By: Ayan Batyrkhanov For Horizon-T group

Slides:



Advertisements
Similar presentations
HELYCON Hellenic Lyeum Cosmic Observatories Network Developing and Constructing An Extensive Air Shower Detector Antonis Leisos Hep2006-Ioannina Hellenic.
Advertisements

Antonis Leisos KM3NeT Collaboration Meeting the calibration principle using atmospheric showers the calibration principle using atmospheric showers Monte.
INSTITUT MAX VON LAUE - PAUL LANGEVIN Fast Real-time SANS Detectors Charge Division in Individual, 1-D Position- sensitive Gas Detectors Patrick Van Esch.
Apostolos Tsirigotis HELYCON Hellenic Lyceum Cosmic Observatories Network a progress report Hellenic Open University, University of Patras, University.
Application for Pierre Auger Observatory.
Antonis Leisos KM3NeT Design Study the calibration principle using atmospheric showers the calibration principle using atmospheric showers construction.
Use of floating surface detector stations for the calibration of a deep-sea neutrino telescope G. Bourlis, N. A. B. Gizani, A. Leisos, A. G. Tsirigotis,
Design and First Results of a Cosmic Ray Telescope For Use In Testing a Focusing DIRC M. P. Belhorn University of Cincinnati The BELLE group at the University.
HiRes Usage. Outline ● Shower energy ( Size, dE/dx ) ● Atmospheric profile ( stdz76, radiosonde) ● Rayleigh Scattering ● Aerosols Model ( density, variability.
AGASA Masahiro Teshima Max-Planck-Institut für Physik, München, Germany for AGASA collaboration.
Timing Properties of T0 Detectors At PHOBOS Saba Zuberi, Erik Johnson, Nazim Khan, Frank Wolfs, Wojtek Skulski University of Rochester.
The UC Simulation of Picosecond Detectors Pico-Sec Timing Hardware Workshop November 18, 2005 Timothy Credo.
Forward Detectors and Measurement of Proton-Antiproton Collision Rates by Zachary Einzig, Mentor Michele Gallinaro INTRODUCTION THE DETECTORS EXPERIMENTAL.
Search for isotropic microwave radiation from electron beam in the atmosphere T. Yamamoto a, I. S. Ohota a, Y. Inome a, D. Ikeda b, H. Sagawa b, S. Ogio.
A crude (lower limit) estimation of resolution and event rate Development and Construction of an Extensive Air Shower Array in HOU Antonis Leisos, Hellenic.
The ANTARES experiment is currently the largest underwater neutrino telescope and is taking high quality data since Sea water is used as the detection.
Report on SiPM Tests SiPM as a alternative photo detector to replace PMT. Qauntify basic characteristics Measure Energy, Timing resolution Develop simulation.
KamLAND Experiment Kamioka Liquid scintillator Anti-Neutrino Detector - Largest low-energy anti-neutrino detector built so far - Located at the site of.
Experimental set-up Abstract Modeling of processes in the MCP PMT Timing and Cross-Talk Properties of BURLE Multi-Channel MCP PMTs S.Korpar a,b, R.Dolenec.
Tunka-133: results and status L.A.Kuzmichev (MSU SINP) On behalf of the Tunka Collaboration th ECRS, MOSCOW.
The MPPC Study for the GLD Calorimeter Readout Introduction Measurement of basic characteristics –Gain, Noise Rate, Cross-talk Measurement of uniformity.
Scintillation hodoscope with SiPM readout for the CLAS detector S. Stepanyan (JLAB) IEEE conference, Dresden, October 21, 2008.
Hjdh Andrea Misner Astrophysics Student Member of “Team Butler” Supervisor: Dr. Malcolm Butler From Cosmic Rays to Local Classrooms High School Physics.
This experiment is to obtain the excitation functions of the 13 C (α, α) 17 O elastic scattering at the initial beam energy 13 C.
Preliminary MC study on the GRAND prototype scintillator array Feng Zhaoyang Institute of High Energy Physics, CAS, China GRAND Workshop, Paris, Feb. 015.
Contributions of the University of Bucharest to the study of high energy cosmic rays in the framework of the KASCADE-Grande experiment Octavian Sima Faculty.
Atmospheric shower simulation studies with CORSIKA Physics Department Atreidis George ARISTOTLE UNIVERSITY OF THESSALONIKI.
Experimental set-up for on the bench tests Abstract Modeling of processes in the MCP PMT Timing and Cross-Talk Properties of BURLE/Photonis Multi-Channel.
