OPERA bricks LNGS G.Rosa, C.Sirignano Emulsion Workshop, 7-9 December 2006.

Slides:



Advertisements
Similar presentations
1 STILL open points: lead, ECC Packaging, CS laminated film, skates Construction Strategy Working groups BAM design and construction BAM LNGS site preparation.
Advertisements

December 8 th, 2006Detector Construction status report Yves Déclais 1 OPERA Detector Preparation 1. Electronic Detectors: status of installation 2. Brick.
Darkroom and Film Processing
Technical Artifacts and Errors
The Chemistry of Photography. Black & White Film Black and white film is composed of 4 layers. *An upper protective coat. *A layer of gelatin that contains.
Progress of TG-1 activities (refurbishment of Phase-I detectors) Stefan Schönert on behalf of TG 1 GERDA general meeting Tuebingen, Nov. 9-11, 2005.
Veterinary Radiology Safety and Procedures. What is a radiograph? When an xray beam (a form of electromagnetic radiation) penetrates tissue to form a.
Emulsion scanning: present status and plans for the coming run Giovanni De Lellis.
Performance of Compton Alignment in OPERA CS, 2008 run Seigo Miyamoto Jan., 2009, MIZUNAMI.
1 BMS activities and brick maniupulation Short summary of 2008 activities and results Extraction and filling activities foreseen in 2009 Black CS extraction.
Jan 16th 2009Spinetti1 Power plant Intervention done by Lngs All short term interventions Repair and deeper maintenance of UPS (Dec 08) Removal of diff.
A short “physical” self introduction I’m Naotaka Naganawa from Nagoya University. I’d been working for emulsion development and compatibility between it.
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.
CS LNGS Current status and perspectives.
Image Processing Developing Pictures In the Dark Room.
Status Report on OPERA Emulsion Nakamura M. Nagoya 2006,Dec.7.
November 24th, 2005OPERA General meeting1 CS facility A. Ariga, M. Kazuyama, S. Hiramatsu Nagoya University Overview Introduction of components.
Location in CSD of electronic detector reconstructed events Scanning results from LNGS scanning lab N. D’Ambrosio, N. Di Marco, L.S. Esposito, P. Monacelli.
Retaining Ring Injection Molding by Dayán Páez. Drawing.
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.
PEANUT exposure summary and brick distribution and Situation of PEANUT analysis Fermilab.
Research History of Tsutomu FUKUDA Tono-Refresh facility Facility construction Mass production shift leader Refreshing control Sensitivity.
CSd scanning report from LNGS Nagoya OPERA workshop January 22 nd, 2008.
pictures courtesy of google images
Dental X-ray Film Processing
Whole School Attendance Whole School Attendance 94.64% Overall School Absence 5.36%
1 BAM status report S.Buontempo on behalf of BAM Committee BAM Committee Firm Pre-selection Tender Documentation BAM site preparation Project strategy.
Emulsion quality WG2 report Thanks to all the OPERA colleagues who are engaged on handling and developing emulsion.
Hamburg - Opera Collaboration Meeting - June 2004 Fiducials & labels F.Laudisio,G.Romano,C.Sirignano Salerno Emulsion Group.
INTRO TO THE DARK ROOM Photography 1.
LNGS Scanning Station Nicola D’Ambrosio (LNGS group) Maiori, 4-6 June 2007.
1 RUN 2008 OPERA events: Status Report M. Ieva on behalf of Bari Emulsion Lab OPERA Collaboration Meeting, April 1st - 5th, 2009.
September 11th, 2006LNGS and the Neutrinos from CERN OPERA 1 OPERA O scillation P roject with E mulsion-t R acking A pparatus.
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.
STF EP, VT commissioning by FNAL AES001 H. Hayano, KEK
LNGS Scientific Committee Status of OPERA/CNGS1 April 8 th, 2005 Yves Déclais on behalf of the OPERA Collaboration.
Darkroom and Film Processing Rad Tech A – Week 9 Fall 2010.
PLATE CHANGER for OIL microscopes Gabriele Sirri INFN Bologna for INFN Bologna and LNGS.
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.
1 Brick Alternative Layout S.Buontempo on behalf of BAM Committee Present design (Baseline) and “minor modifications” New CS and CSS design Alternative.
Emulsion Development Activity C.Sirignano Opera CM - Mizunami - 20/01/2009.
Brick gas tightness & emulsion-lead compatibility Opera Collaboration Meeting Hamburg, June 2004 F.Laudisio, G.Romano, C.Sirignano Salerno Emulsion.
1 ARTIFACTS: AN UNWANTED DENSITY ON THE FILM
VELOPEX EXTRA - X Mk 1V Automatic dental X-ray film Processor
EUROPE Nov 27 –Dec 10 November 27 - Dec 10.
14 th ESLS RF Meeting – Trieste, September 2010 ALBA RF Status 1/28 ALBA RF Status Francis Perez.
OPERA Coll.Meet. October 2002Luca Stanco - Padova1 1.Status of Magnets and financial orders (including RPC) Mario Spinetti15’ 2.Status of RPC (including.
1 Lead/Emulsion compatibility in OPERA bricks Short description of CNGS and OPERA projects What is an OPERA “brick” Alternative packaging Technical description.
Dental radiology د. باسم الاعسم.
Processing of films Definition of processing Processing theory Diagram.
Status Report for E391a (Continuation of the previous PAC on April) G.Y.Lim IPNS, KEK Group Meeting at the JINR 26 th – 29 th July 2003 Dzhelepov Laboratory.
Xenon Detector Installation schedule Satoshi MIHARA.
1 Costs to Completion Common funds &Running Costs Support for Running OPERA Funding Issues L. Votano Resource Coordinator OPERA Funding Agencies meeting.
1 HBD Commissioning Itzhak Tserruya DC meeting, BNL December 13, 2006 Progress from October 3 to November 28, 2006.
Emulsion processing at Gran Sasso a brief update The new building Meetings between Company’s management and GS staff to fully define the project ‘Work.
Darkroom and Film Processing Rad Tech A – Week 10 Fall 2007.
NBI2006 Starting OPERA data-taking with the CNGS beam D.Autiero IN2P3/IPN Lyon 5/9/2006.
NUMI MINOS MINOS Far Detector Installation & Commissioning Jeff Nelson MNHEP DoE Visit September, 2002.
2008 European School of High-Energy Physics - Trest, Czech Republic - 19 August - 1st September Target Tracker Data Analysis In OPERA Experiment S. Dmitrievsky,
Er. Hiralal Agrawal EXECUTIVE ENGINEER.. Apparatus:  Concrete cube moulds of 15 cm size in required numbers.  Standard tamping bar (steel) of 16mm diameter.
Film, Cassettes, and Developing Processes
Darkroom Construction Since x-ray films are more sensitive to light than most photographic films, it is important to have a good darkroom.
Radiography Dentalelle Tutoring.
More results from the OPERA experiment
The SABRE Crystals Frank Calaprice.
OPERA Stato dell’esperimento Run 2007
Automatic lights.
Darkroom and Film Processing
Italian Lab Meeting-CETARA September 2010
Presentation transcript:

OPERA bricks LNGS G.Rosa, C.Sirignano Emulsion Workshop, 7-9 December 2006

Development facility commissioning Last October and November several activities took place at LNGS, every week at least 5 people (Bari, Bologna, Roma and Salerno) were on shift in order to be ready to handle real bricks. Dark room set up (safe lights) Climatization tuning Develop tanks tests and cleaning (water + chemicals) Automatic disposal of chemicals Gridding machine installation

Week 39 Sep Week 40 Oct. 2-6 Week 41 Oct Week 42 Oct Week 43 Oct Week 44 Oct Nov.5 Week 45 Nov G. Rosa L. Ioannucci V. Di Pinto C. Valieri P. Pecchi E. Buccheri E. Carrara A. Pelosi G.Capradossi G. Romano C. Sirignano M. Ieva A. Andriani M. Castagna E. Buccheri P. Sestito A. Pelosi G.Capradossi C. Sirignano D.Di Ferdinando R. Diotallevi P. Di Pinto V. Togo E. Carrara A. Schembri E. Buccheri G. Romano C. Sirignano P. Di Pinto C. Valieri P. Pecchi G. Rosa A.Pelosi G.Capradossi G. Rosa C. Sirignano D.Di Ferdinando L. Ioannucci V. Di Pinto R. Diotallevi E. Buccheri C. Sirignano A. Pastore M. Castagna C. Valieri A. Andriani P. Pecchi G. Rosa C. Sirignano G.Romano M.Ieva P. Di Pinto R. Diotallevi A.Andriani E. Buccheri G.Rosa Shifters Shifts

2 chains ready since November 3rd to be used in manual mode Chemical preparation - Manual Development - Manual Chemical disposal - Automatic First development done using the first chain (Oct 25 th) 1 chain commissioned November 2nd (10 bricks successfully developed)

Development quality 10 bricks from BAM (wrong piling or incorrect wrapping) (1 developed in CS facility as reference) OPERA like procedure (transportation, labeling) Standard develop procedure and solution refresh rate Emulsion quality monitoring (trasparency and fog count)

Film transparency is good and no degradation observed up to now (yellowing or abnormal thickness). Two more months at least are needed to be sure that films will not turn to yellow, anyway no dramatic effects detected Ref FD8.2 (0.5) 37.8 (2) 8.6 (0.4) 7.5 (0.5) 8.2 (0.2) 8.4 (0.4) 7.8 (0.3) 9.1 (0.5) 8.4 (0.5) 8.6 (0.5) Films having hole (first shipment)

Fresh water in DevStopClean Fix Wash1 Wash2 Glyc 30 l 45 l 750 l 500 l 250 l 300 l Transfer of chemicals from preparation tanks 250 l 750 l Waste 1 Waste 2 Waste 3 Wastewater Status

OPERA bricks development (Nov 2006) 14 bricks were developed using the standard procedure 9 bricks were used for cosmic test 5 bricks extracted from the detector We used for cosmic test some bricks that BAM tagged as “out of spec” because of wrong Z dimension; that means they had double lead layers or double emulsion layers. CS were developed in the underground facility and ECC films + VETO films added during the cosmic exposure were developed outside.

CS films measurements We carried on a single development for all CS films and related FD are the following: IDFD (g/(10  m) IDFD (g/(10  m) FD same as TTCS sample developed in August TTCS same sample ???

In order to study more in details fog-up problem on double refreshed films a new exposure at BTF (Frascati) is planned fro the next week and films will be developed at LNGS starting from Dec 20th.

ECC films measurements We carried on a single development for ECC and VETO films: IDFD (g/(10  m) IDFD (g/(10  m) VETO films FD is First shipment + hole

nd shipment 1 st shipment

Develop order Brick IdFD (g/(10  m) 3 Note New developer New fixer Cosmic test bricks

IDFD (g/(10  m) 3 Notes New dev & fix Extracted bricks