CONSULTANCY FOR THE HIGH TECH INDUSTRY             BACK

 

 

Contact:

Fred Kamphues

Mill House

The Netherlands

Email:

 

 

                  

 

Mill House Engineering and Management Consultancy has over 25 years experience in supporting state-of-the art technology projects. Activities include project management, MAIT management, product development and marketing & sales support.

 

 

 P R O J E C T      O V E R V I E W  : 

 

VLT Laser Guide Star Launch Telescopes

Project manager, procurement manager and AIT manager for the Laser Launch Telescopes of the 4LGSF for the Very Large Telescope (VLT) at TNO.

The Laser Guide Star forms a part of the new adaptive optics (AO) system of the UT4 telescope. The AO system corrects for atmospheric turbulence disturbances, thereby vastly increasing the useful resolution of the telescope.

 

The 4 LGSF consists of a high power 25 W CW 589 nm laser, a Beam Conditioning and Diagnostics System (BCDS) and an Optical Tube Assembly (OTA). OTA is a 20x Galilean beam expander, with a 15 mm diameter input beam and a steerable 300 mm diameter collimated output beam. OTA employs four optical elements, a Quarter Wave Plate, a small double concave L1 lens, a Field Selector Mirror and a highly aspherical 380 diameter mm L2 lens. The design is passively athermalized over a large temperature range as well as under the influence of thermal gradients.
To achieve 4.8 arcmin radius field of view on-sky, the FSM has to tilt up to ±6.1 mrad, in combination with less than 1.5 µrad RMS absolute accuracy. The FSM design consists of a Zerodur mirror, bonded to a membrane spring and strut combination to allow only tip and tilt. Since the range is too large for piezos, two (self-locking) spindle drives actuate the mirror, using a stiffness based transmission to increase resolution. Absolute accuracy is achieved with two differential inductive sensor pairs.

 

VLT Laser Guide Star

photo: ESO/Fred Kamphues

 

VLT 4LGSF OTA

photo: Mill House/Fred Kamphues

courtesy of TNO

 

GAIA Basic Angle Monitoring system

Consultancy for TNO for the development of a Basic Angle Monitoring Opto Mechanical Assembly for GAIA. The Gaia mission will create an extraordinarily precise three-dimensional map of more than one billion stars in our Galaxy. Part of ESA's Cosmic Vision programme, the Gaia spacecraft was being built by EADS Astrium and was launched on December 19, 2013. TNO has developed the all Silicon Carbide Basic Angle Monitoring Opto-Mechanical Assembly (BAM OMA) for this mission.

 

The GAIA satellite measures the angles between stars using two telescopes set at a fixed angle of 106.5°, named the Basic Angle. The astrometric measurements will be accurate to 24 microarcsec (at 15 magnitude), comparable to measuring the diameter of a human hair at a distance of 1000 kilometres. This requires ultra high stability, which can only be achieved by using Silicon Carbide for the optical bench and telescopes. In addition the Basic Angle variation shall be measured within a precision of 0.5 microarcsec. Therefore GAIA is equipped with a Basic Angle Monitoring subsystem, a metrology system to monitor the angle between the two telescopes. This system consists of two laser interferometers. Two pairs of parallel laser bundles are sent to the two telescopes, which create two interference patterns on a detector. If the basic angle varies, the interference patterns will shift. With the BAM an Optical Path Difference (OPD) as small as 1.5 picometers RMS can be measured.

Gaia BAM

photo: Mill House/Fred Kamphues

courtesy of TNO

 

 

GAIA spacecraft

illustration: ESA/Medialab

 

Nano-actuator for E-ELT

Development of a breadboard nano-actuator for TNO. A prototype actuator has been built and tested. The prototype actuator is designed to accurately co-phase the 786 hexagonal segments of the 39 meter diameter main mirror of the European Extremely Large Telescope (E-ELT).

 

European Extremely Large Telescope

illustration: ESO

 

VLT Interferometer Delay Line

Assembly, Integration and Testing (AIT) manager and lead mechanical engineer for the overall mechanical design of the first three Delay Lines for the Very Large Telescope Interferometer (VLTI) for ESO, under the responsibility of Fokker Space (see also ESO press release).

The work consisted of the design of highly accurate mechanical components, with strong links to other disciplines (optics, electronics and software), as well as final adjustment of mechanical components of the first VLTI Delay Line at the VLT facility in Paranal, Chile.

 

VLTI delay lines in the tunnel at Cerro Paranal

photo: Mill House/Fred Kamphues

 

Motor Racing - Formula 1

Component development and production for Benetton Formula Ltd. Technical details are classified.

Mill House made an important contribution to 35 podium finishes, including 12 Grand Prix victories, one Driver Formula One title (Michael Schumacher in 1995) and one Constructor Formula One title.

 

Johny Herbert/Benetton B195

photo: Rick Dikeman

 

Solar Arrays and Release Mechanisms for satellites

Consultant for the development of a solar array production line at Fokker Space.

Assembly, Integration and Test (AIT) manager for the Nilesat and Worldstar 2 & 3 solar arrays at Fokker Space.

Consultant for Fokker Space for the concept definition, mechanical design and AIT for the solar array of the Automated Transfer Vehicle (ATV) to the International Space Station.

Consultant for various Holddown and Release Systems for Fokker Space (Quickbird, AXAF, Sciamachy).

 

Nilesat solar array

photo: Fokker Space

Unicef Flyer

Responsible for the design and development of the tank release system.

The project was one of the attempts to fly non-stop around the world in a hot air balloon.

 

Unicef Flyer

photo: Mill House/Fred Kamphues

 

Software development for Motor Racing - F3000 and Indy Cars

1996: Data aquisition engineer for Auto Sport Racing (ASR) with Thomas Biagi in the 1996 International F3000 Championship.

