19/12/06SAM_LGS_1, CTIO, Optics1 SOAR at Horizon Telescope Ring Section= 1272.4x336mm Laser Box Width=300-400mm.

Slides:



Advertisements
Similar presentations
OFD 1 Oli Durney LBTI Optical Engineer Steward Observatory University of Arizona NIC Aperture, Pupil, and Filter Wheel Positions Rev. 3.3 November 3, 2011.
Advertisements

OFD 1 Oli Durney LBTI Optical Engineer Steward Observatory University of Arizona NIC Aperture, Pupil, and Filter Wheel Positions Rev. 2.3 September 19,
Determination of heights – essential terms 1. Equipotential surface = a surface with the invariable gravity potential (perpendicular to the force of gravity.
SPL Intercavity support Conceptual design review 04/11/ A. Vande Craen TE/MSC-CMI.
TPC meeting, NBI, 2-3 September 2002Børge Svane Nielsen, NBI1 Status of laser system TPC meeting, Copenhagen, 2-3 September 2002 Børge Svane Nielsen, Jørn.
TPC meeting, CERN, 7-8 October 2003Børge Svane Nielsen, NBI1 Status of laser system TPC meeting, CERN, 7-8 October 2003 Børge Svane Nielsen, Niels Lindegaard,
Notes on building a Newtonian
SAM LGS-v1, Optics, The Laser Box position on SOAR IR Nasmyth Optical Nasmyth At 67.5Deg from IR Nasmyth Note: Laser umbilical cord of 7m has been.
Surveying I. Lecture 2..
Sz. Rózsa: Surveying I. – Lecture 2
Laser Launch System for the LBT Richard Davies Sebastian Rabien Max Planck Institute for Extraterrestrial Physics  Approaches of other observatories 
MICE Hall – South Mezzanine Jason Tarrant - STFC l Contents »Device checks with current South Mezzanine »South Mezzanine change summary »Conclusion.
S.H.H.S Building Construction
CKOV1 folded geometry 1. Optimization 2. Pion-muon separation 3. Instrumented area 4. Possible developments November 16, 2005 Gh. Grégoire Contents.
MONALISA installation at the ATF2 ATF2 weekly meeting.
AMS-02 tracker mechanics status of assembly and integration Inner tracker integration completion: - Assembly and cabling - Temperature and magnetic field.
NGAO Alignment Plan See KAON 719 P. Wizinowich. 2 Introduction KAON 719 is intended to define & describe the alignments that will need to be performed.
Setup of laser tracker on DX side NOTE: X axis along M1s centers, towards SX Z axis along M1-M2 centers, towards M2.
1 Detector position August 2005, supplement May’06 sub- detectormean Zdelta ZZ_startZ_end TT First pillar =1 st shelf at sides
Preliminary studies for Muon shield modification to accommodate LCLS II Alev Ibrahimov December, 2010 BSY.
Sz. Rózsa: Surveying I. – Lecture 1
Oct 17, 2001SALT PFIS PDR - Structure1 Structure Interface/ constraints Loads Structure design rationale Truss Weight and CG Finite Element Analysis/ Image.
September 28, 2007LGS for SAM – PDR – Optics1 LGS for SAM Optical Alignment R.Tighe, A.Tokovinin. LGS for SAM Design Review September 2007, La Serena.
SAM PDR1 SAM LGS Mechanical Design A. Montane, A. Tokovinin, H. Ochoa SAM LGS Preliminary Design Review September 2007, La Serena.
Proposed injection of polarized He3+ ions into EBIS trap with slanted electrostatic mirror* A.Pikin, A. Zelenski, A. Kponou, J. Alessi, E. Beebe, K. Prelec,
MICE RFCC Module Update Allan DeMello Lawrence Berkeley National Laboratory MAP Winter Collaboration Meeting at JLab, Virginia February 28, 2011.
September 28, 2007LGS for SAM – PDR – Optics1 LGS for SAM Optical Design R.Tighe, A.Tokovinin. LGS for SAM Design Review September 2007, La Serena.
The Mechanical Design of the Second and third Antarctic Survey Telescope Wen Haikun.
Chapter (5) Leveling Introduction:
OFD 1 Oli Durney LBTI Optical Engineer Steward Observatory University of Arizona NIC Aperture, Pupil, and Filter Wheel Positions Rev. 2.1 April 29, 2011.
SAM PDR1 S OAR Adaptive Module LGS LGSsystem Andrei Tokovinin SAM LGS Preliminary Design Review September 2007, La Serena.
Introduction of SONG telescope design Guomin Wang, Bozhong Gu, Xiangyan Yuan Zhiyong Zhang, Xiang Jiang, Shihai Yang The Third Workshop of SONG Beijing.
The FMOS Facility for the SUBARU telescope Gavin Dalton Oxford/RAL.
Status of RICH mechanical design at PNPI E.Vznuzdaev for PNPI group: V.Dobyrn, A.Khanzadeev, E.Kormin, V.Lebedev, N.Miftakhov, V.Polyakov, V.Samsonov,
Considerations on laser-p+ beam merging for CB, BG, PM.
Designing an Intensified Photodiode Mount
MICE RFCC Module Update Allan DeMello Lawrence Berkeley National Laboratory MICE CM29 at RAL, UK February 17, 2011.
C2PU TELESCOPES © C2PU, Observatoire de la Cote d’Azur, Université de Nice Sophia-Antipolis Jean-Pierre Rivet CNRS, OCA, Dept. Lagrange
E.Guschin (INR) 21 November 2003Integration EDR PRS/SPD static envelop, assembly and installation Detector layout Static envelop along the beam Detector.
Survey, Alignment and Metrology Fiducials Requirements Fabien Rey ESS Survey, Alignment and Metrology Group ACCELERATOR TECHNICAL BOARD 23/09/2015.
Survey, Alignment and Metrology Fabien Rey Pawel Garsztka ESS Survey, Alignment and Metrology Group Interface Workshops for ESS Warm-Linac: ISrc - LEBT.
Intelligent Random Box Sizer Animated Flow. Intelligent Random Box Sizer Animated Flow Boxes placed onto Infeed Conveyor.
A2-A5: The drawing has been revised (minor changes), the bid has been approved by INFN management and the invitation letter to the companies will be sent.
SL/BI 16/05/1999DIPAC’99 -- JJ Gras -- CERN SL/BI -- Adaptive Optics for the LEP 2 SR Monitors G. Burtin, R.J. Colchester, G. Ferioli, J.J. Gras, R. Jung,
Redesign of LumiCal mechanical structure W.Daniluk, E.Kielar, J.Kotula, K.Oliwa, Wojciech Wierba, L.Zawiejski Institute of Nuclear Physics PAN Cracow,
Compensation of Detector Solenoid G.H. Wei, V.S. Morozov, Fanglei Lin JLEIC Collaboration Meeting Spring, 2016.
Hcal Geometry and Assembly Videoconference January 2008, 24th.
AirSpeed Calibration Facility by using LDV and A Wind Tunnel at CMS
1 ILD inner region integration meeting M. Joré – Introduction ILD inner region integration meeting Welcome words Charge of the meeting The current concept.
CERN –GSI/CEA MM preparation meeting, Magnetic Measurements WP.
Baby MIND Scintillator modules 11 November 2015 Revision E. Noah.
The Super-FRS Multiplet, Magnetic and Cryogenic requirements
Mars Sextant PDR Opti 523 Paul Ward-Dolkas.
Planning for Proto-DUNE PD Installation and Cabling at CERN
Section 3.5 – Transformation of Functions
Ferrara MECHANICAL SUPPORT for forward tracking detectors Federico Evangelisti INFN - Ferrara GSI – 2-6 march 2009.
Mechanical Design Review February 25, 2008 Université de Montréal
McEvoy and Langston inc
Mechanical Design Review February 25, 2008 Université de Montréal
Chapter (5) Leveling Introduction:
Visit for more Learning Resources
Barrel EMC assembling (EDMS DOCUMENT NUMBER /1)
Cooling pipes and Space for Services
Additional muon stations for the Upgrade of the Elevator Regions in the ATLAS Muon Spectrometer. Integration issues Denis Diyakov, Alexander Seletskiy,
LumiCal mechanical design, integration with LDC and laser alignment
iSHELL Design Review Cryostat & Optics Bench
Progress on 1.8m Telescope with 127-element Adaptive Optics at IOE
Finding Lengths of Horizontal Lines on a Coordinate Plane
Leveling By : Parveen Kumar.
Presentation transcript:

19/12/06SAM_LGS_1, CTIO, Optics1 SOAR at Horizon Telescope Ring Section= x336mm Laser Box Width= mm

19/12/06SAM_LGS_1, CTIO, Optics2 Yoke-Ring Space near Elevation Axis First conclusion: Laser Box cant go on the low side of the ring neither above the Elevation axis.

19/12/06SAM_LGS_1, CTIO, Optics3 Laser Box Size Laser Head(+Connectors):~900x140x90mm Space (Align/Dump Mirror):~150mm Beam Expander: 141x  31.75mm (could be up to 200x  50mm) Compensator: 110x230x166mm (because of rotator and vernier) Steering Mirror stand:~50x50mm Extra Width (Align.Laser/mirror):~100mm Extra Length (Beam/Align Camera):~100mm Base Plate/Table: 25.4 to 60mm Laser Box Estimate: 1510x330x226mm Laser Box Mock : 1600x400x250mm

19/12/06SAM_LGS_1, CTIO, Optics4 Soleil-Babinet Compensator UV-25 from Special Optics CA=25mm, Max. Retardation=400nm, Resolution=0.5nm and Price= $4.150 Space needed (l x w x h)=110x229.4x165.4mm

19/12/06SAM_LGS_1, CTIO, Optics5 Laser Control and Cooler

19/12/06SAM_LGS_1, CTIO, Optics6 Laser Box on Truss Pros: one mirror less, follows serrurier flexure Cons: mechanical support?, adjustable M3 on LLT, ~70Kg on one truss?

19/12/06SAM_LGS_1, CTIO, Optics7 Laser Box Horizontal on SOAR Ring Pros: beam is folded up along a truss then over a spider arm so can be protected, M3 on LLT fixed. Cons: a shelf must be made on the telescope ring, the cable end of the box is positioned opposite to the nasmyths (could be good for the electronics control but bad for the cooling system).

19/12/06SAM_LGS_1, CTIO, Optics8 Laser Box (Hor./Vert.) at Bent-Cass port 2 Pros and Cons are the same as for all vertical (except on truss) and horizontal configurations, i.e. one mirror less and adjustable M3 on LLT v/s M3 fixed and one mirror more (M5). But the bent-cass port has one extra advantage, i.e. we can use the instrument holes that are already there.

19/12/06SAM_LGS_1, CTIO, Optics9 Laser Box Into the Bent-Cass port 2 Pros: most convenient from installation point of view. Cons: only  60mm space for fold mirror M5 and protecting tube and protection tube in the way of the SOAR M1 covers. Proposal: LB in same position but Outside the Tel.Ring (orange) M5 M4 M3

19/12/06SAM_LGS_1, CTIO, Optics10 To Do List Study the Laser cooling system Study the laser control system