud Interaction in RX J1713.7-3946: Evidence for Cosmic-Ray Acceleration in the Young VHE γ-ray Supernova Remnant. Springer, 2016.

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22

Ochoa-Ricoux, Juan Pedro. A Search for Muon Neutrino to Electron Neutrino Oscillations in the MINOS Experiment. Springer, 2011.

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23

Ochoa-Ricoux, Juan Pedro. A Search for Muon Neutrino to Electron Neutrino Oscillations in the MINOS Experiment. Springer, 2013.

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24

Sano, Hidetoshi. Shock-Cloud Interaction in RX J1713.7−3946: Evidence for Cosmic-Ray Acceleration in the Young VHE γ-ray Supernova Remnant. Springer, 2018.

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25

George C. Marshall Space Flight Center., ed. Spectra, composition and interactions of nuclei above 10 TeV using magnet-interferometric chambers (SCIN/MAGIC): Final technical report. Huntsville, AL: National Aeronautics and Space Administration, George C. Marshall Space Flight Center, 1991.

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26

W, Townsend Lawrence, Dubey Rajendra R, and United States. National Aeronautics and Space Administration. Scientific and Technical Information Program., eds. Energy-loss cross sections for inclusive charge-exchange reactions at intermediate energies. [Washington, DC]: National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Program, 1993.

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27

W, Townsend Lawrence, Dubey Rajendra R, and United States. National Aeronautics and Space Administration. Scientific and Technical Information Program., eds. Energy-loss cross sections for inclusive charge-exchange reactions at intermediate energies. [Washington, DC]: National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Program, 1993.

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28

W, Townsend Lawrence, Dubey Rajendra R, and United States. National Aeronautics and Space Administration. Scientific and Technical Information Program., eds. Energy-loss cross sections for inclusive charge-exchange reactions at intermediate energies. [Washington, DC]: National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Program, 1993.

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29

Energy-loss cross sections for inclusive charge-exchange reactions at intermediate energies. [Washington, DC]: National Aeronautics and Space Administration, Office of Management, Scientific and Technical Information Program, 1993.

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30

Ellam, Rob. 2. Isotopic clocks. Oxford University Press, 2016. http://dx.doi.org/10.1093/actrade/9780198723622.003.0002.

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About one in a trillion atoms of carbon is the radioactive isotope 14C. It is a ‘cosmogenic isotope’ produced by the interaction between atmospheric nitrogen (N) and cosmic rays. The half-life of 14C is 5,730 years, so every 5,730 years the ratio of 14C to 12C will halve. ‘Isotopic clocks: the persistence of carbon’ describes how scientists Willard Libby, Hessel de Vries, Hans Seuss, and their contemporaries established the radiocarbon dating technique. Radiocarbon has become one of the most valuable isotopic tools available to scientists looking to date materials formed over the past 50,000 years or to trace and apportion different sources of carbon.
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31

1940-, Wilson John W., Townsend Lawrence W, and Langley Research Center, eds. Abrasion-ablation model for neutron production in heavy ion reactions. Hampton, Va: National Aeronautics and Space Administration, Langley Research Center, 1995.

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32

1940-, Wilson John W., Townsend Lawrence W, and Langley Research Center, eds. Abrasion-ablation model for neutron production in heavy ion reactions. Hampton, Va: National Aeronautics and Space Administration, Langley Research Center, 1995.

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33

Kennel, Charles F. Convection and Substorms. Oxford University Press, 1996. http://dx.doi.org/10.1093/oso/9780195085297.001.0001.

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The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae. The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions. The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for studying this vital region. Charles F. Kennel, a leading scientist in the field, here presents a synthesis of the convection and substorm literatures, and an analysis of convection and substorm interactions; he also suggests that the currently accepted steady reconnection model may be advantageously replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur. Written in an accessible, non-mathematical style, this book introduces the reader to the exciting discoveries in this fast-growing field.
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34

1940-, Wilson John W., Townsend Lawrence W, and Langley Research Center, eds. Abrasion-ablation model for neutron production in heavy ion reactions. Hampton, Va: National Aeronautics and Space Administration, Langley Research Center, 1995.

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35

1940-, Wilson John W., Townsend Lawrence W, and Langley Research Center, eds. Abrasion-ablation model for neutron production in heavy ion reactions. Hampton, Va: National Aeronautics and Space Administration, Langley Research Center, 1995.

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36

1940-, Wilson John W., Norbury John W, and Langley Research Center, eds. Parameterizations of pion energy spectrum in nucleon-nucleon collisions. Hampton, Va: National Aeronautics and Space Administration, Langley Research Center, 1998.

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37

1940-, Wilson John W., Norbury John W, and Langley Research Center, eds. Parameterizations of pion energy spectrum in nucleon-nucleon collisions. Hampton, Va: National Aeronautics and Space Administration, Langley Research Center, 1998.

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