high energy telescopes

telescopes is based on the imaging air Cherenkov technique. This allowed searches for millisecond time-scale burst emission in very-high-energy (VHE) gamma-rays as well as the optical band. The aim of … The detection of high energy gamma rays with the H.E.S.S. They are instrumented with 12-14 telescopes each. The U.S. Department of Energy's Office of Scientific and Technical Information High energy neutrino astronomy and its telescopes (Journal Article) | OSTI.GOV skip to main content Future High Energy Neutrino Telescopes C.Spieringa aDESY Zeuthen D-15738 Zeuthen, Germany This talk summarizes the main physics goals and basic methods of telescopes for high energy neutrinos. Neutrino telescopes and high-energy astrophysics. High energy neutrino detection with Cherenkov underwater telescopes Candidate: Chiara Perrina E-mail: chiara.perrina@roma1.infn.it Supervisor: Prof. Antonio Capone E-mail: antonio.capone@roma1.infn.it 1. Before discussing the detectors we review the arguments that pinpoint $0.1\rmkm~2$ as the natural scale of a neutrino telescope. Commissioning of the AMANDA, DUMAND and NESTOR detectors will follow soon. Short description of the research team. Neutrino telescopes and high-energy astrophysics M. Spurio Dipartimento di Fisica dell’Universit`a di Bologna and INFN, Sezione di Bologna Bologna, Italy (ricevuto il 19 Settembre 2009; pubblicato online il 23 Novembre 2009) Summary. The telescope systems have characteristics sufficient to record precise information about the shower structure in the energy range under consideration. Manager/head of the team: Prof. Piero Rosati. Ann.Rev.Nucl.Sci 10 (1960) 63. Year 2010 - Issue 6 - November-December Incontri di Fisica delle Alte Energie - IFAE 2010. under-ground optical: - deep water - deep ice-air showers-radio-acoustics. The Telescope Array has been collecting data in the high desert in Millard County, Utah, USA since 2007. (in standard rock) the intensity of atmospheric muons becomes lower than the background flux of muons locally produced by neutrinos in the surrounding material. Very high-energy muons in neutrino water (ice) telescopes A.G. Bogdanov 3 since at depths more than about 10 km w.e. Welcome. 2. on Twitter or on Facebook for news regarding the H.E.S.S. This paper presents a review of the history, motivation and current status of high energy neutrino telescopes. With Earth’s atmosphere acting as a near-total shield against high-energy γ-rays, astronomers have traditionally relied on space telescopes to detect them. IRIS è la soluzione IT che facilita la raccolta e la gestione dei dati relativi alle attività e ai prodotti della ricerca. The evolution of high energy neutrino telescopes Christian Spiering DESY. We shortly discuss the motivations for HE neutrino astrophysics; a full and detailed version is reported in T. Chiarusi and M. Spurio, High-Energy Astrophysics with Neutrino Telescopes, arXiv:0906.2634 [astro.ph.HE]. Taking into account energy loss fluctuations, such depth corresponds to The first optical modules of the Baikal high energy neutrino telescope have recently been deployed. high-energy neutrino telescopes detect muons produced in cosmic ray inter-action in the atmosphere (so called atmospheric muons). We are currently adding a low energy extension to the Telescope Array which will enable us to study the changes in the energy spectrum and chemical composition over a broader energy range. Scopri Greater than 25 Mev Proton Events Observed by the High Energy Telescopes on the STEREO A and B Spacecraft and-or at Earth During the First Approximately Seven Years of the STEREO Mission di Ian G. Richardson: spedizione gratuita per i clienti Prime e per ordini a partire da 29€ spediti da Amazon. Thermal infrared (TIR) earth observation telescopes in low earth orbit can monitor the energy output of buildings. Year 2009 - Issue 3-4 - May-August Incontri di Fisica delle Alte Energie - IFAE 2009. High-energy neutrino telescopes. High­Energy ν astronomy: a new sky P. D. Serpico, MPIfP (WHI)­ Munich “Neutrino mixing @ HE ν telescopes” 23­25/11 /05 ECFA/BENE Week – CERN Neutrinos: a powerful tool for high energy … section.. Introduction One of the main questions in Physics is the origin of high energy Cosmic Rays (CRs). To learn more about H.E.S.S. 10 9 tons and more. The evolution of high energy neutrino telescopes …a long march which has not yet reached its end. 30 TH INTERNATIONAL C OSMIC R AY C ONFERENCE The High Energy Telescopes for the STEREO Mission T.T. Many years after … The energy information is obtained from the amount of electromagnetic showers, induced by bremsstrahlung, that occur along the muon track. Follow H.E.S.S. VON R OSENVINGE 1, A.C. C UMMINGS 2, R.A. L ESKE 2, R.A. M EWALDT, D.V. In order to supply for such extremely hostile environmental conditions, new frontiers technologies are under development. Team members: Dott.Cristiano Guidorzi, Emeritus Professor Filippo Frontera and Dott. instrument and its science The effective target masses of such detectors could be approx. Telescopes are located in the Tien-Shan mountains at the altitude of 3340 m a.s.l. SHALON telescopes Introduction Cosmic rays were discovered a century ago [1], but … S TONE 2, M.E. and the high energy universe, or to view pictures from the telescopes and the site in Namibia visit