Bern 13 Feb 2006 G. Sirri – INFN BO1 Scan back with dry objective G. Sirri for Bologna group Dry objective with correction collar: ZEISS LD Achroplan (code.

Slides:



Advertisements
Similar presentations
We are now working with 2 microscope: 1st Microscope Official setup: MICOS stage NIkON optics and illuminator DALSA camera cad-4 Recently several hardware.
Advertisements

1 Status report of the PEANUT analysis Giovanni De Lellis Collaboration Meeting, June 5th 2007, Maiori.
Microscope Objective Parameters. What do the Numbers on the Objective Mean ?
G. Sirri – INFN BO1 Test of Lamp with centering filament and mirror  An UPGRADE for the illumination with back mirror-lens and fine centering and focusing.
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.
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.
OPERA brick (16215) scanning results Luisa Arrabito on behalf of Lyon Scanning Group Emulsion Workshop Nagoya 22th-23th January 2008.
Cristiano Bozza – European Emulsion Scanning Group – Nagoya Jan OPERA brick scanning by the European Scanning System.
Giovanni De Lellis University of Naples (Italy) An overview of the European Scanning System (ESS) Nucl.Instrum.Meth. A568 (2006) Nucl.Instrum.Meth.
CSd analysis Natalia for the European CS Scanning Team.
Reconstruction of neutrino interactions in PEANUT in general scanning (unbiased) mode Giovanni De Lellis on behalf of Andrea Russo Naples University.
Cristiano Bozza – European Emulsion Scanning Group of OPERA– Jan 2008, Nagoya 1 Status and evolution of the European Scanning System  Basic concepts 
Edge Scanning: new plate design for the European Scanning System G. Sirri for Bologna group.
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.
Summary of the event location in Europe Giovanni De Lellis.
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.
Support to the event location in CS Scanning Station Fabio Pupilli LNGS Scanning Team OPERA Collaboration Meeting 02/04/2009 ANKARA.
Wide Field Scanning K. Morishima Nagoya University.
Status of Napoli scanning laboratory OPERA Emulsion Workshop, Nagoya, 7/12/2006 F. Di Capua on behalf of Napoli group.
Umut Kose Neutrino interaction location in the OPERA Experiment New Development of Flavor Physics, , Tennomaru, Gamagori Nagoya University.
Jean Favier OPERA Meeting Ankara 3/04/09 1 Some ECC features studied with GenIma Efficiency with no fog Efficiencies with fog Micro-track number versus.
Scanning status in Europe Giovanni De Lellis University of Naples.
CS to brick and track follow-up ● Cosmic ray test ● CS scanning ● CS to brick connection ● Track following Napoli Scanning Lab.
MonteCarlo simulation of neutrino interactions in PEANUT Giovanni De Lellis on behalf of Alberto Marotta and Andrea Russo Naples University.
Reconstruction of neutrino interactions in PEANUT G.D.L., Andrea Russo, Luca Scotto Lavina Naples University.
EM shower reconstruction and located neutrino event analysis Ciro Pistillo (Bern LHEP) on behalf of the Swiss OPERA groups.
Introduction to Microscopy. Objectives Learn to use a compound microscope correctly. Diagram the path of light through a compound microscope. Name major.
BOLOGNA Scanning Lab INFN - Sezione di BOLOGNA Physics Dep. of Alma Mater Studiorum Università di Bologna M.Pozzato – Ankara – 09/04/02.
G.Sirri – INFN Bologna videconf /14 Fiducial Mark Finding with ESS  Lateral Mark Finding [FlexMapX]: Recommended release 42b ( )
European Scanning System R&D Bari, Bologna, Bern, Lyon, Napoli, Roma, Salerno Tuning of 10 cm 2 /hour on the OPERA emulsions But not refreshed and 32 micron.
1 RUN 2008 OPERA events: Status Report M. Ieva on behalf of Bari Emulsion Lab OPERA Collaboration Meeting, April 1st - 5th, 2009.
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.
LNGS 4 Jul 2006 INFN BO1 Grain analysis with High-Resolution microscope  An High Resolution microscope was developed in parallel with the ESS and is working.
DB-based DAQ monitoring and Physics analysis tools Emiliano Barbuto European Emulsion Group (LNGS May 2003)
Jean Favier LAPP OPERA meeting Hamburg 5/06/04 GenIma: program to simulate emulsions.
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.
Bologna Report M. Pozzato on behalf of Bologna Group Cetara Meeting – 13/09/2010.
PLATE CHANGER for OIL microscopes Gabriele Sirri INFN Bologna for INFN Bologna and LNGS.
Status of European Scanning System (Bari, Bern, Bologna, Lyon, Napoli, Neuchatel, Roma, Salerno) The final fast version is ready and working up to 20 cm.
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.
OPERA scanning session, CERN 03/05/06 DB-driven Scan-back with collar Nikon dry obj.
RICH upgrade simulation: updates RICH upgrade-software meeting 1 S.Easo.
RICH upgrade simulation: updates S.Easo RICH upgrade-mechanics meeting 1.
Gluing machine (scanning at the edge…) G. Sirri for Bologna Group.
TecnoCut PlateChanger Set Up / videoconferenceG.Sirri - INFN Bologna1 HARDWARE (complete):  both glued / not glued emulsion setup  cabling.
Event location and decay search in Switzerland Swiss group.
I.Kreslo / LHEP BERN1 Status of scanning in Bern HW status SW status pi/mu separation ( PSI 2004 ) vertex search (CERN 2004)
Emulsion Simulation Y. Caffari (IPN Lyon) F. Juget (IPH Neuchatel) A. Marotta (CNRS-IN2P3 Lyon) CERN 3-5/05/2006.
OPERA Physics Coordination, CERN, 03/05/2006 Effect of  and  radiation on the on-line emulsion scanning M. Cozzi for the Bologna group.
I.Kreslo / LHEP BERN1 Status of scanning lab in Bern 2 Microscopes are operating Data acquisition/sharing setup Scanning performance: 2x2cm 2.
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,
Electron Reconstruction through OpEmuRec Collaboration meeting 22/09/10 Florian Brunet.
Nuclear Emulsion Readout Techniques Developed for the CHORUS Experiment or “...how we managed in CHORUS to convert nuclear emulsion into an electronic.
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.
IMEKO TC 16 (Pressure) International Conference Cultivating metrological knowledge November, 27 – 30, 2007, Merida, Mexico A 36 MPa PRESSURE BALANCE IN.
Wide Field Scanning K. Morishima Nagoya University.
“MIXED” test Cosmics Tono LNGS I.Kreslo LHEP BERN.
Edge Scanning: new plate design for the European Scanning System
Results from OPERA Pablo del Amo Sánchez for the OPERA collaboration
HPS Collaboration meeting, JLAB, Nov 16, 2016
Compensation of Detector Solenoid with Large Crossing Angle
Bari emulsion lab: status report
Presentation transcript:

Bern 13 Feb 2006 G. Sirri – INFN BO1 Scan back with dry objective G. Sirri for Bologna group Dry objective with correction collar: ZEISS LD Achroplan (code ) magnification: 40x (nominal) numerical aperture: 0.60 working distance: 1.8 mm correction range: 0-2 mm The collar has been motorized with a DC motor and a drive belt. The motor controller are connected through a serial line. Efficiency, angular residuals, position residuals, base-track density on the non-exposed plate were already shown (behavior similar to the oil). Working conditions: two collar position c.c. 0 for the TOP scanning c.c. 0.3 for the BOTTOM scanning Analysis of the reference brick: efficiency : >90% angular residuals: 1.0 mrad [at 0 mrad], 4.5 mrad [at 400 mrad] position residuals: 1 µm [at 0 mrad], 3 µm [at 400 mrad] base-track density on the non-exposed plate = 4.0 tr/mm2/||<0.4 rad

Bern 13 Feb 2006 G. Sirri – INFN BO2 Software implementation  The acq. software has been modified in order to move the collar during the ACQ and to minimize the time to switch from Top to Bottom positions. Main points:  Interface to the controller implemented inside VertigoScan.  Switch the collar position during focusing, scan and “single view” scan  Fiducial marks finding with an intermediate correction (c.c. 0.15)  different magnification Top/Bottom µm/pixel (c.c. 0, top) µm/pixel (c.c. 0.3, bottom)  Focal plane shifts due to the correction (~ 10 µm)

Bern 13 Feb 2006 G. Sirri – INFN BO3 DB scan back setup  Same brick and predictions of the oil scan back in order to compare the results. 325 predictions (coming from a general scan of the first 10 plates up to 0.4 rad,  see Michela talk) same DB intercalibration performed with oil  Minor changes in the acquisition parameters: cluster size >= 3 n° of grains per microtrack >= 6 CIMG2063.AVI

Bern 13 Feb 2006 G. Sirri – INFN BO4 Angular residuals (pred – found) Black = dry Red = oil

Bern 13 Feb 2006 G. Sirri – INFN BO5 Position residuals (pred – found) Black = dry Red = oil

Bern 13 Feb 2006 G. Sirri – INFN BO6 Out of 325 predictions: 248 passing through (last found plate >53) 77 stopping points entries Scanning efficiency (on passing tracks) Stop plate

Bern 13 Feb 2006 G. Sirri – INFN BO7 Comparison with two oil scan backs  Scan back preformed on 2 oil microscopes (MIC2, MIC3) and on the dry microscope (MIC1)  Out of 325 predictions … (P = passing through, X = stopping) MIC1 (dry)MIC2MIC3 PPP223 PPX11 PXP12 XPP14 PXX2 XPX6 XXP2 XXX55 35 identified by all microscopes

Bern 13 Feb 2006 G. Sirri – INFN BO8 Efficiency (passing tracks) Green = DRY Blue = OIL (mic3)

Bern 13 Feb 2006 G. Sirri – INFN BO9 Segments of stopping tracks Green

Bern 13 Feb 2006 G. Sirri – INFN BO10 Conclusions  Also in the scan back procedure, the dry objective with correction collar results are very similar to the oil case.  The total scan (with this objective) and the vertex confirmation are in progress.  A Nikon dry objective with correction collar is under test and will be motorized soon.