PPT-100 years since the discovery of Cosmic Rays. A brief histo

Andrea Chiavassa Universita degli Studi di Torino Carpathian Summer School of Physics 2012 June 24 July 7 Sinaia Romania Most of the material comes from the book . Noda and Y Kamide Supervised by Y Muraki brPage 2br Have you ever had an Xray examination at the hospital In 1896 a German physicist W C R57590ntgen astonished people with an image of bones captured through the use of Xrays He had just discovered th Koji Mukai. NASA/GSFC/CRESST and UMBC. How RXTE matches up with WDs. Luminosity: up to ~a few x 10. 34. erg s. -1. for symbiotic stars, ~a few x 10. 33. erg s. -1. for typical intermediate . polars. Douglas Bergman. University of Utah. Cosmic Rays – LHC Workshop, ECT* Trento. 2 December 2010. The Final Word (almost). HiRes Collaboration. J. Boyer, B. Connolly, C.B. Finley, B. Knapp, E.J. . Mannel. The Future of Cosmic Ray Research. .. 8 The Future of Cosmic Ray Research . As we have seen, a few cosmic rays can be detected with energies somewhat . greater . than 10. 20. . eV. . . These high energies must be due to particle accelerations . AMS Discoveries Affecting Cosmic-Ray SIG Priorities. Eun-Suk. . Seo. Inst. for Phys. Sci. & Tech. and . Department of Physics. University of Maryland. AAS HEAD meeting, Chicago, IL, 19 August 2014. at. . Hartnell. . College. : A Case Study in Successful Undergraduate Research at a Two-Year College. Leo . Osornio. Hartnell. College. Presented at the 2012 AAPT Summer Meeting, Philadelphia. July 30, 2012. The Discovery of Antimatter!. In 1932 Carl Anderson studied cosmic rays using a “cloud . chamber”. . Charged particles produced in cosmic rays would enter the chamber and leave “tracks”. The tracks would bend in circles because the chamber was placed in a strong magnetic field. :. . the need for cross section data. Fiorenza Donato. Torino University and INFN. Compass Analysis Meeting. CERN, 16.04.2015. Plan of my talk. What are cosmic rays (CRs). Searches for dark matter in CRs. North Bengal University. TeV Neutrinos and Gamma rays from Pulsars/Magnetars. Introduction. The energy spectrum of cosmic rays extends to extremely high energies, values exceeding 10. 20. . eV. .. The origin of the cosmic rays and the mechanism responsible for acceleration of cosmic rays to such high energies . Koji Mukai. NASA/GSFC/CRESST and UMBC. How RXTE matches up with WDs. Luminosity: up to ~a few x 10. 34. erg s. -1. for symbiotic stars, ~a few x 10. 33. erg s. -1. for typical intermediate . polars. Plasma. . Astrophysics. Roger . Blandford. Paul Simeon. Yajie. Yuan. KIPAC. Stanford. 27 i 2012. AronsFest. 2. Describing Cosmic Plasma. Fluid description. P. , . . , . v. , B…. Magneto Fluid Dynamics . the Heliosphere. Riaan Steenkamp. University of Namibia. . 5. . July . 2018. History and Discovery. A short history of the discovery of Cosmic Rays. At beginning of 20. th. Century:. Hypothesis: . Eun-Suk. . Seo. Inst. for Phys. Sci. & Tech. and . Department of Physics. University of Maryland. AAS HEAD meeting, Chicago, IL, 19 August 2014. w. ith edits & voice from . Angela V. Olinto. 16 – 20 March 2015. Cosmic Rays: the current position -. from AMS to the Auger Observatory. 1. Alan Watson. University of Leeds. a.a.watson@leeds.ac.uk. Lecture 1:. Overview of the cosmic ray scene.