Alba Cappa Universita’ and INFN Torino Čerenkov Light Measurements for the EUSO Experiment Rencontres de Moriond – Very High Energy Phenomena in the Universe.
1 Energy loss correction for a crystal calorimeter He Miao Institute of High Energy Physics Beijing, P.R.China.
Properties of giant air showers and the problem of energy estimation of initial particles M.I. Pravdin for Yukutsk Collaboration Yu.G. Shafer Institute.
Tunka Experiment: Towards 1км 2 EAS Cherenkov Array B.K.Lubsandorzhiev for TUNKA Collaboration.
The single shower calibration accuracy is about 6.7 degrees but the accuracy on the mean value (full data set calibration accuracy) scales down inversely.
Study of high energy cosmic rays by different components of back scattered radiation generated in the lunar regolith N. N. Kalmykov 1, A. A. Konstantinov.
EAS Time Structures with ARGO-YBJ experiment 1 - INFN-CNAF, Bologna, Italy 2 - Università del Salento and INFN Lecce, Italy A.K Calabrese Melcarne 1, G.Marsella.
The KASCADE-Grande Experiment: an Overview Andrea Chiavassa Universita’ di Torino for the KASCADE-Grande Collaboration.
What we do know about cosmic rays at energies above eV? A.A.Petrukhin Contents 4 th Round Table, December , Introduction. 2. How these.
The SPHERE Project Antarctic Balloon-Borne Measurements Of Cosmic Rays Spectrum In Energy Range 1-100EeV Rem Antonov – Moscow State University R.A. Antonov,
D.V.Skobeltsyn INP Moscow State University “Energia” Korolev (Rocket Space Corporation) “Luch” Syzran SCTB, Russia JINR, Dubna, Russia Mexico University,
Performances of the KM2A prototype array J.Liu for the LHAASO Collaboration Institute of High Energy Physics, CAS 32nd International Cosmic Ray Conference,
Nearly vertical muons from the lower hemisphere in the Baikal neutrino experiment Zh. Dzhilkibaev - INR (Moscow) for the Baikal Collaboration ( Uppsala,
NEVOD-DECOR experiment: results and future A.A.Petrukhin for Russian-Italian Collaboration Contents MSU, May 16, New method of EAS investigations.
Tunka-133: Primary Cosmic Ray Energy Spectrum in the energy range 6·10 15 – eV L.A.Kuzmichev (SINP MSU) On behalf on the Tunka Collaboration 32th.
Beam Profile Monitor for Spot-Scanning System Yoshimasa YUASA.
AGASA Results Masahiro Teshima Max-Planck-Institut für Physik, München, Germany for AGASA collaboration.
MC study of TREND Ground array Feng Zhaoyang Institute of High Energy Physics,CAS
Lingling Ma IHEP China Measurement of Cosmic rays with LHAASO at 10PeV~100PeV 4th Workshop on Air Shower Detection at High Altitude Institute of High Energy.
1 Cosmic Ray Physics with IceTop and IceCube Serap Tilav University of Delaware for The IceCube Collaboration ISVHECRI2010 June 28 - July 2, 2010 Fermilab.
The photomultiplier tubes selection for KM2A electromagnetic particle detectors (EDs) hou chao IHEP The 2nd workshop of air shower detection at high altitudes.
The Tunka-133 EAS Cherenkov light array: status 2011 N.Budnev, Irkutsk State University, on behalf of the Tunka Collaboration.
A Measurement of the Ultra-High Energy Cosmic Ray Spectrum with the HiRes FADC Detector (HiRes-2) Andreas Zech (for the HiRes Collaboration) Rutgers University.
 13 Readout Electronics A First Look 28-Jan-2004.
The dynamic range extension system for the LHAASO-WCDA experiment
Ultra fast SF57 based SAC M. Raggi Sapienza Università di Roma
“Performance test of a lead glass
L.L.Ma for LHAASO collaboration Beijing China
Expectation of Cosmic Ray Energy Spectrum with LHAASO
Scintillation Detectors
Institute of High Energy Physics, CAS
Analysis of FADC single-crystal data
35th ICRC, Busan, Korea, July 2017
A First Look J. Pilcher 12-Mar-2004
Multicore Cosmic Shower in the ARGO-YBJ experiment
Litao Zhao Liaoning University&IHEP
A new 1 km2 EAS Cherenkov Array in the Tunka Valley
Karen Andeena, Katherine Rawlinsb, Chihwa Song*a
Telescope Array Experiment Status and Prospects
Study of Event Reconstruction for Saturated Pulse
The MPPC Study for the GLD Calorimeter Readout
Hellenic Open University
Presentation transcript:

