'Pierre auger observatory' diaporamas de présentation

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Presented for Arnulfo Zepeda On behalf of the Mexican Collaboration

PHYSICS AND ASTROPHYSICS OF ULTRA HIGH ENERGY COSMIC RAYS. BUAP CINVESTAV UMSNH UNAM. Presented for Arnulfo Zepeda On behalf of the Mexican Collaboration. Material selected and prepared for Rebeca López. Sep. 2000. GOAL.

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Results from the Pierre Auger Observatory

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Chapter 13 Neutron Stars

Chapter 13 Neutron Stars. Chapter 13 Neutron Stars and Black Holes. Units of Chapter 13.1 - 13.4. Neutron Stars Pulsars Neutron Star Binaries Gamma-Ray Bursts. Neutron Stars. After a Type I supernova, little or nothing remains of the original star.

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Ultra High Energy Cosmic Rays at Pierre Auger Observatory

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Recent Results from the Pierre Auger Observatory

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Status, Performance and Perspectives of the Auger Observatory

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Seismic Network at the Pierre Auger Observatory

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Research at VATLY : main themes and recent results

Research at VATLY : main themes and recent results. PN Diep , PN Dong, PTT Nhung, P Darriulat, NT Thao and VV Thuan VATLY, INST, Hanoi, Vietnam. Hoi An, 2007.

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Dan Hooper Theoretical Astrophysics Group Fermi National Laboratory dhooper@fnal

Theoretical Particle-Astrophysics At Fermilab. Dan Hooper Theoretical Astrophysics Group Fermi National Laboratory dhooper@fnal.gov. Annual DOE Review May 17, 2006. How To Study Particle Physics?. Traditionally, particle physics has been studied using collider experiments

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An Ultra-High-Energy Cosmic Ray Experiment

An Ultra-High-Energy Cosmic Ray Experiment. Glenn Sembroski QuarkNet Summer Workshop July 24,2012. The Big Question Which has become the Big Mystery. Where do Cosmic Rays come from? A multi-part question. i.e. Lots of small mysteries Different answers for different energy regimes

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HEP Applications status in EELA

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Fl uorescence from A ir in Sh owers ( FLASH )

Proposal E-165. Fl uorescence from A ir in Sh owers ( FLASH ) J. Belz 1 , Z. Cao 2 , P. Chen 3* , C. Field 3 , P. Huentemeyer 2 , W-Y. P. Hwang 4 , R. Iverson 3 , C.C.H. Jui 2 , T. Kamae 3 , G.-L. Lin 4 , E.C. Loh 2 , K. Martens 2 , J.N. Matthews 2 , W.R. Nelson 3 , J.S.T. Ng 3 ,

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Auger Project Computing Needs

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The Pierre Auger Project

The Pierre Auger Project. By Megan Edwards Bancroft-Rosalie. Pierre Auger. Can be considered as the discoverer of the giant air showers in 1938 generated by the interaction of very high-energy cosmic rays with the earth's atmosphere.

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Auger North

Auger North. Continuation of plans to construct the Pierre Auger Observatory: detector systems located at two sites, on both hemispheres Southern observatory (in Mendoza, Argentina) is under construction Northern observatory (in Colorado, USA) is in planning stage.

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Atmospheric Aerosol Measurements at the Pierre Auger Observatory

HE 1.4. Atmospheric Aerosol Measurements at the Pierre Auger Observatory. L. Valore for the Pierre Auger Collaboration.

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