NVT capillary collimator NORTH NIGHT VISION TECHNOLOGY CO., LTD

Slides:



Advertisements
Similar presentations
SWD 2005, Taormina, Jun,19-26 An EUV Imaging Detector of Space Solar Telescope Qian Song, Binxun Ye, Zhaowang Zhao National Astronomical Observatories,
Advertisements

Telescope Tear-Down Anatomy of a 114mm f/8 Newtonian Reflector.
Telescopes and Spacecraft Astronomy 311 Professor Lee Carkner Lecture 7.
Telescope Design The W.M. Keck (I & II) Telescopes Jana Hunt & Kent Van ME250 Precision Machine Design April 8, 2003.
Use of a commercial laser tracker for optical alignment James H. Burge, Peng Su, Chunyu Zhao, Tom Zobrist College of Optical Sciences Steward Observatory.
Characterization of Detectors NEP= noise equivalent power = noise current (A/  Hz)/Radiant sensitivity (A/W) D = detectivity =  area/NEP IR cut-off maximum.
IMEC - INTEC Department of Information Technology WAVEGUIDES IN BOARDS BASED ON ORMOCER  s
Fiber optic Take a walk to the. Fiber optics Basics for fiber optics.
Lecture 2-Building a Detector George K. Parks Space Sciences Laboratory UC Berkeley, Berkeley, CA.
Introduction to Precision Metrology
1 Fluorescence Cameras -Dr James Milnes -Live Cell Imaging – Stem Cell Research -Portland Place, London, 24 June 2009 Live Cell Imaging.
D EDICATED S PECTROPHOTOMETER F OR L OCALIZED T RANSMITTANCE A ND R EFLECTANCE M EASUREMENTS Laetitia ABEL-TIBERINI, Frédéric LEMARQUIS, Michel LEQUIME.
Department of Metallurgy and Materials Engineering Materials Performance and Non-Destructive Testing Optimization and validation of micro-CT for the characterization.
Dyadenko M.V. scientific researcher, candidate of technical sciences (department of glass and ceramic technology) New Delhi 2013 Glass for an optical fiber.
The Hard X-ray Modulation Telescope Mission
Secondary Emission Ionization Calorimetry Detectors
PACS IIDR 01/02 Mar 2001 FPFPU Alignment1 D. Kampf KAYSER-THREDE.
Chang,Liang YNAO,CAS July 09-10,2011 Fore Parts of Optical Design Scheme of FASOT (from telescope to spectrograph)
Scale-Up Activities in Atomic Layer Deposition at Argonne Jeffrey Elam, Anil Mane, Joe Libera December 9, 2011 Large Area Picosecond Photodetector Collaboration.
MARS Design Review PP-1 Requirements Definition Performance: –Tip/Tilt error < 0.06″ rms mirror coordinates 0.12″ rms image coodinates 0.28″ fwhm image.
WSO/UV-LSS Detector with large dimension MCP Baosheng Zhao* National Astronomical Observatories of CAS *
Specification of niobium sheets 031/05/2010 O. Capatina G. Arnau Izquierdo W. Weingarten S. Atieh.
K-D-PR Fabrication and testing of KGMT FSM prototype Oct Ho-Soon Yang, Hak-Yong Kihm, Il-Kwon Moon, Jae-Bong Song, Yun-Woo Lee Korea.
Detectors and Cross Talk Presented below are cross talk measurements carried out on 2 Burle and 1 Hamamatsu MCP PMTs and 1 Hamamatsu MultiAnode PMT (MAPMT).
WFIRST IFU -- Preliminary “existence proof” Qian Gong & Dave Content GSFC optics branch, Code 551.
イメージスライサー型可視光 面分光ユニットの開発 Development of an integral field unit (IFU) with an image slicer Shinobu Ozaki, Satoshi Miyazaki, Takuya Yamashita, Takashi Hattori,
MAXIM Periscope ISAL Study Highlights ISAL Study beginning 14 April 2003.
Improvement of Infrared Lights Sensitivity on PZT EMITER Daisuke Takamuro, Hidekuni Takao, Kazuaki Sawada and Makoto Ishida.
MCP MicroPitting and Performance Issues Latest 40µm pore 8” MCPs had some patchy discoloration Cleaning using standard techniques at SSL made no difference.
THE CRAO'S CONTRIBUTION FOR THE WSO / UV PROJECT N.V.STESHENKO.
© Synkera Technologies, Inc.
Optical Sciences Center and Steward Observatory University of Arizona
THE GAMMA-400 PROJECT Direct measurements of the primary gamma- radiation in the energy range 30 GeV – 1 TeV GAMMA-400 COLLABORATION: Lebedev Physical.
Grid Fabrication and Characterization Brian Dennis, GSFC Gordon Hurford, UCB.
Atomic Layer Deposition for Microchannel Plates Jeffrey Elam Argonne National Laboratory September 24, 2009.
ZTF Optics Design ZTF Technical Meeting 1.
33mm MCP Testing at UC Berkeley
14FEB2005/KWCAE2-UsersGroup Astro-E2 X-Ray Telescopes XRT Setup & Structure Performance Characteristics –Effective Area –Angular Resolution –Optical Axes.
El-Mul Technologies Ltd – Confidential & Proprietary El-Mul Technologies El-Mul Technologies Ltd – Confidential & Proprietary Prof. Eli Cheifetz, Chairman.
The High Altitude Observatory (HAO) at the National Center for Atmospheric Research (NCAR) The National Center for Atmospheric Research is sponsored by.
Polypterus senegalus SEM Imaging Sample Preparation Protocol Sample Imaging Parameters -Scales were embedded in resin and cured at 60˚ C for 16 hours -Embedded.
Chamber mechanics Chamber mechanics Production in China Peking University Group – 20 Aug
 A PCB is printed circuit board, also known as a printed wiring board. It is used in electronics to build electronic devices. A PCB serves 2 purposes.
Lingling Ma IHEP China Measurement of Cosmic rays with LHAASO at 10PeV~100PeV 4th Workshop on Air Shower Detection at High Altitude Institute of High Energy.
Simulation geometry 2000 V terminal Vacuum Glass substrate, ε = 5.8 Resistive coating, ε = 6.8 and σ = 1e-8 S/m The pore has a 40μ diameter and 40:1 aspect.
Development of Micro-Pore Optics at NAOC MPO research group X-ray Imaging Laboratory, NAOC Presented by Chen Zhang.
3D SCANNING TECHNOLOGIES IN MECHANICAL ENGINEERING AND MANUFACTURE Gábor Kimmel Computer engineering 3D Graphics Professional Days.
SPS High Energy LSS5 Thermal contact & cooling aspects
BWS Design meeting Jose Luis Sirvent PhD. Student XX/03/2014
Introduction to Precision Metrology
Chandrayaan-2 Large Area Soft X-ray Spectrometer (CLASS)
Presentation on SEM (Scanning of Electron Microscope) Represented by:-Ravi Kumar Roll:- (BT/ME/1601/006)
Detector development for
Night vision goggles [1] Front Lens [2] Photocathode
2013 KAPRA & KPS/DPP Conference
Development of Large-Area Photo-detectors:
Simulations for WXT aboard Einstein Probe mission with Geant4
Introduction to Scanning Electron Microscope by Sameer S
METALLURGICAL MICROSCOPE
NANO 230 Micro/NanoFabrication
Sezgin Cengiz1, Mehmet Yazici1,2, Y. Gencer1,*, M. Tarakci1,
Detectors of the New Projects at NAOC
Detector development for
Heritage from the LOFT-M3 study: Collimator Assembly
ENGINEERING PHYSICS B.TECH :I YEAR SEM-I MECHANICAL & CIVIL
ME instrument and in-orbit performance
Scanning Electron Microscopy (SEM)
Optics Alan Title, HMI-LMSAL Lead,
Status of ALD 33 mm MCP Development at Argonne
Progress of DLC Resistive Electrode
Presentation transcript:

NVT capillary collimator NORTH NIGHT VISION TECHNOLOGY CO., LTD Xu Zhao NORTH NIGHT VISION TECHNOLOGY CO., LTD Mar. 21, 2017

Contents 1 2 3 4 Introduction of NVT Engineering Capacity Technical Progress of Collimator 4 Development Plan

1. Introduction of NVT Introduction Core business: low-light-level night vision vacuum devices The only image intensifier manufacturer in China One of five major suppliers of image intensifier in the world Kunming Nanjing branch

1. Introduction of NVT Core business Vacuum image intensifier, large photomultiplier tube, special high voltage power supply, micro channel plate(MCP), fiber optic device.

Micro channel plate(MCP) & Fiber optic device 1. Introduction of NVT Micro channel plate(MCP) & Fiber optic device

Hard X-ray modulation telescope (HXMT) Pore surface roughness 2. Engineering Capacity Hard X-ray modulation telescope (HXMT) China Aerospace Science &Technology Corporation(CASC) Detector: 1 pieces of collimator , 2 pieces of MCPs 8 NVT detectors Parameters Nominal value Pore size 40μm Plate size 100mm×50mm Thickness 1.2mm Open area ratio >60% Pore surface roughness Not required

Einstein probe satellite (EP) Pore surface roughness 2. Engineering Capacity Einstein probe satellite (EP) National Astronomical Observatories of China (NAOC) Micro pore optic (MPO) Engineering samples Parameters Nominal value Pore size 20μm×20μm Plate size 40mm×40mm Thickness 1.25mm Open area ratio >60% Pore surface roughness <1nm Technical progress 2014.6 2015.10 2016.3 2016.8

Production capacity of collimator 2. Engineering Capacity Production capacity of collimator Stages Pieces each year Development stage 300 Engineering stage 500-800

3. Technical Progress Technical specification of collimator Parameters Requirements Measured value Lead-oxide equivalent content ≥37% 39% Pore size 83μm 83.2μm Open area ratio ≥70% 71.1% Plate size 111mm×72.5mm 100mm×50mm Thickness 5mm Pore surface roughness >13nm 5nm Pore to pore alignment ≤1 arc minute 3.4 arc minute Pore to surface alignment 6 arc minute Plate flatness 0.68 arc minute

Production process of collimator 3. Technical Progress Production process of collimator Core fitted to cladding Primary draw Multifiber stack Secondary draw Etch Slice and Polish Stack & Fuse

3. Technical Progress Glass composition XRF results Core and cladding K K Core and cladding XRF K2O PbO Sample 2016 3.2% 39%+50% Sample 2017 0.03% 39% 3.3keV Sample in 2016 Sample in 2017

3. Technical Progress Microstructure Parameters Measured value Multifiber error ±0.005mm Pore size 83μm Open area ratio 71% Multifibers Sample in 2016 Sample in 2017

Pore surface roughness Pore surface roughness 3. Technical Progress Pore surface roughness Sample in 2016 Sample in 2017 Pore surface roughness Measured value Sample 2016 1nm Sample 2017 5nm Large collimator sample

4. Development Plan Future improvements Time Problems to be solved Specifications Related processes 2017 Pore surface roughness ≥13nm Etch & Draw Pore to pore alignment ≤1 arc minute Draw 2018 Pore to surface alignment Fuse & Slice Build a testing system for micro pore structure

Thank you!