1996: Implementing of spare part logistics and mileage database software for Auto Sport Racing (ASR) in F3000.

1996: Development of car setup database software for Auto Sport Racing (ASR) in F3000.

1994: Implementing of spare part logistics and mileage database software for Arie Luyendyks Indy Car team Indy Regency Racing.

1993: Development of spare part logistics and mileage database software for Crypton Engineering in F3000.

1993: Development of car setup database software for Crypton Engineering in F3000. 

 

Arie Luyendyk

photo: Mill House/Fred Kamphues

 

 

 P U B L I C A T I O N S : 

 

 

 2014: 

 

Damping in space constructions, Jan de Vreugd et al, European Conference on Spacecraft Structures, Materials & Environmental Testing, Braunschweig, April 2014

 

 

 2013: 

 

Star Separators for the Very Large Telescope Interferometer - Increasing sensitivity for distant planets and supermassive black holes, Jan Nijenhuis and Fred Kamphues, Mikroniek, Vol. 53, issue 3, June 2013

 

 

 2012: 

 

* Design, analysis, and testing of the optical tube assemblies for the ESO VLT four laser guide star facility, SPIE Volume 8447-172, July 2012

* Gaia basic angle monitoring system, SPIE Volume 8442-61, July 2012

 

 

 2011: 

 

Optical Tube Assemblies for the ESO VLT Four Laser Guide Star Facility, Second international conference on Adaptive Optics for Extremely Large Telescopes, Victoria, BC, Canada, September 2012.

* Athermal design of the Optical Tube Assemblies for the ESO VLT Four Laser Guidestar Facility (Conference Proceedings Paper), Optical Engineering + Applications, SPIE Volume 8149-04, August 2011.

 

 

 2009: 

 

* Picometer metrology for the GAIA mission (Conference Proceedings Paper), Astronomical and Space Optical Systems, SPIE Volume 7439, August 2009

* Corrective polishing of strongly curved aspheric silicon carbide mirrors (Conference Proceedings Paper), SPIE Optifab, May 2009

Picometer metrologie voor de Gaia missie, NVR Ruimtevaart 2009-2

 

 

 2008:

 

Astronomische Telescopen, article in NVPT Yearbook 2009, November 2008, NVPT 

 

Pico Meter Metrology for Gaia mission, International Conference on Space Optics (ICSO) 2008, October 2008 

 

Picometre metrology in space, article in Mikroniek, periodical for precision technology, June 2008

 

* Picometer metrology for the Gaia mission (Conference Proceedings Paper), Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, 12 July 2008, SPIE Volume 7010

 

* Simultaneous observation of two stars using the Prima Star Separator (Conference Proceedings Paper), Space Telescopes and Instrumentation 2008: Instruments, July 2008, SPIE Volume 7013

 

* PACT: the actuator to support the primary mirror of the E-ELT (Conference Proceedings Paper), Space Telescopes and Instrumentation 2008: Segment mirror technologies, July 2008, SPIE Volume 7018

 

 2007:

 

* The development of a breadboard cryogenic optical delay line for Darwin (Conference Proceedings Paper), Cryogenic Optical Systems and Instruments XII, 66920A, 17 September 2007, SPIE Volume 6692

 

The development of a breadboard cryogenic optical delay line for Darwin, 12th European Space Mechanisms and Tribology Symposium (ESMATS) 2007

 

Darwin - Een optische vertragingslijn voor een ruimtetelescoop, NVPT Yearbook 2007, text: Ben Braam, Teun van den Dool, Fred Kamphues

 

 2006:

 

* The DARWIN breadboard optical delay line verification programme (Conference Proceedings Paper), Advances in Stellar Interferometry, 62682O, 28 June 2006, SPIE Volume 6268

 

* The Darwin Breadboard Cryogenic Optical Delay Line, Sixth International Conference on Space Optics, Proceedings of ESA/CNES ICSO 2006, held 27-30 June 2006 at ESTEC, Noordwijk, The Netherlands. Edited by A. Wilson. ESA SP-621. European Space Agency, 2006.

 

 

 2005:

 

* The manufacturing, assembly and acceptance testing of the breadboard cryogenic optical delay line for DARWIN, SPIE  Conference Optics and Photonics [5904- p. 367-377], August 2005, San Diego, USA

 

The development of a cryogenic delay line for DARWIN, ICMENS  Conference, July 2005, Banff, Canada

 

 

2004:

 

* Magnetic Bearing optical delay line,  SPIE Conference Optical Science and Technology [5528A-37], August 2004, Denver, USA

 

Metrology concept design of the GAIA basic angle monitoring system,  SPIE Conference Astronomical Telescopes and Instrumentation SPIE [5495-02], june 2004, Glasgow, UK

 

* DARWIN cryogenic optical delay line, SPIE Conference Astronomical Telescopes and Instrumentation [5495-40], June 2004, Glasgow, UK

 

* Advanced optical delay line demonstrator, SPIE Conference Astronomical Telescopes and Instrumentation [5495-41], June 2004, Glasgow, UK

 

 

 2000:

 

Test results of the VLTI delay line system verification program, H. Hogenhuis, Fokker Space B.V. (Netherlands), SPIE Conference Astronomical Telescope and Instrumentation [4006-22], March 2000, Munich, Germany

 

 

* © COPYRIGHT SPIE - These papers are published in the Proceedings of various SPIE Conferences and are made available as an electronic reprint with permission of SPIE.  One print or electronic copy may be made for personal use only.  Systematic or multiple reproduction, distribution to multiple locations via electronic or other means, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.