EUSO Atmospheric Monitoring from Space M.Teshima on behalf of the EUSO collaboration MPI für Physik, München (Werner-Heisenberg-Institut)

Slides:



Advertisements
Similar presentations
AGASA Results Max-Planck-Institut für Physik, München, Germany Masahiro Teshima for AGASA collaboration at 3 rd Int. Workshop on UHECR, Univ. Leeds.
Advertisements

Calibration for LHAASO_WFCTA Yong Zhang, LL Ma on behalf of the LHAASO collaboration 32 nd International Cosmic Ray Conference, Beijing 2011.
The First Flight of EUSO Balloon a prototype of JEM-EUSO Jim Adams a, Evgeny Kuznetsov a, Matthew Rodencal a, Jurgen Sawatzki a, Mark Christl b, Lawrence.
EUSO Onboard LIDAR M.Teshima Discussion by Valentin Mitev Neuschatel Observatory
Low Energy, Low Cost Swift A design experiment June 2010.
Probing the HiRes Aperture near eV with a Distant Laser C. Cannon, L. Pedersen, R. Riehle, M. Seman, J. Thomas, S. Thomas, L. Wiencke for the HiRes.
CRAYS and TA telescope calibration ICRR N. Sakurai, M. Fukushima Utah University L. Wiencke.
The Pierre Auger Observatory Nicolás G. Busca Fermilab-University of Chicago FNAL User’s Meeting, May 2006.
EUSO: Extreme Universe Space Observatory Jessica Cerny Bancroft-Rosalie School.
AGASA update M. Teshima ICRR, U of CfCP mini workshop Oct
Characterization of Orbiting Wide-angle Light-collectors (OWL) By: Rasha Usama Abbasi.
Systematics in the Pierre Auger Observatory Bruce Dawson University of Adelaide for the Pierre Auger Observatory Collaboration.
SPHERE PEG GAY FAIRBURY JR SR HIGH SCHOOL. PROJECT SPHERE  Cherenkov light: radiation which is emitted whenever charged particles pass through matter.
Leroy Nicolas, HESS Calibration results, 28 th ICRC Tsukuba Japan, August Calibration results of the first two H·E·S·S· telescopes Nicolas Leroy.
Atmospheric Monitoring in the TA experiment
B. Gentry/GSFCSLWG 06/29/05 Scaling Ground-Based Molecular Direct Detection Doppler Lidar Measurements to Space Using Wind Profile Measurements from GLOW.
- Functional Requirements - Background - Examples of expected Signal Track - An “idea” of angular resolution EUSO-BALLOON DESIGN REVIEW, , CNES.
The Lidar System for the Pierre Auger Observatory A shifter´s point of view. To obtain reliable calorimetric information from the fluorescence stations,
The Second International Workshop on Ultra-high-energy cosmic rays and their sources INR, Moscow, April 14-16, 2005 from Extreme Universe Space Observatory.
Space fluorescence detectors TUS/KLYPVE for study of UHECR. (Italian-Russian seminar on space detectors) 19 October 2005 B. A. KHRENOV 19 October 2005.
TUS Experiment: A space fluorescence detector for study of EECR TUS Experiment: A space fluorescence detector for study of EECR Humberto Salazar for the.
Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays Paolo Privitera Carlos Hojvat Fermilab, June FD SD.
The Experimental Program of the “FLASH” Experiment.
Measurement of the UHECR energy spectrum from hybrid data of the Pierre Auger Observatory Presenter: Lorenzo Perrone Università del Salento and INFN Lecce.
Why Neutrino ? High energy photons are absorbed beyond ~ 150Mpc   HE  LE  e - e + HE s are unique to probe HE processes in the vicinity of cosmic.
Moon shadow analysis -- Using ARGO experiment Wang Bo, Zhang Yi, Zhang Jianli, Guo Yiqing, Hu Hongbo Apri for NanJing Meeting
GSFC Scanning Holographic Receivers for Air and Space Geary Schwemmer Meeting of the Working Group on Space-based Lidar Winds Sedona, Arizona January 27.
Atmospheric Aerosol Measurements at the Pierre Auger Observatory The Pierre Auger Observatory operates an array of monitoring devices to record the atmospheric.
Analysis chain for MAGIC Telescope data Daniel Mazin and Nadia Tonello Max-Planck-Institut für Physik München D.Mazin, N.Tonello MPI for Physics, Munich.
Ultra High Energy Cosmic Rays -- Origin and Propagation of UHECRs -- M.Teshima Max-Planck-Institut f ü r Physik, M ü nchen Erice Summer School July
E.Plagnol - TA/TALE feb Acceptance and Counting Rates of EUSO ë Detecting UHECR from space ë The EUSO detector : Who does what. ë Some characteristics.
