'Fluorescence detector' presentation slideshows

Valerio Verzi INFN Roma Tor Vergata for the Pierre Auger Collaboration

Results on Ultra-High Energy Cosmic Rays from the Pierre Auger Observatory. Valerio Verzi INFN Roma Tor Vergata for the Pierre Auger Collaboration. COSMIC RAYS SPECTRUM (2008). l. Flux x E 2.5. UHECR. ~ 10 20 eV. 1 particle/km 2 /century!. WHERE DO COME FROM?. B. R.

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Rutherford Appleton Seminar 19 March 2008

Rutherford Appleton Seminar 19 March 2008. Is the search for the origin of the Highest Energy Cosmic Rays over? Alan Watson University of Leeds, England a.a.watson@leeds.ac.uk. OVERVIEW Why there is interest in cosmic rays > 10 19 eV

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Humberto Salazar (FCFM-BUAP) for the Pierre Auger Collaboration ,

Ultrahigh Cosmic Rays: The highest energy frontier. Humberto Salazar (FCFM-BUAP) for the Pierre Auger Collaboration , CTEQ- Fermilab School Lima, Peru, August 2012. The Auger Observatory in the Southern Hemisphere Hybrid shower measurements

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622 views • 49 slides

Particle Astrophysics

Particle Astrophysics. Cosmic rays Gamma-ray astronomy Neutrino astronomy. Multi-messenger astronomy. Protons , g -rays , n , [gravitational waves] as probes of the high-energy universe Protons : directions scrambled by magnetic fields Photons : straight-line propagation but

640 views • 48 slides

TUS Experiment: A space fluorescence detector for study of EECR

TUS Experiment: A space fluorescence detector for study of EECR. Humberto Salazar for the TUS/TUS-M collaboration September, 2006, Puebla. Is there the cut off in cosmic ray energy spectrum?. G.T. Zatsepin, 1968

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SPACE DETECTORS TUS and KLYPVE for STUDY of ULTRA HIGH ENERGY COSMIC RAYS

SPACE DETECTORS TUS and KLYPVE for STUDY of ULTRA HIGH ENERGY COSMIC RAYS. TALK AT THE INTERNATIONAL SEMINAR ON ULTRA HIGH ENERGY COSMIC RAYS 14 APRIL 2005 B. A. KHRENOV D.V. Skobeltsyn Institute of Nuclear Physics

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Ultra High Energy Cosmic Rays at Pierre Auger Observatory

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VATLY, a cosmic ray laboratory in Hanoi, progress report

VATLY, a cosmic ray laboratory in Hanoi, progress report. PN Diep , PN Dong, PTT Nhung, P Darriulat, NT Thao, DQ Thieu and VV Thuan VATLY, INST, Hanoi, Vietnam. http://www.inst.gov.vn/inst/English/About/VATLY/Vatly.htm.

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Motivation for Top-Up: A beamline perspective

Motivation for Top-Up: A beamline perspective. David Paterson Top-Up Workshop. I 0 incident flux. Potassium. Calcium. Iron. Cobolt. Zinc. 4 good reasons for topup. stability resolution speed flexibility. Pt spectrum located in a tumour cell Hambley et al, U Sydney.

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Recent results from the Pierre Auger Observatory

Recent results from the Pierre Auger Observatory. Pham Ngoc Diep for the Pierre Auger Observatory. Vinh 10/2011. x = 2.7. x = 3.0. x = 2.7. Cosmic rays. charged particles, extremely high energies ~10 20 eV=16 Joules! power law spectrum ~ E -2.7 Galactic: DSA in young SNR shells

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Microbial Genetics

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Status of the Pierre Auger Observatory

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DEHP Leaching from PVC into Contents of Medical Devices

DEHP Leaching from PVC into Contents of Medical Devices. Rajvi Mehta Chem 4101, Fall 2011 December 9, 2011. Analyte: DEHP. Di-2-ethylhexyl Phthalate (DEHP) is a phthalate ester plasticizer that is used to make PVC medical devices soft and flexible.

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DEHP Leaching from PVC into Contents of Medical Devices

DEHP Leaching from PVC into Contents of Medical Devices. Rajvi Mehta Chem 4101, Fall 2011 December 9, 2011. Analyte: DEHP. Di-2-ethylhexyl Phthalate (DEHP) is a phthalate ester plasticizer that is used to make PVC medical devices soft and flexible.

274 views • 12 slides

Claudio Di Giulio University of Roma Tor Vergata, INFN of Roma Tor Vergata

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