PPT-LOFAR Cosmic Ray KSP

Heino Falcke Radboud University Nijmegen ASTRON Dwingeloo What we dont know about UHECRs We know their energies up to 10 20 eV their overall energy spectrum We dont know. Cosmic Catering isn’t just about tasty, healthful, local food, crafted by a Restaurant School trained Chef (who has a passion for vegetables!) though.  We are pride of holding reasonable prices, keeping a prompt delivery record and being meticulous about our cleanup.  All within an award-winning business model of sustainable practices. Connect the Fluke 415 HV supply output to the input of the voltage distribution box. (Make sure HV is off.). Connect the outputs of the HV distribution box to the HV supply for the phototubes in the cosmic ray . The Future of Cosmic Ray Research. .. 8 The Future of Cosmic Ray Research . As we have seen, a few cosmic rays can be detected with energies somewhat . greater . than 10. 20. . eV. . . These high energies must be due to particle accelerations . (astro-ph: 0809.2428). Geraint Harker. Kapteyn Astronomical Institute, Groningen. Wed. 17th Sept. 2008. 1. Hamburg LOFAR Workshop. The problem. Extract a cosmological signal from a datacube, the three axes of which are x and y positions, and frequency.. & Large scale structure. Tarun Souradeep. I.U.C.A.A. .. Cosmology . IUCAA . VSP program. (. May 18-22, . 2012). Lec. . . 4:. Current frontiers. Mildly Perturbed universe at z=1100. Present universe at z=0. and Other Applications: Hydrology +. Neutron Monitor Community Workshop—Honolulu, Hawaii . October . 24-25, 2015. Physicist. National Urban Security Technology Laboratory . Science and Technology Directorate. Arunava. . bhadra. High Energy & Cosmic ray research centre, University of North Bengal. Siliguri. , India. Collaborators: . Biplab. . Bijay. , . Prabir. . Banik. The knee in the Energy spectrum. The Discovery of Antimatter!. In 1932 Carl Anderson studied cosmic rays using a “cloud . chamber”. . Charged particles produced in cosmic rays would enter the chamber and leave “tracks”. The tracks would bend in circles because the chamber was placed in a strong magnetic field. Bruce Reynolds, November 2015. 1. Outline. Cosmic Definition. Functional Size Measurement. Functional User Requirements. Non-Functional Requirements. COSMIC Approach. In-Class Exercise. COSMIC—a Real World example. AA single station snapshot correlation. S.Salvini. , . F.Dulwich. , . B.Mort. , . K.Zarb-Adami. stef.salvini@oerc.ox.ac.uk. Content. Fundamentals. Results 1: . Chilbolton. LOFAR. Results 2: Simulated sky tests (experiments). at low frequencies with LOFAR. Kimon Zagkouris. University of Oxford. In collaboration with the LOFAR Pulsar Working Group. Ierapetra June 2014. Image Credit. : David A. Aguilar (. CfA. ) / NASA / ESA. Exoplanets. Jake D. Turner. University of Virginia. astrojaketurner@gmail.com. Exoplanet Magnetic Fields . Motivation. Interior . structure . Star. -planet Interactions. Habitability. Jake . Turner (. USING DATA ON EXTRAGALACTIC DIFFUSE . GAMMA-RAY EMISSION. . A. . Uryson. Lebedev. Physical Institute RAS, . Moscow. INTRODUCTION. UHECR data are obtained by Pierre Auger Observatory (PAO) and Telescope Array (TA):. Complex Ion Formation. Multiple Equilibria. Factors Affecting Solubility. Solubility Equilibrium. E. quilibrium . between . precipitates or solid compounds and their ionic species in aqueous solutions;.