PPT-Atmospheric Muon Lifetime, Standard Model of Particles and

Cioli Barazandeh Angel Gutarraleon and Walerian Majewski Mentor Walerian Majewski Department of Physics Northern Virginia Community College Annandale VA Experiments Hello and welcome to my Presentation. 00 NA NA NA NA Resident 44 and Under 26000 26000 26000 27600 NA Resident 45 to 50 21000 21000 21000 13200 NA Resident 51 to 55 16000 16000 16000 9900 NA Resident 56 to 60 11000 11000 11000 6600 NA Resident 61 to 64 6000 6000 6000 35 Upgrade Status. P. Campana, . Muon Upgrade . Meeting, . September 3rd, . 2010. . Progress of the work on Muon Upgrade. . Preparation of LOI-Muon. 1. 2. Some work done since our last meeting:. ODE electronics (Caterina et al. – see separate talk). 2. :CO. 2. ratios . over the Southern Ocean. Britton Stephens (NCAR), Ralph Keeling (Scripps), Gordon . Brailsford. (NIWA), Andrew Manning (UEA), Sara . Mikaloff. -Fletcher (NIWA), . Prabir. . Patra. Nick Barlow. (University of Cambridge). on behalf of the ATLAS collaboration. Contents. Motivation . for searching for long-lived particles.. Very. quick look at a couple of . signal models. .. The ATLAS detector and the 2011 dataset.. Upgrade Status. P. Campana, . Muon Upgrade . Meeting, . September 3rd, . 2010. . Progress of the work on Muon Upgrade. . Preparation of LOI-Muon. 1. 2. Some work done since our last meeting:. ODE electronics (Caterina et al. – see separate talk). (work funded through the Great Lakes Restoration Initiative). Dr. Mark Cohen. NOAA Air Resources Laboratory (ARL). College Park, MD, USA. Briefing Slides for GLRI Monthly Call. January 9, 2013. Atmospheric deposition is believed to be the largest . Corrections. Atmospheric Effects on EMR. Kodiak Island, AK – Volcanic ash and clouds (MODIS image). Learning Objectives. What are the main ways that the atmosphere affects light traveling through it?. How did . the universe come to be the way that it . is?. Democritus (~2500 years ago). Recall the four fundamental forces:. GRAVITY: . All particles are influenced.. Relative strength: . WEAK: . All particles are influenced.. Outline. Class 1 Atlas Control Room Shifts. Booking. Present Status + Experience+ Feedback. Class . 2 reminder. A. . Polini. & Z. Yan. May 21. th. 2012. Class 1 Control Room . Muon. Shifts. Following Steering and IB discussions in November:. Talk given in the last year. V. . Kaushik. M. King. P. . Klluit. V. . Kouskoura. J.F . Laporte. J. Meyer. N. Orlando. A. . Orraou. P. . Pais. A. . Polini. E. . Pueschel. S. . Rosati. A. . Salvucci. S. . . . ILC and More Workshop. Lake Como, Italy. . May 16-17, 2013. Why . Muons. ?. What’s so special about . Muons. ?. Muons. are . Heavy. LHC, MAP, and LEMC. David . Neuffer. July 2018. 2. Outline. Next Heavy Lepton Collider . up to ~14 . TeV. in LHC tunnel. Needs muon source. PS or new MW proton . Linac. /storage ring. cooling …. or LEMC??. in . the. TA experiment. Takayuki . Tomida. . and the TA collaboration. RIKEN. Fluorescence Detector (FD. ). Surface Detectors . SDs. . Plastic . scintillator. Telescope . Array(TA. ). Experiment. EARTH SURFACE. gravity. random. motion. Weight of all air molecules is propagated to surface by random motion of molecules. Random motion of molecules causes pressure to be applied in all directions.