Richard Wade PSD 2007 PPARC Science Challenges. Position sensitive detectors and PPARC Technology Challenges. Big Questions, Big Projects. Developing technology,

Slides:



Advertisements
Similar presentations
Observation of the Universe from the Moon – Elisabetta Cavazzuti – LNF May 7, 2007 ITALIAN VISION FOR MOON EXPLORATION OBSERVATION OF THE UNIVERSE FROM.
Advertisements

Professor Dave Delpy Chief Executive of Engineering and Physical Sciences Research Council Research Councils UK Impact Champion Competition vs. Collaboration:
8.2 Exploring the Sun Homework: page 340 # 2, 3, 5, 7, 9
Panel created in 2001 as part of restructuring of PPARC Advisory Structure One of five advisory panels: Astronomy Advisory Panel (AAP) Solar System Advisory.
Space Science and Technology Looking up – looking down Peter Allan STFC Head of Space Data Division.
Towards Better Exploitation and Economic Impact: Developing the EPSRC Partnership with the University Vince Osgood Associate Director, Economic Impact.
The Engineering and Physical Sciences Research Council › We are the main UK government agency for funding research and training in engineering and the.
Philip Diamond RadioNet Co-ordinator University of Manchester Jodrell Bank Observatory.
Announcements Turn in Homework 5, pick up Homework 6. Another test this week! Same days (W,Th), same format as before. First project due October 13.
The Electromagnetic Spectrum
Committee on Science, Engineering and Public Policy Board on Physics and Astronomy Committee on Setting Priorities for NSF’s Large Research Facility Projects.
LHC Experiments at Liverpool E2V Visit – Nov 2005 Introduction Si Technology Upgrade/Maintenance Summary.
Gravitational waves LIGO (Laser Interferometer Gravitational-Wave Observatory ) in Louisiana. A laser beam is.
Gamma-Ray Astronomy Dana Boltuch Ph. D
NASA_G_O_02_09_05.ppt 1 National Goals and Objectives National Goal To advance U.S. scientific, security, and economic interests through a robust space.
Reading Unit 28, Unit 29, Unit 30 Will not be covered by the first exam.
Electromagnetic Spectrum Identify and explain how different parts of the electromagnetic spectrum are used.
CHIPP Workshop on Detector R&D June - University of Geneva Common R&D for astroparticle physics: Activities of ApPEC and ASPERA Bernard Revaz and.
Seeing the Invisible Prof. Lynn Cominsky Sonoma State University Director, Education and Public Outreach.
Scientists learn about the Universe by collecting Wave- Energy from the Electromagnetic Spectrum.
Point 1 activities and perspectives Marzio Nessi ATLAS plenary 2 nd October 2004 Large Hadron Collider (LHC)
Science and Society - the example of the LHC Mike Green Royal Holloway University of London.
ASPERA Status Astronet GB 20 September 2006 S.Katsanevas CNRS/IN2P3.
A new start for the Lisbon Strategy Knowledge and innovation for growth.
Exploring the Universe Harcourt Science Unit D Chapter 4 Mrs.Strand 6th grade Lockwood Middle School.
Prospects in space-based Gamma-Ray Astronomy for Europe --- Objective of the meeting Jürgen Knödlseder Centre d’Etude Spatiale des Rayonnements, Toulouse,
Knowledge Transfer | Accelerating Innovation Turkey – CERN Industry Day, , D. Mazur David Mazur IP Dissemination Section Leader Knowledge Transfer.
6.3 Telescopes and the Atmosphere 6.4 Eyes and Cameras: Everyday Light Sensors Our goals for learning How does Earth’s atmosphere affect ground-based observations?
THE ATTRACT INITIATIVE Marzio Nessi, Markus Nordberg CERN.
National Aeronautics and Space Administration November 23, Gamma-ray Large Area Space Telescope (GLAST) Kevin Grady, Project Manager Steven Ritz,
ATLAS experiment at the CERN Large Hadron Collider Peter Watkins, Head of Particle Physics Group, University of Birmingham, UK
Black Holes - Observation How do you see something you can’t see ?????