By: Ayan Batyrkhanov For Horizon-T group Fast Charged Particle Detector with High Dynamic Range at Horizon-10T Cosmic Rays Detector System By: Ayan Batyrkhanov For Horizon-T group

Horizon-T Group R. U. Beisembaev, E. A. Beisembaeva, O. D. Dalkarov, V. A. Ryabov, S. B. Shaulov, M. I. Vildanova, V. V. Zhukov P. N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russia K. A. Baigarin, A. Batyrkhanov, A. Iakovlev, T. Uakhitov, A. Yeltokov Nazarbayev University, Astana, Kazakhstan T. X. Sadykov LLP “Institute of Physics and Technology”, Almaty, Kazakhstan D. Beznosko Bard College, New Orleans, LA, USA

Horizon-10T (HT) Detector System [1,2,3] An innovative detector system pulse shape -> disk width information 2 ns resolution EAS E> 1016 eV ; Zenith angles (0o - 85o). At Tien Shan high-altitude Science Station ~3340 meters above the sea level 10 charged particle detection points [8] separated by the distance up to 1.3 kilometer Optical detector subsystem to view the Vavilov- Cherenkov light from the EAS Station name Center Yastre bov Stone Flower Left Kurash kin Right Bottom Upper Cher 600m Bunker Station # 1 2 3 4 5 6 7 8 VCD 9 10

Temporal structure of eas Time, ns Distance from core, m Can reconstruct using particle density distribution Need to calibrate detection points to obtain equivalent MIP number If know time and width, additional methods can be used (CORSIKA) [5] Observation level with detectors

Data examples for Standard EAS Standard EAS signal (bottom) and unusual event (right) from each HT detector Corresponds to simulation Estimated Energy: ~2·1016 eV (left) high zenith angle 5

EAS characteristics from temporal structure Disk arrival time ~r2 (used for arrival direction determination) Disk passage time (e.g. width) is growing with ~r Can use particle density and pulse width additional information from each detection point Need high time resolution

Horizon-T (HT) Detector System 1 m2 polysterene-based scintillators & scintillating glass with PMT 1 m above R7723 Hamamatsu [6] PMT (52 mm diameter) 2kV max voltage 1.7 ns pulse rise time 1.1 ns time spread 500 MHz digitization CAEN [9] DT5730 ADC Cherenkov-Vavilov light detector All channels MIP/cable/linear range calibrated Two physics runs: 2016-2017 and 2017-2018

Detector design and simulation Various designs were checked Different PMT positions Different scintillator shapes PMT from the top gives better uniformity as well as circular scintillators Calibration tests are for single MIP detection Bottom of the scintillator is painted in order to increase reflectivity

