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for the KASCADE-Grande Collaboration. Motivation for ... KASCADE-Grande. Trigger efficiency in a. fiducial area of 0.28 km2. Including reconstruction cuts ...
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Despite the fact, that one cannot say anything about momentum ... Only pions above 80 GeV are considered ... EAS may also be used for investigation of primary ...
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primary elemental groups (but relative abundaces heavily depend on the ... Unfolding of 2-Dimensional shower size spectra, in different bin of zenith angle, ...
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Calibration of the hadron calorimeter of the KASCADE-Grande experiment with a ... Calorimeter worked fine, preliminary results are encouraging ...
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MAKET-ANI detector designed to measure Extensive Air Showers (EAS) from Primary ... The attenuation length by MAKET-ANI data is equal ?=211 38 g/cm2, for KASCADE ...
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x:xapmeta xmlns:x='adobe:ns:meta/' x:xaptk='XMP toolkit 2.8.2-33, framework 1.5' ...
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The main aim is: TO SOLVE THE 'KNEE PROBLEM' Other aims: ... It contradicts emulsion chamber experiments (Pamir) and air luminescence data (Hi Res) ...
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What s new and what questions remain since our previous meeting? Workshop on Physics at the End of the Galactic Cosmic-ray Spectrum April 26-30, 2005
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GAMMA Experiment Mutually compensative pseudo solutions of the primary energy spectra in the knee region Samvel Ter-Antonyan Yerevan Physics Institute
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describes 'PAMIR' Collaboration's data at E0 5 1015 eV ... CPGM explains the effect 'Pamir' & CPGM data have maxima at ZC 4 TeV cm. QGSMs ...
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Build on successes of optical Cherenkov in IMB, Kam, SuperK - SN1987A & muon ... Using commercial hydrophones (Benthos, ITC, ..) 100 MeV beam at ITEP into water tank ...
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Future ambitious plan of radio detections of highest energy cosmic rays
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~102/m2/secondo ~1/m2/anno Ginocchio ~1/km2/anno Caviglia ~1/km2/secolo Misure indirette Misure dirette Sviluppo di un EAS e segnali che arrivano al livello di ...
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... cosmic ray energy spectra in the knee region obtained with the GAMMA experiment ... GAMMA Experiment Ln(Nch ) 0.1, s 0.05, x, y 0.5-1m, 1.50 Ln(N ) 0.35-0.2 ...
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The next 10 years in Particle Astrophysics Workshop summary Some personal observations Tribute to Alan
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Title: Antares simulation tools Author: brunner Last modified by: brunner Created Date: 10/3/2003 12:54:47 PM Document presentation format: Affichage l' cran
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(2) Light components around the knee energy region obtained by Tibet ASgamma experiment. ... Energy flux and spectrum of HE particles at AS cores (Tibet) ...
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Title: Diapositiva 1 Created Date: 10/28/2006 5:31:24 PM Document presentation format: Presentazione su schermo Other titles: Arial Times New Roman Wingdings Comic ...
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l2 l r larger zenith angle longer path. Electrons are mostly absorbed, muons not ... Zenith angle 75 , geomagnetic angle 88 . Conclusions ...
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1930 Pierre Auger discovers particle showers. ... ray showers at four locations in Switzerland separated by. more than 50 km1) ...
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Alternative Detection Methods for Highest Energy Neutrinos
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Leeds, July 23, 2004. in honor of Alan Watson ... pre-pre-production DAQ and main board. monitoring temperatures during austral winter ...
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Title: Slide 1 Last modified by: SCIPP Document presentation format: Custom Other titles: Times New Roman Tahoma Arial Wingdings Avant Garde Gothic Comic Sans MS ...
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Institute for Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of ... dcr ~ 10-3 at 1012 - 1014 eV - anisotropy. rg ~ 1E/(Z 3 1015 eV) pc - Larmor radius ...
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Institute for Nuclear Research of Russian Academy of Sciences (INR) ... AURIGA. DUAL R&D. ROG. MiniGRAIL. SFERA. Baksan Neutrino Observatory b) Interferometers ...
