Eusoballoon optics characterisation Camille Catalano and the Toulouse team Test configuration Calibration of the beam Exploration of the focal plan.

Slides:



Advertisements
Similar presentations
Optics and magnetic field calculation for the Hall D Tagger Guangliang Yang Glasgow University.
Advertisements

Copyright © 2009 Pearson Education, Inc. Chapter 35 Diffraction and Polarization.
Phys 102 – Lecture 23 Diffraction.
Topic 11.3 Diffraction.
Foundations of Physics
Optics 1. 2 The electromagnetic spectrum Visible light make up only a small part of the entire spectrum of electromagnetic waves. Unlike sound waves and.
Review from last class – Complete in your notes. 1.A pinhole camera creates an image of a 37- meter-tall tree. If the image is 2.4 cm tall and inverted,
Chapter 16.3 – Reflection and Color
Lecture 33 Review for Exam 4 Interference, Diffraction Reflection, Refraction.
IVA. Electromagnetic Waves and Optics
IPCMS-GEMME, BP 43, 23 rue du Loess, Strasbourg Cedex 2
The Hong Kong Polytechnic University Optics II----by Dr.H.Huang, Department of Applied Physics1 Interference Conditions for Interference: (i) (  2 
Could CKOV1 become RICH? 1. Characteristics of Cherenkov light at low momenta (180 < p < 280 MeV/c) 2. Layout and characterization of the neutron beam.
Interference & Diffraction
Spectrophotometer Jan 28, 2002 Deryck Hong Suryadi Gunawan.
Wide-field, triple spectrograph with R=5000 for a fast 22 m telescope Roger Angel, Steward Observatory 1 st draft, December 4, 2002 Summary This wide-field,
Fiber Optics Defining Characteristics: Numerical Aperture Spectral Transmission Diameter.
GEANT4 simulations for the Lund R 3 B prototype Douglas Di Julio Lund University, Lund, Sweden.
Chapter 25: Interference and Diffraction
R. M. Bionta SLAC November 14, 2005 UCRL-PRES-XXXXXX LCLS Beam-Based Undulator K Measurements Workshop Use of FEL Off-Axis Zone Plate.
1 Aurélien Barrau LPSC-Grenoble (CNRS / UJF) A few words on the LPSC The LPSC in few words: The scientific environment : Grenoble 4 Universities.
Astronomical Spectroscopy
Example: What is the ratio of the irradiances at the central peak maximum to the first of the secondary maxima?
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
Chapter 17 Optics 17.1 Reflection and Refraction
Convex Lens A convex lens curves outward; it has a thick center and thinner edges.
Measurement of the absolute efficiency,
An unpolarized beam of light is incident on a pane of glass (n = 1
Diffraction: single slit How can we explain the pattern from light going through a single slit? w screen L x.
Ray Model A useful model under certain circumstances to explain image formation. Ray Model: Light travels in straight-line paths, called rays, in ALL.
Light, Mirrors, and Lenses O 4.2 Reflection and Mirrors.
LIGHT CH. 18. What is Light? Light is an electromagnetic wave that travels through space requiring no medium.
Diffraction and Limits of Resolution. Diffraction through a circular aperture of diameter D Intensity Diameter D Image on Screen θ = 1.22 λ /D Because.
Optics 2: REFRACTION & LENSES. REFRACTION Refraction: is the bending of waves because of the change of speed of a wave when it passes from one medium.
Reflection Regular reflection occurs when parallel light rays strike a smooth surface and reflect in the same direction. Diffuse reflection occurs when.
High Resolution Echelle Spectrograph for Chinese Weihai 1m Telescope. Leiwang, Yongtian Zhu, Zhongwen Hu Nanjing institute of Astronomical Optics Technology.
The whole instrument Tests performed Conclusions EUSO-BALLOON, EUSO-BALLOON flight review 04/06/2014 P. Barrillon on behalf of the many hard workers involved.
S Optical CT scanning of PRESAGE TM polyurethane samples with a CCD-based readout system S J Doran 1*, N Krstajic 1, J Adamovics 2 and P M Jenneson 1 1.
Jean Favier LAPP OPERA meeting Hamburg 5/06/04 GenIma: program to simulate emulsions.
Eusoballoon optics test Baptiste Mot, Gilles Roudil, Camille Catalano, Peter von Ballmoos Test configuration Calibration of the light beam Exploration.
September 16, 2008LSST Camera F2F1 Camera Calibration Optical Configurations and Calculations Keith Bechtol Andy Scacco Allesandro Sonnenfeld.
The Hong Kong Polytechnic University Optics 2----by Dr.H.Huang, Department of Applied Physics1 Diffraction Introduction: Diffraction is often distinguished.
Chapter 38: Diffraction and Polarization  For a single opening in a barrier, we might expect that a plane wave (light beam) would produce a bright spot.
Calibration of the LSST Camera Andy Scacco. LSST Basics Ground based 8.4m triple mirror design Mountaintop in N. Chile Wide 3.5 degree field survey telescope.
Laser-Based Finger Tracking System Suitable for MOEMS Integration Stéphane Perrin, Alvaro Cassinelli and Masatoshi Ishikawa Ishikawa Hashimoto Laboratory.
Development of a Gamma-Ray Beam Profile Monitor for the High-Intensity Gamma-Ray Source Thomas Regier, Department of Physics and Engineering Physics University.
 Myth: 3 sec memory  Reality: 3 years are passed  I’m not a goldfish, but…
DIFFRACTION AND INTERFERENCE. Specification Topics Interference The concept of path difference and coherence The laser as a source of coherent monochromatic.
Lab 10: Wave optics Only 2 more labs to go!! Light is an electromagnetic wave. Because of the wave nature of light it interacts differently than you might.
The law of reflection: The law of refraction: Image formation
N A S A G O D D A R D S P A C E F L I G H T C E N T E R I n s t r u m e n t S y n t h e s i s a n d A n a l y s i s L a b o r a t o r y APS Formation Sensor.
1 Electromagnetic waves: Multiple beam Interference Wed. Nov. 13, 2002.
Reflection Regular reflection occurs when parallel light rays strike a smooth surface and reflect in the same direction. Diffuse reflection occurs when.
CS-498 Computer Vision Week 7, Day 2 Camera Parameters Intrinsic Calibration  Linear  Forward and backward projection 1.
Aerogel detector revisited Sokolov Oleksiy, UNAM, progress report, 20 Sept 2006 E int = M – wall reflectivity є – PMT relative area Belle geometry (traditional):
Date of download: 6/23/2016 Copyright © 2016 SPIE. All rights reserved. (a) Schematic diagram of computer-aided Mach–Zehnder interferometer; laser beam.
Astronomical Spectroscopic Techniques
Notes 23.1: Optics and Reflection
l 66TH MEETING OF THE ESRF l May 2014 l Author
Physics Case of the Day - Sunday
Light, Mirrors, and Lenses
Interference Requirements
From: A Novel, Real-Time, In Vivo Mouse Retinal Imaging System
Notes 23.3: Lenses and Images
Waves may reflect diffusely based on…
Fraunhofer Diffraction
Mirrors and Lenses.
Chapter 10 Diffraction February 25 Fraunhofer diffraction: the single slit 10.1 Preliminary considerations Diffraction: The deviation of light from propagation.
Volume 109, Issue 12, Pages (December 2015)
DIFFRACTION AND INTERFERENCE
Presentation transcript:

eusoballoon optics characterisation Camille Catalano and the Toulouse team Test configuration Calibration of the beam Exploration of the focal plan

1 - Configuration of the optics tests Typical light source : 390nm LED 1m collimator to create a parallel light beam Typical Incident angle of 3.5° CCD camera + NIST calibrated photodiode used at the focal plan The optics system is composed from only two fresnel lenses

2 - Calibration of the collimated beam Scan of the entire beam, calibrated in light power -> 80494±4370 nW (~5% error) Calibration of the beam : Grid pattern placed on the aperture of the instrument ~160 measurements with the NIST

Visualisation of the beam with azurins in white paper on the aperture of the instrument -> the photo of the white screen is comparable with the NIST measurements from the NIST mapping of the beam from the photo of the white paper on the aperture 2 - Calibration of the collimated beam

3 - Exploration of the focal plan Method : Measurement of the light flux with the NIST along an axis perpendicular with the optical axis Approximation of the encircle energy with the calculation at each position of the integrated flux on a ring of 1cm of thickness (size of the nist = 1cm^2). The integrated flux is then summed with those from the inner rings. Method to approximate the encircle energy collimatorCollimated light beam Optical system NIST measurements along perpendicular axis

3 – Exploration of the focal plan Encircle energy with the NIST : e opt = 30.5±3 % Efficiency : (defined as the fraction of the flux collected in the cm 2 centered on the focal spot) Full Width at Half Maximum = ~8mm Scan of the focal plan with the NIST. Blue = direct measurement of the NIST Red = encircle flux λ=391nm θ=3.5° off axis

Encircled energy In the central cm2 : e opt = 30.5 % In ~3x3 PDM pixels : e opt = 24 %

eusoballoon optics simulation for data analysis Camille Catalano

Simulation for data analysis Modeled real object (forest, flasher,…) Simulated data Real data Simulation of the whole instrument

Simulation for data analysis Problem : simulation programs didn’t simulate all the diffuse light measured during the optics characterisation Simulation made with ZEMAX

Simulation for data analysis A solution : Add artificial scattering on optical surfaces in order to truly reproduce the experimental data Then introduce those changes in the whole instrument simulation My ZEMAX study of artificial scattering in progress…