'Cerenkov' presentation slideshows

Low frequency radio-emission from UHE cosmic ray air showers

Low frequency radio-emission from UHE cosmic ray air showers. KALYANEE BORUAH Physics Department, Gauhati University. Radio Emission from Air Showers: A Brief History. Oscilloscope traces of CR radio pulses. Jelley et al. (1965) ?. Historical development. Theory

482 views • 39 slides

Muon trigger upgrade

412 views • 33 slides

Philosophy and Feasibility of Dual Readout Calorimetry

Philosophy and Feasibility of Dual Readout Calorimetry. The main simple idea is to measure a hadronic shower twice - as if two different calorimeters make an image of the same shower.

433 views • 31 slides

Acceptance and Counting Rates of EUSO

Acceptance and Counting Rates of EUSO. Detecting UHECR from space The EUSO detector : Who does what. Some characteristics of UHECR A statistical view of clouds A first approach of the acceptance The influence of clouds on the signal The different Atmosphere Sounding Devices

258 views • 16 slides

Determination of Sr-89/Sr-90 in primary cooling water

559 views • 15 slides

Cerenkov Radiation contribution to Stray Light in NIRCam

Cerenkov Radiation contribution to Stray Light in NIRCam. Peter McCullough 19 Jan 2006 STScI TIPS. History.

307 views • 15 slides

Scattered e- momentum

Scattered e- momentum. RHRS run20978,20980, 20989, 20999. HRS p0 settings are written on the plot. From this, you will see the shift of the peak. Normalized the distribution as N* prescale /(1-DT)/current/time, assuming other factors are same for each run as Karl said

193 views • 12 slides

GLAST Observations of Supernova Remnants and Pulsar Wind Nebulae

NASA / ESA / J. Hester / A. Loll / ASU. GLAST Observations of Supernova Remnants and Pulsar Wind Nebulae. Bryan Gaensler The University of Sydney / Harvard-Smithsonian Center for Astrophysics. Introduction. radio. optical. X-rays. Supernova remnants (SNRs) & pulsar wind nebulae (PWNe)

335 views • 12 slides

Y.Onel, University of Iowa D.R.Winn, Fairfield University

New Calorimeter Technologies for NLC (a) Secondary Emission Calorimeter Sensors (b) Cerenkov Compensated Precision Calorimetry. Y.Onel, University of Iowa D.R.Winn, Fairfield University. (a) Secondary Emission Sensor Modules for Calorimeters. Basic Idea:

197 views • 11 slides

Preliminary Geometry of Cerenkov Detector for New BigBite Spetrometer

Preliminary Geometry of Cerenkov Detector for New BigBite Spetrometer. Bo Zhao College of William and Mary. Hall A weekly meeting, March 22, 2011. 1. Specification of Cerenkov.

155 views • 9 slides

RUN3 Cerenkov analysis (update)

RUN3 Cerenkov analysis (update). Kazuya Aoki Kyoto University Muon trigger meeting 2003-09-02. Outline. Electron energy spectra ( tunnel 15, 20 , IR) The cross section of [S1xS2xCxMuID1D] Compare the cross section with the DAQ limit. Cerenkov in the South Tunnel. 15deg. MuID wall.

176 views • 8 slides

ADRIANO : A D ual R eadout I ntegrally A ctive N on-segmented O ption for Future Colliders

ADRIANO : A D ual R eadout I ntegrally A ctive N on-segmented O ption for Future Colliders. Corrado Gatto INFN. On behalf of:. TWICE Collaboration. Merging the advantages of sampling and total active techniques. ADRIANO technique: i.e. embedd scintillating fibers into heavy glass

85 views • 8 slides