Claudio Di Giulio University of Roma Tor Vergata, INFN of Roma Tor Vergata IDAPP 2D Meeting, Ferrara, May The origin and nature of cosmic rays above.
Andrii Neronov JEM-EUSOJEM-EUSO. Problem of the origin of cosmic rays Galactic Extragalactic?
Ground and satellite-based night-time cloud identification techniques
Space fluorescence detectors TUS/KLYPVE for study of EECR. M.I. Panasyuk and B.A. Khrenov D.V.Skobeltsyn Institute of Nuclear Physics of the Moscow State.
HiRes 5Y Operations – Program and Context What Physics Will be Done? How Does it Compare With Other Projects?
Stefano Argirò 1 for the Auger Collaboration 1 University of Torino, Italy, and INFN Physics case The Auger Observatory Performance Preliminary Analysis.
Design for Wide FOV Cherenkov telescope upgrading THE 2 nd WORKSHOP OF IHEP Shoushan Zhang Institute of High Energy Physics.
T. Suehara, H. Yoda, T. Sanuki, Univ. of Tokyo, T. Kume, Y. Honda, T. Tauchi, High Energy Accelerator Research Organization (KEK) ATF2-IN2P3-KEK kick-off.
Hybrid measurement of CR light component spectrum by using ARGO-YBJ and WFCTA Shoushan Zhang on behalf of LHAASO collaboration and ARGO-YBJ collaboration.
1 João Espadanal, Patricia Gonçalves, Mário Pimenta Santiago de Compostela 3 rd IDPASC school Auger LIP Group 3D simulation Of Extensive Air.
The Auger Observatory for High-Energy Cosmic Rays G.Matthiae University of Roma II and INFN For the Pierre Auger Collaboration The physics case Pierre.
Exploring Laser Light Ruben Conceição. Pierre Auger Observatory Ultra High Energy Cosmic Rays Pierre Auger Observatory – Fluorescence Detector Longitudinal.
A Future All-Sky High Duty Cycle VHE Gamma Ray Detector Gus Sinnis/Los Alamos with A. Smith/UMd J. McEnery/GSFC.
Atmospheric Monitoring at HiRes Status Enhancements Lawrence Wiencke HiRes NSF Review Nov Washington DC.
A Cross Check of Atmospheric Attenuation for the High Resolution Fly’s Eye Astroparticle Experiment Chris Cannon Advisor: Lawrence Wiencke University of.
Measurement of the UHECR energy spectrum from hybrid data of the Pierre Auger Observatory Presenter: Lorenzo Perrone Università del Salento and INFN Lecce.
Geant4 Simulation of the Pierre Auger Fluorescence Detector
Exploring an evidence of supermassive black hole binaries in AGN with MAXI Naoki Isobe (RIKEN, ) and the MAXI
D.V.Skobeltsyn INP Moscow State University “Energia” Korolev (Rocket Space Corporation) “Luch” Syzran SCTB, Russia JINR, Dubna, Russia Mexico University,
Probing the HiRes Aperture near eV with a Distant Laser C. Cannon, L. Pedersen, R. Riehle, M. Seman, J. Thomas, S. Thomas, L. Wiencke for the HiRes.
The Large High Altitude Air Shower Observatory LHAASO.
The JEM-EUSO Mission to Explore the Extreme Universe Toshikazu Ebisuzaki RIKEN for the JEM-EUSO Collaboration Toshikazu Ebisuzaki RIKEN for the JEM-EUSO.
Demonstration for cm-size space debris REDUCTION/REMEDIATION from the International Space Station Toshikazu Ebisuzaki, S. Wada, L.W. Pitrowski, M. Casolino.
Shoushan Zhang, ARGO-YBJ Collaboration and LHAASO Collaboration 4 th Workshop on Air Shower Detection at High Altitude Napoli 31/01-01/ IHEP (Institute.
NLC – The Next Linear Collider Project Colorado Univ. - Boulder Calorimetry-Arlington Calorimetry Detector Study Plans at Colorado Uriel Nauenberg for.
Measurement of the CR light component primary spectrum B. Panico on behalf of ARGO-YBJ collaboration University Rome Tor Vergata INFN, Rome Tor Vergata.
TA-EUSO: First simulation study and status
HiRes 5Y Operations – Program and Context
The EUSO-SPB mission Valentina Scotti INFN Sezione di Napoli.
Atmospheric Aerosol Characterization using
Ultra High Energy Cosmic Ray Spectrum Measured by HiRes Experiment
Pierre Auger Observatory Present and Future
30th International Cosmic Ray Conference
Absolute energy calibration of
大気モニタR&D Atmospheric Monitoring for TA
Monitor of All sky X-ray Image (MAXI)
Electron Beam as a standard candle for EHECR air shower
The Aperture and Precision of the Auger Observatory
Shanghai Institute of Technical Physics , Chinese Academy of Science
Presentation transcript:

EUSO Atmospheric Monitoring from Space M.Teshima on behalf of the EUSO collaboration MPI für Physik, München (Werner-Heisenberg-Institut)

EUSO Concept Large Distance and Large F.O.V.  Large Aperture ~6x10 5 km 2 sr ~6x10 5 km 2 sr Good Cosmic Ray detector 3000 times sensitive to C.R. bursts ~2000 Giga-ton atmosphere ~2000 Giga-ton atmosphere Good neutrino detector All Sky coverage North and south sky covered uniformly. ISS orbit: ~50°inclination. North and south sky covered uniformly. ISS orbit: ~50°inclination. Complementary to the observation from the ground Different energy scale Different energy scale Different systematic errors Different systematic errors Shower Geometry is well defined Constant distance from detector Constant distance from detector Attenuation correction is minimum!!

Atmospheric monitoring in EUSO IR ~10μm CCD camera (256x256), UV CCD Camera IR: Cloud monitor (clould looks colder than the ground temperature) IR: Cloud monitor (clould looks colder than the ground temperature) UV; Detection of lightening and other background, for example, air plane flash UV; Detection of lightening and other background, for example, air plane flash Ground Light Source; Complimentary to Onboard lidar Ground based LIDAR system, stations Ground based LIDAR system, stations Flashers, Hamamatsu L6604 Flashers, Hamamatsu L ground stations + NASA research aircraft P-3B flashes/station can be used for monitoring Onboard LIDAR system Power and mass budget Power and mass budget Effectiveness on the analysis Effectiveness on the analysis Current Baseline design Current Baseline design one color 1064nm LIDAR system, 50mJ/100Hz, 140kg, 300W Blind LIDAR for EUSO Information Information top of thick cloud altitude Thin cloud transmission at 1000nm

Flasher and the intensity Integrated transmission can be measured Hamamatsu L6604 ~1J/shot

Flasher Image on EUSO FS ~30Hz flash rate 0.05 deg / flash Total ~1000 flashes EUSO FOV EUSO ~16km/s

50mJ Nd: YAG Ground LIDAR Define beam intensity in each laser path by G.B.L. Transmissions between space and various altitude Simulate shower track Check reconstruction quality Check reconstruction quality End to end experimental calibration End to end experimental calibration 10stations  ~1/day

Lidar Image on EUSO FS 100Hz shot rate 0.01 deg / shot Total ~3000 shots Good simulation for Cherenkov + fluorescence EUSO ~16km/s EUSO FOV