the About H.E.S.S. Dr Ian Parry from Cambridge’s Institute of Astronomy has been awarded funding for high-resolution thermal infrared space telescopes for monitoring the energy efficiency of buildings. — Neutrino astrophysics offers new perspectives on Universe investi- Ann.Rev.Nucl.Sci It reviews the present status of deep underwater telescopes and sketches the ICECUBE project as an example for a cube kilometer detector. High Energy NeutrinoGenerator for Neutrino Telescopes Marek Kowalski and Askhat Gazizov DESYZeuthen,Platanenallee6,D-15738Zeuthen,Germany Abstract We present the high energy neutrino Monte Carlo event generator ANIS (All Neutrino Interaction Simulation). High Energy Neutrino telescopes Ice Cherenkov detector: AMANDA, IceCube located at the South Pole (Southern hemisphere) → different FoV (uniform coverage of the northern sky at the South Pole and non uniform exposure but larger FoV in the Mediterranean) Northern hemisphere detectors have a direct Thematic fields of interest/research areas: Realization of focusing optics for High energy telescopes. Using observations from the High Energy Telescopes (HETs) on the STEREO A and B spacecraft and similar observations from near-Earth spacecraft, we summarize the properties of more than 200 individual > 25 MeV solar proton events, some detected by multiple spacecraft, that occurred from the beginning of the STEREO mission in October 2006 to December 2013, and provide a catalog of these … Welcome to the webpages of H.E.S.S., one of the leading observatories studying very high energy (VHE) gamma-ray astrophysics. An incident high-energy gamma ray interacts high up in the atmosphere and generates an air shower of secondary particles.The number of shower particles reaches a maximum at about 10 km height, and the shower dies out deeper in the atmosphere. W IEDENBECK 3 1Astroparticle Physics Laboratory, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA 2Downs Laboratory, California Institute of Technology, Pasadena, … X-ray and Gamma-ray telescopes are usually installed on Earth-orbiting satellites or high-flying balloons since the Earth's atmosphere is opaque to this part of the electromagnetic spectrum. R EAMES 1, E.C. High energy neutrino detection with Cherenkov undersea telescopes Candidate: Chiara Perrina E-mail: chiara.perrina@roma1.infn.it Supervisor: Prof. Antonio Capone E-mail: antonio.capone@roma1.infn.it 1. Many years after these detectors were first conceived, the operation of kilometer-cubed scale detectors is finally on the horizon at both the South Pole and in the Mediterranean Sea. Fornisce a ricercatori, amministratori e valutatori gli strumenti per monitorare i risultati della ricerca, aumentarne la visibilità e allocare in modo efficace le risorse disponibili. The telescopes for cosmic high energy neutrino detection by radioemission of cascades induced underground, but whose development continues in the atmosphere were proposed by others. Due to the low in-teraction probability of neutrinos, the trigger rates due to atmospheric muons is generally orders of magnitude higher than that of atmospheric neutrinos. High Energy Neutrino Telescopes K D Ho man Department of Physics, University of Maryland, College Park, MD 20742 USA E-mail: kara@umd.edu Abstract. This paper presents a review of the history, motivation and current status of high energy neutrino telescopes. Neutrino telescopes and high-energy cosmic neutrinos Andrea Palladino1,Maurizio Spurio2 ;3,and Francesco Vissani4 5 1 Deutsches Elektronen-Synchrotron (DESY), Platanenallee 6, D-15738 Zeuthen, Germany 2 NFN-Sezione di Bologna, Viale Berti-Pichat 6/2, 40127 Bologna, Italy 3 Dipartimento di Fisica e Astronomia, dell’Universit a, Viale Berti Pichat 6/2, 40127 Bologna, Italy In the high-energy neutrino telescopes the emphasis is put on the directional resolution, energy resolution being only of secondary importance. CRIS Current Research Information System. Many years after these detectors were first conceived, the operation of kilometer-cubed scale detectors is finally on the horizon at both the South Pole and in the Mediterranean Sea. Higher energy X-ray and Gamma-ray telescopes refrain from focusing completely and use coded aperture masks: the patterns of the shadow the mask creates can be reconstructed to form an image. This paper presents a review of the history, motivation and current status of high energy neutrino telescopes. We conducted simultaneous observations of FRB 121102 with the Arecibo and MAGIC telescopes during several epochs in 2016–2017. During more than 25-year operation SHALON has studied in details the objects of different type at energies up to 100 TeV , and continues to produce the results in the field of very high energy astrophysics. The ICECUBE project as an example for a cube kilometer detector C UMMINGS 2 R.A.. Muons ) DUMAND and NESTOR detectors will follow soon Professor Filippo Frontera and Dott ) gamma-ray astrophysics the Tien-Shan at. Delle Alte Energie - IFAE 2010 at depths more than about 10 km.. In very-high-energy ( VHE ) gamma-ray astrophysics output of buildings of FRB 121102 with the Arecibo MAGIC! The high energy telescopes output of buildings, energy resolution being only of secondary importance ) earth observation telescopes in low orbit! 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