Detector design and simulation PMT ‘above’ results in statistically significantly higher light yield: 3.65 ± 0.04 detected photon per MIP for ‘above’ 3.19 ± 0.03 for ‘below’ Uniformity increases / saturates depending on position Detected photon number decreases

Signal Width measurements Linearity of the width vs. number of photons detected Linearity holds for 1 MIP and up to 3000 PMT response vs. voltage applied linearity

Time response measuremetns ~ 2.2 ns rise time response (10-50% of the pulse area) of the PMT+glass ~ 1.7 ns pulse width is limited by PMT, ADC characteristics and geometry ~ 5.1 ns total time response (10- 90% of pulse area) of the PMT+glass

Conclusion and Future plans In HT data, ‘unusual’ events have been identified To study it better time resolution is required Rise time of the PMT should match ADC rate Fast time response Far periphery detectors upgrade to larger areas is planned up to 12 m2

references [1] RU Beisembaev, EA Beisembaeva, OD Dalkarov, VA Ryabov, AV Stepanov, NG Vildanov, MI Vildanova, VV Zhukov, KA Baigarin, D Beznosko, TX Sadykov, NS Suleymenov, "The 'Horizon-T' Experiment: Extensive Air Showers Detection," arXiv:1605.05179 [physics.ins-det], May 17 2016. [2] Rashid Beisembaev, Dmitriy Beznosko, Kanat Baigarin, Elena Beisembaeva, Oleg Dalkarov, Vladimi Ryabov, Turlan Sadykov, Sergei Shaulov, Aleksei Stepanov, Marina Vildanova, Nikolay Vildanov, Valeriy Zhukov. "Horizon-T experiment status." EPJ Web Conf. 145 11004 (2017). DOI: 10.1051/epjconf/201614511004 [3] Rashid Beisembaev, Dmitriy Beznosko, Kanat Baigarin, Elena Beisembaeva, Oleg Dalkarov, Vladimir Ryabov, Turlan Sadykov, Sergei Shaulov, Aleksei Stepanov, Marina Vildanova, Nikolay Vildanov, Valeriy Zhukov. " Extensive Air Showers with unusual structure." EPJ Web Conf. 145 14001 (2017). DOI: 10.1051/epjconf/201614514001 ISVHECRI [4] R U Beisembaev, D Beznosko, K A Baigarin, A Batyrkhanov, E A Beisembaeva, T. Beremkulov, O D Dalkarov, A Iakovlev, V A Ryabov, N S Suleimenov, T Kh Sadykov, Z Tagay, T Uakhitov, M I Vildanova and V V Zhukov. "Horizon-T experiment and detection of Extensive air showers with unusual structure", accepted to Journal of Physics: Conference series, 2018 [5]. D. Heck, J. Knapp, J.N. Capdevielle, G. Schatz, T. Thouw. CORSIKA: A Monte Carlo Code to Simulate Extensive Air Showers, Forschungszentrum Karlsruhe Report FZKA (6019). [6]. HAMAMATSU PHOTONICS K.K., Electron Tube Division, 314-5, Shimokanzo, Iwata City, Shizuoka Pref., 438-0193, Japan, http://www.hamamatsu.com [7] R.U. Beisembaev, D. Beznosko, E.A. Beisembaeva, A. Duspayev, A. Iakovlev, T.X. Sadykov, T. Uakhitov, M.I. Vildanova, M. Yessenov and V.V. Zhukov, "Fast and simple glass-based charged particles detector with large linear detection range," Journal of Instrumentation, vol. 12, no. T07008, 2017. [8] D. Beznosko, T. Beremkulov, A. Iakovlev, S. Jakupov, D. Turganov, A. Tussipzhan, T. Uakhitov, M.I. Vildanova, A. Yeltokov, V.V. Zhukov."Horizon-T Experiment Upgrade and Calibration of New Detection Points", arXiv:1803.08309 [physics.ins-det], Mar 22, 2018. [9].CAEN S.p.A. Via della Vetraia, 11, 55049 Viareggio Lucca, Italy. http://caen.it.