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Air showers emit short, intense radio pulses ... Dept of Astrophysics, Nijmegen, The Netherlands. L. B hren S. Buitink. H. Falcke J.R. H randel ...
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PowerPointPrsentation
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Distancia de la estaci n m s cercana al punto de impacto medida en el plano de la lluvia. ... en la Estaci n m s Cercana. Simulaciones de las lluvias: Aires ...
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... but problems with data acquisition (oscilloscopes! ... Oscilloscope traces. of CR radio pulses. Coherent Geosynchrotron Radio Pulses in Earth Atmosphere ...
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Fly's Eye, Haverah Park, Akeno. mixed composition. Hires elongation rate ... acceleration energy is fixed by the geometry of the source and its magnetic field ...
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COSMIC RAY ORIGINS
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High-Energy Particles and Air Showers. CORSIKA 6.203. Methods and Results. An Educational Idea ... HISPARC (High School Project on Astrophysics Research with Cosmics) ...
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AGASA has an indication of clustering, indicating extra-galactic source. Neither show enhancement near the galactic center for energies E 1018. ...
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1. GAMMA Experiment. Samvel Ter-Antonyan. Yerevan Physics Institute ... Just this approach was used in the GAMMA experiment. GAMMA Experiment ...
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An active zinc and copper mine situated in Pyh salmi in central Finland. ... MUG (muon flux at 0m, 90m, 210m, SGO) MUD (muon background flux measurements, 0m-1400m) ...
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The LHCf experiment at LHC
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The importance of knowing the primary mass and how little we ... 'Fere libenter homines id, quod volunt, credunt!' 'Men wish to believe only what they prefer' ...
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Introduction : Principaux types de d tecteurs gazeux et liquides actuels ... Calorim tre argon liquide : H1, D0, ATLAS. Calorim tre avec liquide temp rature ...
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Greisen-Zatsepin-Kuzmin(GZK) Limit. Cosmic rays with energies above 5 1019 eV will interact with the cosmic ... This process would continue until the energy of ...
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Louisiana State University, Baton Rouge, LA, USA ... 1051 ergs in the blast wave. SN rate 2/century 2X1049ergs/yr. Blast wave must convert ~1% of its energy into ...
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Actuellement, avec les ? d' nergie 100 GeV, on atteint une r solution de 4 6 minutes d'arc ( comparer quelques secondes d'arc en astronomie X) ...
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ginkgo SIZE: Medium HABIT: Pyramidal when young; wide spreading with age FOL: Bright green in summer; excellent, golden yellow in fall; leaves change uniformly ...
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New Cosmic Rays at the Highest Energies
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Laboratory Astrophysics Working Group Summary Pisin Chen Stanford Linear Accelerator Center Stanford University Introduction Calibration of Observations
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Laboratory Astrophysics Working Group Summary
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Emulsion chambers
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SPARC (Stored Particle Atomic Physics Collaboration) CBM (Compressed ... Linux installed: SLC4 32bit version on each system, the gLite 3.1 package installed ...
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5University of Houston, Department of Physics, Houston, TX, US ... Primary GCRs interact with the Earth's atmosphere originating atmospheric ...
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... P ' ' n*x KQn ' ?M LF M PNG ...
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Dipartimento di Fisica e Astronomia & INFN. Universit di Catania (Italy) ... a six hours flight with a balloon gondola (August 7, 1912) Hess & Wolf carefully ...
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Wave equations for the spatially inhomogeneous medium derived from first principles (Maxwell) ... Dielectric properties, attenuation in the regolith ...
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Future Experiments in Astrophysics Energy Range: 1'95 K relic neutrino 1020 eV
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EC and exotic events A short Summary talk O' Saavedra
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Dark Energy Missions. Necessary to set the stage for APP missions ... Anita, Auger. Flux * E (GeV/ cm sec sr) Sensitivity to HE diffuse. neutrino fluxes ...
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