'Muon data' diaporamas de présentation

The energy spectrum from the KASCADE-Grande muon data (Update)

525 views • 41 slides

Make NM data for Analysis

1 North. 2. 4. 3. 5. 6. 7. 8. 9. 10 South. Make NM data for Analysis. Count rate at i-th patch C i (t) is calculated from observed rate at k-th station as. nk: number of the station in i-th patch. Predict IMF from NM data. m, N: defined parameter

522 views • 40 slides

GRAPES-3 ROOT Framework

412 views • 25 slides

The energy spectrum from the KASCADE-Grande muon data

399 views • 25 slides

Use of Cosmic Ray eLab to Teach the Research Process

Use of Cosmic Ray eLab to Teach the Research Process. Deborah Roudebush Oakton High School 2900 Sutton Road Vienna, VA 22181. AAPT 2009 Winter Meeting February 15, 2009 Chicago, Illinois. What is QuarkNet?.

262 views • 16 slides

Muon Offline Status

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UK Analysis tasks (WP1)

UK Analysis tasks (WP1). David Ward Nige Watson. TexPoint fonts used in EMF. Read the TexPoint manual before you delete this box.:. Tools: Beam Line reconstruction. Each of these items should consist of one or a few, Marlin processors.

207 views • 10 slides

Atmospheric neutrino fluxes

Atmospheric neutrino fluxes. A background and an interesting measurement How well do we know the atmospheric neutrino fluxes? The primary CR spectrum Can we have a muon and neutrino flux from the same code? A tool for simulation and analysis: a C++ class and a library

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Summary

Summary. Uncertainties on conventional atmospheric neutrino fluxes Enu CR hadronic quadrature 10 GeV-100 GeV 10% 15% 18% 1 TeV 15% 15% 21% 10 TeV 35% 25% 43%

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Status of Group E2

Status of Group E2. Short term goal: define the S-Link data format and firmware specs for all Level-2 data paths. We would like to standardize the format as much as possible. What have we done so far: we have been focusing on understanding the data

190 views • 7 slides