M. Fraga, Prague, May 17th. 2006 The role of temperature on air fluorescence measurements M. Fraga 1, A. Onofre 1,2, N. F. Castro 1, F. Fraga 1, L. Pereira.

Slides:



Advertisements
Similar presentations
USE OF GEANT4 FOR LHCB RICH SIMULATION S. Easo, RAL, LHCB AND ITS RICH DETECTORS. TESTBEAM DATA FOR LHCB-RICH. OVERVIEW OF GEANT4 SIMULATION.
Advertisements

Analysis of the Optical Properties of Organic Liquid Scintillator in LENA DPG-Tagung in Heidelberg M. Wurm, T. Marrodán Undagoitia, F. v. Feilitzsch,
LENA Scintillator Characterization Transregio 27 SFB-Tage in Heidelberg 9/10. Juli 2009 Michael Wurm.
for Fusion Power Monitoring
DHC 101 Introduction to scintillation detectors. How many PE/MIP should we expect? Scintillation & Fluorescence WSFWSF PMTPEs  (MIP)
Measuring the Speed of Light! Photonic partners: David Orenstein Anuta Bezryadina Nathan Burd.
S. Bricola, A. Menegolli, M. Prata, M.C. Prata, G.L. Raselli, M. Rossella, C. Vignoli INFN and University of Pavia - Via Bassi, 6 – Pavia – Italy.
Computed Tomography RAD309
FIWAF 10/2002Pierre COLIN 1 a measurement of the fluorescence light in UV emitted by various gas (air, pure N 2...) when high-energy charged particles.
PERFORMANCE OF THE DELPHI REFRACTOMETER IN MONITORING THE RICH RADIATORS A. Filippas 1, E. Fokitis 1, S. Maltezos 1, K. Patrinos 1, and M. Davenport 2.
HiRes Usage. Outline ● Shower energy ( Size, dE/dx ) ● Atmospheric profile ( stdz76, radiosonde) ● Rayleigh Scattering ● Aerosols Model ( density, variability.
Fluorescence from Air in Showers (FLASH) J. Belz 1, Z. Cao 2, P. Chen 3*, C. Field 3, P. Huentemeyer 2, W-Y. P. Hwang 4, R. Iverson 3, C.C.H. Jui 2, T.
Downstream e-  identification 1. Questions raised by the Committee 2. Particle tracking in stray magnetic field 3. Cerenkov and calorimeter sizes 4. Preliminary.
Types of Analyses Single Collector –Uses only one collector or detector –This is the case with a Daly or EM Advantages: –Need only one detector –Peaks.
Characterization of CF 4 primary scintillation Andrey Morozov.
Geant4 simulation of the attenuation properties of plastic shield for  - radionuclides employed in internal radiotherapy Domenico Lizio 1, Ernesto Amato.
Hamamatsu R7525 HA: outer conductive coating with insulating sleeve CC: convex-concave window mm thick (standard plano-concave: 1mm center, 6.1.
Kinetic-Molecular Theory Describes the behavior of an “ideal” gas in terms of particle size, motion, and energy based on 5 assumptions…
EXL/crystal simulations B. Genolini Simulation of NUSTAR crystals with Litrani Presentation of Litrani: simulation of.
Study of plastic scintillator quenching factors Lea Reichhart, IOP Glasgow, April /17.
Modelling of Electron Air Showers and Cherenkov Light A.Mishev J. Stamenov Institute for Nuclear Research and Nuclear Energy Bulgarian Academy of Sciences.
Development of A Scintillation Simulation for Carleton EXO Project Rick Ueno Under supervision of Dr. Kevin Graham.
Cube Measurements Tent Crew. Scintillation BNL 241 Am Semi- collimated  Spectralon Diffuse UV Reflector SBD  -Trigger Scint. Light Poisson.
Physics 1 Revision Lesson 2 Factors affecting cooling and Insulating buildings.
1 Fast Timing via Cerenkov Radiation‏ Earle Wilson, Advisor: Hans Wenzel Fermilab CMS/ATLAS Fast Timing Simulation Meeting July 17,
18/05/06P. Nedelec - 4th Air Fluorescence Workshop Measurements of FLY with MACFLY.
BNL/ Tatsuya CHUJO CNS workshop, Tokyo Univ. Identified Charged Single Particle Spectra at RHIC-PHENIX Tatsuya Chujo (BNL) for the PHENIX.
EPECUR – Investigation of narrow baryon resonances Konovalova Elena St. Petersburg Nuclear Physics Institute (PNPI) with collaboration Institute of Theoretical.
E-165 (FLASH) Experiment Status Report Johnny S.T. Ng SLAC EPAC Meeting, Nov. 15, 2003.
Gwenaëlle LEFEUVRE APC-Collège de France, Paris, France paris7.fr.
The Experimental Program of the “FLASH” Experiment.
