Performance of Compton Alignment in OPERA CS, 2008 run Seigo Miyamoto Jan., 2009, MIZUNAMI.

Slides:



Advertisements
Similar presentations
Beam direction and flux measured by MUMON K. Matsuoka (Kyoto) for the MUMON group Contents: 1.Beam stability (direction/flux) 2.Absolute  beam flux.
Advertisements

NAKAMURA M. (NAGOYA Univ.)
Automated analysis of nuclear emulsions using new tracking technique presented by Tsutomu Fukuda ( Toho University ) Workshop on Nuclear Track Emulsion.
Track ranking in CS analysis T. Fukuda 20/Jan ‘09 OPERA–JAPAN (Mizunami) meeting.
SUTS data taking and processing K.Morishima. Introduction to Morishima ・ Refresh ・ Development of Plate Changer ・ Development of Dry lens scanning ・ Development.
Slides for the discussion Cosmic ray density. Cosmic ray density. Cosmic ray is  useful for the alignment between plates. Decay search Momentum measurement.
SUTS Data taking and processing with Monitoring K. Morishima Flab Nagoya Univ. OPERA Emulsion Workshop 2008/01/22-23.
Emulsion scanning: present status and plans for the coming run Giovanni De Lellis.
Support to the event location in CS Scanning Station Fabio Pupilli LNGS Scanning Team OPERA Collaboration Meeting 20/01/2009 MIZUNAMI.
WG-3 summary CS scanning. People O.SatoNagoya Y.NonoyamaNagoya S.MiyamotoNagoya J.YoshidaNagoya T.FukudaNagoya T.NakanoNagoya S.AokiKobe Luigi Salvatore.
Status of the MICE SciFi Simulation Edward McKigney Imperial College London.
OPERA experiment T.Toshito (Nagoya univ. Japan) for the OPERA collaboration Apr
OPERA brick (16215) scanning results Luisa Arrabito on behalf of Lyon Scanning Group Emulsion Workshop Nagoya 22th-23th January 2008.
Gyaku(Inverse) Data Base Y.Nonoyama Nagoya Univ. New idea of Emulsion track link to SFT trigger in PEANUT.
Automatic Track Follow Program A program to trace a given set of tracks automatically –Event location for PEANUT and OPERA –DONUT “not-located” events.
CSd analysis Natalia for the European CS Scanning Team.
Stack to Stack connection O.Sato. Motivation Emulsion coordinate aligned to TT coordinate by Komatsu :: CTransEmulToTT(*); Emulsion tracks.
Reconstruction of neutrino interactions in PEANUT in general scanning (unbiased) mode Giovanni De Lellis on behalf of Andrea Russo Naples University.
Electron identification and shower analysis in ECC T.Toshito (Nagoya Univ.) 8.Mar.2002
CS LNGS Current status and perspectives.
Application of the Beta-ray alignment for the OPERA CSDs Seigo Miyamoto.
I. Kreslo, LHEP, Bern Bern Scanning Laboratory Hunting muonless interactions...
Status of OPERA N. Naganawa (Nagoya University) Flavor physics.
Kouji Narita Nagoya University, Japan CHORUS collaboration Study of charm production in neutrino interactions.
November 24th, 2005OPERA General meeting1 CS facility A. Ariga, M. Kazuyama, S. Hiramatsu Nagoya University Overview Introduction of components.
S. Aoki Kobe University OPERA Emulsion Workshop 2006/12/09 Gamma-ray Telescope.
Film Storage and book-keeping Scanning Quality Control Cosmic Ray Density Vertex Confirmation Vertex Location WG4 summary.
CS Scan report at Nagoya Film samples August run Rock muon events Comic ray events October run Rock muon events 1 event (1 Brick) Cosmic.
NC like event location 9 th /Dec/2006 OPERA Emulsion Work Shop T. Fukuda, K. Morishima, N. Nagoya univ.
Time stamping for Emulsion Tracks with Gyaku Data Base method Y.Nonoyama.
Support to the event location in CS Scanning Station Fabio Pupilli LNGS Scanning Team OPERA Collaboration Meeting 02/04/2009 ANKARA.
CS LNGS Current status and perspectives Luigi Esposito (European CS Scanning Team)
Neutrino Event location Connection from Electric Detector to Emulsion Detector Tsutomu FUKUDA Fundamental Particle Physics Lab, Nagoya-univ 9th March,
Calo Prediction Trial Nagoya University F - LAB Kunihiro Morishima.
