PEANUT Brick Scanning for NETSCAN by S-UTS Kunihiro Morishima F-Lab Nagoya University BL118 Peanut Fermi Lab 2007/01/22-23.

Slides:



Advertisements
Similar presentations
The Principles of Design
Advertisements

We are now working with 2 microscope: 1st Microscope Official setup: MICOS stage NIkON optics and illuminator DALSA camera cad-4 Recently several hardware.
1 Status report of the PEANUT analysis Giovanni De Lellis Collaboration Meeting, June 5th 2007, Maiori.
Automated analysis of nuclear emulsions using new tracking technique presented by Tsutomu Fukuda ( Toho University ) Workshop on Nuclear Track Emulsion.
Π 0 search N.Kitagawa Flab Nagoya University OPERA Emulsion Workshop 2008/01/22-23.
Status of the Bologna scanning laboratory G. Sirri for the Bologna Group* Nagoya 7-9 Dec 06 Bologna Group: L. Consiglio (PhD), M. Cozzi, D. Di Ferdinando.
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.
Vertex location status of Japan Nagoya vertex hunting team Y.Nonoyama, K.Hamada, S.Takahashi, H.Kubota, R.Komatani 2009 Jan 22 OPERA Japan Meeting.
Performance of Compton Alignment in OPERA CS, 2008 run Seigo Miyamoto Jan., 2009, MIZUNAMI.
Experimental investigations of the flow during the stage separation of a space transportation system Andrew Hay Aerospace Engineering with German.
A short “physical” self introduction I’m Naotaka Naganawa from Nagoya University. I’d been working for emulsion development and compatibility between it.
Volume Scan 福田 努 (Tsutomu Fukuda) Nagoya-univ.. Event Brick#CC/NC Stop Plate CC PL CC PL NC PL
Cristiano Bozza – European Emulsion Scanning Group – Nagoya Jan OPERA brick scanning by the European Scanning System.
Automatic Track Follow Program A program to trace a given set of tracks automatically –Event location for PEANUT and OPERA –DONUT “not-located” events.
NetScan for BL118 PEANUT Fermilab 22-23/Jan/2007.
Stack to Stack connection O.Sato. Motivation Emulsion coordinate aligned to TT coordinate by Komatsu :: CTransEmulToTT(*); Emulsion tracks.
CS Distortion Kazuyama Yoshioka. Scanning Samples Realistic CS film x 10  2 nd refresh from ’06 July (include Aug. run TTCS)  Some are installed to.
Reconstruction of neutrino interactions in PEANUT in general scanning (unbiased) mode Giovanni De Lellis on behalf of Andrea Russo Naples University.
Edge Scanning: new plate design for the European Scanning System G. Sirri for Bologna group.
Emulsion Scanning System “SUTS”. Follow Shot Optics.
E-pair Search in CSD Tsutomu Fukuda Nagoya-univ..
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.
Vertex localization in Lyon Emulsion Workshop 7th-9th Dec. 2006, Nagoya Luisa Arrabito – IPN Lyon.
NC like event location 9 th /Dec/2006 OPERA Emulsion Work Shop T. Fukuda, K. Morishima, N. Nagoya univ.
CS LNGS Current status and perspectives Luigi Esposito (European CS Scanning Team)
BL007, BL039 and BL040 PL01-PL02 Scanning Result K. Narita Nagoya University Dec PEANUT meeting.
Wide Field Scanning K. Morishima Nagoya University.
PEANUT meeting Fermilab Giovanni and Komatsu 23/Jan./2007.
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.
Status of “Full scanning” 2007/ 03/ 26 Y.Nonoyama.
Umut Kose Neutrino interaction location in the OPERA Experiment New Development of Flavor Physics, , Tennomaru, Gamagori Nagoya University.
PEANUT exposure summary and brick distribution and Situation of PEANUT analysis Fermilab.
1 Status of Located Event Analysis On behalf of Nagoya Scanning Group Umut KOSE OPERA Emulsion Workshop, January 2008, Nagoya, JAPAN.
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.
Virtual Alignment alignment technique for no CR exposure or very low density case Satoru Takahashi Nagoya Univ.
CS Brick connection at Nagoya O.Sato
Status of the OPERA experiment Yoshiaki Nonoyama Nagoya Univ.
Emulsion quality WG2 report Thanks to all the OPERA colleagues who are engaged on handling and developing emulsion.
G.Sirri – INFN Bologna videconf Fiducial Mark Finding with ESS 1/6 VersionDateBinarySourceConfigNote zip same as 62 Recommended.
LNGS Scanning Station Nicola D’Ambrosio (LNGS group) Maiori, 4-6 June 2007.
LNGS 25 May 2005 G. Sirri – INFN BO1 Test of a dry objective with correction collar Dry objectives having an high numerical aperture give aberration when.
Jean Favier LAPP CERN Physics and soft meeting 23/04/04 Why Monte-Carlo ? To understand and separate influences of parameters (ex: fog d, distorsions,m.i.p.
DE/dX measurement by OPERA film Tsutomu Fukuda (Nagoya Univ) Emulsion work shop (11/12,2005)
G.Sirri – INFN Bologna 1/19 Lateral X-ray marks finding with ESS  Goal: implementation of the lateral mark finding in the ESS software  First Test: Plate-to-plate.
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.
G. Sirri - Bologna videoconf /9 Lateral X-rays with ESS  Goal: implementation of the lateral mark finding in the ESS software  test version.
Changeable Sheet A.Ariga, Nagoya univ. CS strategy R&D~2004-Oct –BG rejection Distortiondistortion itself, precise measurement, packing Self-Refreshparameter.
1 SUTS ariga. SUTS Track Recognition Board 10 FPGA for track recognition, 1 FPGA for communication 40cm2/h scanning power / board.
Ch23
100  m Nuclear emulsions are made of micro- crystals of silver halides (AgBr) dispersed in a gelatin layer. The energy released by ionizing particles.
OPERA Physics Coordination, CERN, 03/05/2006 Effect of  and  radiation on the on-line emulsion scanning M. Cozzi for the Bologna group.
European Scanning System: status report. DRY Fill factor 92.4 ± 1.6 % DB-driven Scan-back and Total Scan in Bari OIL Fill factor 93.1 ± 1.2 % Brick #8,
T2K muon measurement 2014 Momentum module A.Ariga, C. Pistillo University of Bern S. Aoki Kobe University 1.
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.
Better automation for lateral mark alignment 2 additional camera for measurement of marks. – 4 marks with 2 steps by fixing on main optics Idea of 2 additional.
G.Sirri – INFN Bologna LNGS /19 Status Report of the Bologna Scanning Lab Bologna Scanning Lab Last activities in the Bologna scanning lab.
Emulsion Test Beam first results Annarita Buonaura, Valeri Tioukov On behalf of Napoli emulsion group This activity was supported by AIDA2020.
Wide Field Scanning K. Morishima Nagoya University.
Lecture 53: X-ray crystallography. Electrons deflect x-rays We try to recreate electron density from the x-ray diffraction pattern Each point in space.
Nuclear emulsions One of the eldest particle detectors, still used in particle physics experiment (CHORUS, DONUT, OPERA) for its unique peculiarities:
The Status of the OPERA experiment II
Edge Scanning: new plate design for the European Scanning System
Model Reversion : A Client : Slider qty : 1 Model : Latte 2nd
Italian Lab Meeting-CETARA September 2010
Presentation transcript:

PEANUT Brick Scanning for NETSCAN by S-UTS Kunihiro Morishima F-Lab Nagoya University BL118 Peanut Fermi Lab 2007/01/22-23

First data taking of S-UTS 2 nd stage

S-UTS 2 nd Stage scanning speed : 33 cm 2 / hour Speed : 50 views / sec Optics : Tiyoda 50 magnitude lens Field of view : 160 x 160 micron 2 Scanning step : X:135 micron, Y:135 micron

Scanning area 35 mm 25 mm 50 mm Stage Coordinate X Y 25 cm 2

Prediction and Scanning Flow Scanning Direction 1 prediction lens side stage side 10 lines Scanning order X Y 5mm x 1400 micron : 100 sec

Parameter of scanning ・ Angle Allowance : tan θ<= 0.4 ・ Ph cut lens side : 8 ( tan θ< 0.1 ), 7 ( 0.1 =< tan θ ) stage side : 7 ( tan θ< 0.1 ), 6 ( 0.1 =< tan θ ) Parameter of Ph cut depends on thickness of emulsion at scanning Thickness of Lens side is more thin than stage side about 5 micron

Film thickness at scanning 44 micron at exposure Difference between lens side and stage side is about 5 micron

Plate Setting Optics : objective lens Emulsion immersion oil vacuum channel oil fence Scanning area

Position Distribution pl08 Lens side 1000 trks / view

pl08 stage side Position Distribution 2000 trks / view

Angle Distribution Stage side Lens side pl06 ・ Ph cut lens side : 8 ( tan θ< 0.1 ) 7 ( 0.1 =< tan θ ) stage side : 7 ( tan θ< 0.1 ) 6 ( 0.1 =< tan θ )

PH Distribution pl21 lens sidestage side Ph cut = 7 Ph cut = 6 Thickness = 31 Thickness = 37

Number of Tracks in 25cm 2 ( 1plate ) hundred million 1 hundred million tracks / plate 2 hundred million tracks / plate

Scanning Time Average time = 2h15min / plate

Total data taking speed 1 brick / 10 days re-scanning, Because data taking was failure ・ 25cm 2 / both side / plate ・ 1shift / 18h / day

checking quality of data in whole area

Position Distribution pl08 Lens side

pl08 Distribution of Track Density Lens side

Distribution of Track Density pl08 Stage side

Distribution of Track Density Pattern 1 : random Pattern2 : line pl08

Distribution of Track Density pl08 Pattern 1

Distribution of Track Density 185 / = 0.1% pl08 Pattern 1 confirmed scratch pattern by eye check

Other sample pl23 Stage side

The Ratio of the Failure of scanning < 1 %

Distribution of Track Density pl08 Pattern 2

Distribution of Track Density pl08 Pattern 2 Plot of Raw Micro Tracks average of gaps ~ 70 micron mechanical trouble caused these gaps / prediction → Dead Space is about 5 % / surface → Now this trouble is corrected ( after plate No 45 ) 10 line / prediction unit

After correction of mechanical trouble pl45 Lens side

After correction of mechanical trouble pl45 stage side

After correction of mechanical trouble pl45 Lens side 4 prediction No dead space of line structure

The Ratio of Dead Space originDead Space Pattern 1Scratch<< 1% Pattern 2 mechanical trouble ( ~ pl44) 5 % Dead Space is about 3 % of all scanned area before pl 44. But, after pl45, less than 1 %

conclusion ・ data taking speed is 10 days / both surface / 25 cm 2 / brick with 1 shift / 18h / 33 cm 2 /h -> 40 days / both surface / 100 cm 2 / brick ・ dead space of scanning data is less than 1% depends on emulsion itself