Effect of air fluorescence properties on the reconstructed energy of UHECR José Ramón Vázquez, María Monasor, Fernando Arqueros Universidad Complutense.
T. Sugitate / Hiroshima / PHX031 / Nov.01 The Photon Spectrometer for RHIC and beyond PbWO 4 Crystal Density 8.29 g/cm 3 Radiation length 0.89 cm Moliere.
Temperature behaviour of threshold on broad area Quantum Dot-in-a-Well laser diodes By: Bhavin Bijlani.
A gas scintillation proportional counter for thermal neutron scattering measurements D.Raspino, N.J.Rhodes, E.M.Schooneveld (ISIS-STFC), I.Defendi, M.Jurkovic,
work for PID in Novosibirsk E.A.Kravchenko Budker INP, Novosibirsk.
1 5-9 October th ICATPP, Como, Italy S. Maltezos NITROGEN MOLECULAR SPECTRA OF AIR FLUORESCENCE EMULATOR USING A LN 2 COOLED CCD S. Maltezos, E.
1 Satoshi Mihara for the   e  collaboration, review meeting at PSI, Jul 2002 Photon Detector Satoshi Mihara ICEPP, Univ. of Tokyo 1.Large Prototype.
1 CF4 Scintillation and Aging LIP - Coimbra Luís Margato Andrei Morozov Luís Pereira Margarida Fraga Francisco Fraga.
VHEPU Mar-2005 P. N édélec - LAPP Air Fluorescence Light Yield Measurements Summary of the IWFM05 Workshop Thanks.
MPPC status M.Taguchi(kyoto) T2K ND /7/7.
Filipe Castro Departamento de Física & i3n Universidade de Aveiro C S I(N A ) W AVELENGTH - SHIFTING FIBER GAMMA CAMERA USING S I PM S LIP Lisboa Apr.
Xe-TMA update ANDRÉ CORTEZ Laboratory of Instrumentation and Experimental Particle Physics (LIP-Coimbra) Physics Department University of Coimbra Coimbra,
Radioactive source and cosmic-ray test for the MWPC Davide Pinci on behalf of the Frascati-Roma1 MWPC group.
Atmospheric Radio Soundings in Argentina - Effects of Air Density Variations - Forschungszentrum Karlsruhe in der Helmholtz-Gemeinschaft Bianca KeilhauerTokyo,
1 Neutron Effective Dose calculation behind Concrete Shielding of Charge Particle Accelerators with Energy up to 100 MeV V. E Aleinikov, L. G. Beskrovnaja,
Development of a new Building Energy Model in TEB Bruno Bueno Supervisor: Grégoire Pigeon.
Collection of Photoelectrons from a CsI Photocathode in Triple GEM Detectors C. Woody B.Azmuon 1, A Caccavano 1, Z.Citron 2, M.Durham 2, T.Hemmick 2, J.Kamin.
THIN FILMS FOR CLIC ELEMENTS Outline Motivation The role of MME-CCS DB and MB transfer lines Main beam Main beam quadrupoles Other issues conclusions CLIC.
The Double Chooz Monte Carlo (selected topics !) Dario Motta (Irfu/SPP) Anatael Cabrera (APC)
Development of a Single Ion Detector for Radiation Track Structure Studies F. Vasi, M. Casiraghi, R. Schulte, V. Bashkirov.
Photon Transport Monte Carlo September 27, 2004 Matthew Jones/Riei IshizikiPurdue University Overview Physical processes PMT and electronics response Some.
P HOTON Y IELD DUE TO S CINTILLATION IN CF4 Bob Azmoun, Craig Woody ( BNL ) Nikolai Smirnov ( Yale University )
Applications of the GEM at high pressure for neutrons and X-rays T.L. van Vuure , R. Kreuger , C.W.E. van Eijk  and R.W. Hollander , L. M. S. Margato.
Present status of production target and Room design Takashi Hashimoto, IBS/RISP 2015, February.
Seoul National University Han-wool Ju CUNPA Kick-off Meeting Aug.22-23, 2013.
R&D Plan on Light Collection Takeyasu Ito Los Alamos National Laboratory.
Forschungszentrum Karlsruhe Erice, 7th July th International School for Cosmic Rays Astrophysics Motivation Energy Reconstruction Air Fluorescence.
Study of the cryogenic THGEM-GPM for the readout of scintillation light from liquid argon Xie Wenqing( 谢文庆 ), Fu Yidong( 付逸冬 ), Li Yulan( 李玉兰 ) Department.
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.
Precise measurement of air fluo yield
Simplified Study of Storey Configurations
KM2A Electron Detector Optimization
Siara Fabbri University of Manchester
Particle Identification in LHCb
Measuring the Speed of Light!
Deng Ziyan Jan 10-12, 2006 BESIII Collaboration Meeting
COMPTON SCATTERING IN FORWARD DIRECTION
Presentation transcript:

M. Fraga, Prague, May 17th The role of temperature on air fluorescence measurements M. Fraga 1, A. Onofre 1,2, N. F. Castro 1, F. Fraga 1, L. Pereira 1, F. Veloso 1, P. Vieira 1, R. Ferreira Marques 1, M. Pimenta 3, A. Policarpo 1 J. A. C. Gonçalves 4, C. C. Bueno 4 1 LIP- Coimbra, Dep. Física, Univ. Coimbra, Coimbra, Portugal 2 UCP, R. Dr. Mendes Pinheiro, 24, 3080 Figueira da Foz, Portugal 3 LIP-IST, Av. Elias Garcia 14, Lisboa, Portugal 4 IPEN and PUC, S. Paulo, Brasil

M. Fraga, Prague, May 17th Layout: Theory; Experimental set-up; Previous measurements taken with alpha particles as excitation source (Nc versus T for  = const.); Simulation of the chamber and correction factors evaluation; Corrected data versus T and comparison with recent measurements; Further tests – the need of a precise knowledge of the behaviour all the components of the experimental set up; Conclusions and plans for the future

M. Fraga, Prague, May 17th In steady state conditions, the light yield for the v’v’’ band is given by: with The rate constant is given by: F (  ) represents the fraction of the excitation processes which produce photons that arrive at the PMT window. N 2 scintillation 2nd positive system ( nm)

M. Fraga, Prague, May 17th Experimental set-up and data (raw) on Dec – Jan PM1, PM2 - XP2020Q Cooling unit to vacuum pump gas input PM3 Excitation source:  particles (5.4 MeV)

M. Fraga, Prague, May 17th Am-241 source outside the chamber, exposed to air –For a constant , as the temperature is lowered, the energy loss outside the chamber increases: the mean energy,, with which the a particle enters the chamber is lower for lower temperatures; the length of the  track is also shorter for lower temperatures ;  y = 6 mm

M. Fraga, Prague, May 17th Filter Transmission * : T(  i ) Filter: Melles Griot, c = 340 nm;  = 10 nm For small angles of incidence,  i * S. Klepser, AirLight 03, Dec. 2003, Bad Liebenzell, Germany. 0º Transmission curve as given by the manufacturer Otherwise it has to be measured:

M. Fraga, Prague, May 17th Monte Carlo simulation using GEANT4 code * Outside the chamber: air (273 K) air (273 K) Inside:  N 2 (336 hPa at 20ºC) = 46 mm N 2 (818 hPa at 20ºC)  = 22 mm P air < 0.1 torr Outside the chamber: P air < 0.1 torr Inside: Dry air (434 hPa at 20ºC) 5 events * Note: pressure effects on light yields are not included in the simulation

M. Fraga, Prague, May 17th Results of simulation: typical F (  factors with air at 1013 hPa outside the chamber Uncertainties in /  : < 2% - due to variations of atmospheric pressure < 1% - due temperature variations 818 hPa336 hPa dE/dx

M. Fraga, Prague, May 17th Introducing the corrections to the experimental data (0-0 band)... one gets...

M. Fraga, Prague, May 17th  Light yield versus t (ºC). Values are corrected for the geometrical factors and different energy losses inside the chamber. For constant  one would expect that: and or  Inverse of light yield versus.

M. Fraga, Prague, May 17th Dependence of Light Yield on Pressure, at room temperature Inverse of light yield versus pressure at room temperature (0-0 band at 337 nm) B/A = (5.8±1.4)×10 -3 hPa -1 k 20 /k 10 For T = constant,

M. Fraga, Prague, May 17th Improvement in the experimental set-up: very low pressure in the region of the alpha source

M. Fraga, Prague, May 17th Experimental data with the  source in a low pressure atmosphere

M. Fraga, Prague, May 17th Fraction of the alpha particle energy, lost in the gas.  particle source in a low pressure environment. Correction factors : For P 20º = 243 hPa, (#coinc/s) Patm /(#coinc/s) low P = 1.26 ± 0.03 and Patm / low P = 1.16 ± 0.08

M. Fraga, Prague, May 17th Dry Air - N 2 + O 2 (80:20) Dry Air - N 2 + O 2 (80:20) (H 2 O < 3 ppm, C n H m < 0.5 ppm) O 2 – (20 ±1) %

M. Fraga, Prague, May 17th Further corrections: variation of the PMT gain with T m = (±0.008) #/ºC for  = 337 nm; Variation of quantum efficiency of the photocathode with T – in progress Variation of the transmission of the interference filter with T – in progress

M. Fraga, Prague, May 17th Study of the transmission of the IF Set-up : Data from Melles Griot

M. Fraga, Prague, May 17th Conclusions and plans for the future A coherent set of results were obtained under  particle excitation. The expected dependence on T is not clear from the present set of experimental data and further studies and tests are needed (and they are underway). An important issue is to lower the temperature of the gas below -20º ; this implies improvements on the experimental set-up (studies are underway). Simulation of the chamber will go on. Measurements using  particles (Sr-90) (already underway) will be carried out ;