Cosmic Rays and Nuclear Interactions at High Energies

Herausgegeben:Skobel tsyn, D. V.

• Broschiertes Buch

Produktbeschreibung

Apparatus and Method of Investigating Multiple Production at Energies of Hundreds of GeV.- Method of Treatment of Experimental Data Obtained with Cloud Chamber.- Experimental Data on Inelastic Strong Interaction at Energies of 100¿3000 GeV and Their Interpretation.- Extensive Air Showers and Interaction of Particles with Energies above 1013 eV.- Apparatus for Investigation of Extensive Air Showers and Nuclear Interactions of Cosmic-Ray Particles with Energy 1012¿1016 eV.- Quasi-nucleonic Nuclear Interactions of 23-GeV Protons in a Nuclear Emulsion Irradiated in a Pulsed Magnetic Field of 180 kOe.- Measurement of Energy of Electron ¿ Photon Cascades by Photometry of Spots on X-Ray Films.- Transition Effects in the Ionization Calorimeter.- Investigation of the Nuclear Component of Cosmic Rays in a Period of Minimum Solar Activity.

Produktdetails

• The Lebedev Physics Institute Series 46
• Verlag: Springer / Springer US / Springer, Berlin
• 1971
• Seitenzahl: 236
• Erscheinungstermin: 8. Oktober 2012
• Englisch
• Abmessung: 279mm x 210mm x 13mm
• Gewicht: 586g
• ISBN-13: 9781475700602
• ISBN-10: 1475700601
• Artikelnr.: 41322372

Inhaltsangabe

Apparatus and Method of Investigating Multiple Production at Energies of Hundreds of GeV.- Method of Treatment of Experimental Data Obtained with Cloud Chamber.- Experimental Data on Inelastic Strong Interaction at Energies of 100 3000 GeV and Their Interpretation.- Extensive Air Showers and Interaction of Particles with Energies above 1013 eV.- Apparatus for Investigation of Extensive Air Showers and Nuclear Interactions of Cosmic-Ray Particles with Energy 1012 1016 eV.- Quasi-nucleonic Nuclear Interactions of 23-GeV Protons in a Nuclear Emulsion Irradiated in a Pulsed Magnetic Field of 180 kOe.- Measurement of Energy of Electron Photon Cascades by Photometry of Spots on X-Ray Films.- Transition Effects in the Ionization Calorimeter.- Investigation of the Nuclear Component of Cosmic Rays in a Period of Minimum Solar Activity.