CS general status on behalf of JAPAN CS Analysis task force team T.Fukuda, S.Miyamoto, Y.Sakatani, Y.Taira 2nd April, OPERA Collaboration
Umut Kose Neutrino interaction location in the OPERA Experiment New Development of Flavor Physics, , Tennomaru, Gamagori Nagoya University.
The OPERA Experiment 12 th Topical Seminar on Innovative Particle and Radiation Detectors (IPRD10) 7-10 June 2010, Siena, Italy Jonas Knüsel Albert Einstein.
CS Edge part Distortion analysis T.Yoshioka M.Kazuyama.
CS to brick and track follow-up ● Cosmic ray test ● CS scanning ● CS to brick connection ● Track following Napoli Scanning Lab.
Comments on OPERA OPERA is going on. We will have good Tau neutrino interactions within years, if νμ - ντ oscillation is the real solution. New Techniques.
Research History of Tsutomu FUKUDA Tono-Refresh facility Facility construction Mass production shift leader Refreshing control Sensitivity.
Study of compact emulsion spectrometer for identification of neutrino/anti-neutrino interaction OPERA emulsion Nagoya Univ. Chika Fukushima.
Hybrid emulsion detector for the neutrino factory Giovanni De Lellis University of Naples“Federico II” Recall the physics case The detector technology.
CS Brick connection at Nagoya O.Sato
Deformation measurement by compton alignment Satoru Takahashi, Nagoya Univ. OPERA emulsion workshop.
Status of the OPERA experiment Yoshiaki Nonoyama Nagoya Univ.
Tsutomu Fukuda Nagoya University, JAPAN
Operation of and results from OPERA Ciro Pistillo LHEP Bern University CHIPP Plenary meeting Lausanne, EPFL-LPHE September
DE/dX measurement by OPERA film Tsutomu Fukuda (Nagoya Univ) Emulsion work shop (11/12,2005)
OPERA Emulsion Workshop – Nagoya, 7-9 Dec From CS to Brick: first results from low density cosmic ray exposure at LNGS M. De Serio from Bari emulsion.
Muon-raying the ATLAS Detector
Muon absolute flux measurement in anti-neutrino mode A.Ariga 1, C. Pistillo 1, S. Aoki 2 1 University of Bern, 2 Kobe University.
100  m Nuclear emulsions are made of micro- crystals of silver halides (AgBr) dispersed in a gelatin layer. The energy released by ionizing particles.
T2K muon measurement 2014 Momentum module A.Ariga, C. Pistillo University of Bern S. Aoki Kobe University 1.
CHIPP meeting Appenberg, 24 Aug 2009 Preparation for LHC beam, Jeroen van Tilburg 1/15 Jeroen van Tilburg (Universität Zürich) LHCb: Preparation for LHC.
NUCLEAR FRAGMENT SEARCH IN HADRON INTERACTIONS JIRO KAWADA(LHEP, BERN) ANIS BEN DHAHBI (F.S.T *, LHEP) JONAS KNUESEL (LHEP) * Faculty Science of Tunis.
Event Location Rehearsal in PEANUT Bricks OPERA collaboration meeting Gran Sasso, May 2006 Kodama, Sato, Fukuda, Komatsu, Narita, Nonoyama NAGOYA.
Measurement devices Cloud chamber Geiger counter Bubble chamber Nuclear emulsion 2.
G.Sirri – INFN Bologna LNGS /19 Status Report of the Bologna Scanning Lab Bologna Scanning Lab Last activities in the Bologna scanning lab.
Beam direction and flux measured by MUMON K. Matsuoka (Kyoto) for the MUMON group Contents: 1.Horn focusing effect 2.Beam stability (direction/flux) 3.Beam.
Emulsion Test Beam first results Annarita Buonaura, Valeri Tioukov On behalf of Napoli emulsion group This activity was supported by AIDA2020.
Electromagnetic shower reconstruction with emulsion films in the OPERA experiment F. Juget IPH Université de Neuchâtel On behalf of the OPERA collaboration.
Characterization of muon beam in T2K with emulsion detectors A. Ariga, T. Ariga, C. Pistillo AEC-LHEP University of Bern 1.
ICARUS T600: low energy electrons
Nuclear emulsions One of the eldest particle detectors, still used in particle physics experiment (CHORUS, DONUT, OPERA) for its unique peculiarities:
Current Status of The OPERA Experiment
The Status of the OPERA experiment II
Status of the OPERA experiment
Results from OPERA Pablo del Amo Sánchez for the OPERA collaboration
Stability (fitted beam center)
Presentation transcript:

Performance of Compton Alignment in OPERA CS, 2008 run Seigo Miyamoto Jan., 2009, MIZUNAMI.

April, Refreshing OPERA Films Fundamental training to see track with my eyes, treatment,develop emulsion electron shower energy calibration in ECC (10~20GeV) history of my study (The way to establish this technology) The balloon analysis High energy Cosmic rays analysis of atmospheric muon flux I got important data and Idea of MeV electron detection Test experiment and analysis of Compton Alignment momentum calibration in ECC (~1GeV) Development of automatic programs for OPERA CSD Application for Real OPERA CS and quality check CS Manual Check Making Refresh Chamber Making Balloon Chamber and Launching Hardware data analysis

deformation of the films Emulsion film have very good position resolution in the very small area. In 10cm x 10cm position resolution decrease ~20um because the films deform in exposure -> develop -> drying. In the case of CS doublet, bad alignment makes many fake coincidence.

Electron from natural R.I. ~ 1 MeV ~ 100 keV

Deformation Calibration by finding MeV electron peak 10μm Δx from X-ray Alignment

SCAN CS1CS2 SCAN micro track Making base track Compton Alignment base track calibration map Doublet Track Selection (4hold, 3hold, muon selection) Manual Confirm These processes performs fully automatically, which is controlled by Morishima. TT Hit Automation of CS track selection

Automation of getting the deformation map 1. Division of scanning area (5mm x 5mm) 2. Peak search Detection of Compton electrons in the Shift_x,y map for all divided areas 3. Estimation that each alignment is successful or not in each divided areas. 4. Linear interpolation for not successful areas 5. Estimation performance for all areas.

Evaluation performance of Compton Alignment Samples are 425 CSDs scanned in Japan (~early Dec., 2008.) No available alignment in any scanning region 5 (1%) Getting good alignment pattern map (at least 5cm 2, and they are adjoining ), and # of pattern = 1 347(82%) # of pattern is >= 273(17%)

Ratio successful area Samples are 420 CSDs (at least 5cm 2 is available, and including multiple pattern) # of CSD ratio successful is more than 80% is about 360(85%). The Areas couldn’t get available alignments are almost due to large gaps. ~85%

Alignment accuracy Samples are 163 muon track that observed in CSD ( ratio successful is more than 80% ) from beginning to early Dec., Residual from X-ray Alignment 5.5um7.6um

Alignment accuracy Samples are 163 muon track that observed in CSD ( ratio successful is more than 80% ) from beginning to early Dec., Residual from Compton Alignment 2.0um

Summary Compton Alignment is applied for all CSDs full automatically in 2008 RUN. 99% CSD succeed to get alignment at least 5cm 2, and multi pattern is about 17%. CSD - its ratio successful is more than 80% - is about 85%. Alignment accuracy is 2um, BG reduction power is around 1/10.

Future Plan: General MeV electron Detector which has micron position resolution Material Science -Study of Structural Phase Transitions ( Dr. Tanimura (Osaka univ.) presented in Emulsion WorkShop 2008.) Any other ideas ( It’s secret. )