Aim: How can we explain the four fundamental forces and the standard model? Do Now: List all the subatomic particles that you can think of.
E-Science Research Councils awarded e-Science funds ” science increasingly done through distributed global collaborations enabled by the Internet, using.
Particle Physics Research - Birmingham group HEFCE academic staff 7 Research staff 13, Engineers 2, Technicians 2 PhD students 12.
The Nucleus Nucleons- the particles inside the nucleus: protons & neutrons Total charge of the nucleus: the # of protons (z) times the elementary charge.
5.1 Electromagnetic Radiation. Wave motion The transfer of energy without matter is called wave motion Two Types.
Space Science Chapter 1. Bell Work 1/4/10  Welcome Back! I hope you all enjoyed your break.  Please obtain a pink sheet from the counter by the sinks.
WILGA k61/10 Search for cosmic rays from gamma ray bursts Marcin Molak Faculty of Physics Warsaw University of Technology.
Steve Worm – Gateway CentresApril 25, The Gateway Centres and their context in the STFC Strategy Steve Worm Rutherford Appleton Laboratory.
Build on success to show feasibility of scale-up and physics capability [Brunel, Durham, Sheffield, Sussex, AAE Ltd., e2v Ltd., Rhyal Ltd., Technodyne.
The Square Kilometre Array Dr. Minh Huynh (International Centre for Radio Astronomy Research and SKA Program Development Office) Deputy International SKA.
Space Telescopes.
Energy Transfer & Transformations How does energy impact the motion of an object?
Sponge: Draw the four types of reflectors.. Light from different directions focuses at different points, and an image is formed near the prime focus.
Astronomy. What is astronomy? Astronomy is the study of the universe and its components. –Planets –Stars –Galaxies –Moons –Comets –Black holes They study.
1) Name the planets in our solar system in order
The Engineering and Physical Sciences Research Council Funding (EPSRC)
Chapter 14 Section 14.1.
Unit 13: Particle Physics Four fundamental interactions in nature 1.Strong – responsible for binding neutrons and protons into nuclei 2.Electromagnetic.
ASP2011 Measurement Techniques Lectures 7-8 Dr. Duncan Galloway University of Melbourne
Delivering Innovation Prof. Janet Bainbridge Senior Specialist Advisor Government & Europe One NorthEast
Robin Clegg EPPOG 7Apr06 PPARC AND PUBLIC ENGAGEMENT WITH PARTICLE PHYSICS Robin Clegg Science and Society programme PPARC Swindon Office.
Black Holes By: Kat Dygowski Mr. Reed Science 1 Period:6 November 10 th, 2012.
Name: P4 6 mark question practice All 6 mark questions are marked using the following Quality of Written Answer guidelines: LEVEL 3 (5-6 marks) Answer.
HPRF Faraday Partnership Industrial Activities in support of Accelerator Science David Wilcox Doug Clunie HPRF Faraday Partnership 26 September 2006.
High Energy Observational Astrophysics. 1 Processes that emit X-rays and Gamma rays.
BY: SAMANTHA 9B Space and Gravity. Definitions Gravity- the force that attracts a body towards the centre of the earth, or towards any other physical.
CPM 2012, Fermilab D. MacFarlane & N. Holtkamp The Snowmass process and SLAC plans for HEP.
The Structure of UK Science: Lessons to be learned. Ian Halliday Chief Executive Particle Physics and Astronomy Research Council.
Space And Gravity By Dylan Vaghela 9B. Gravity Gravity-the force that attracts a body towards the center of the earth, or towards any other physical body.
Capabilities and Programmes of STFC’s Accelerator Science & Technology Centre (ASTeC)
The Quest for Gravitational Waves: a global strategy
National Goals and Objectives
Space and Gravity By:Nikitha.
John Womersley Super-B Workshop Oxford May 2011
The Structure of UK Science: Lessons to be learned.
Nature of Electromagnetic Waves
Stanford Linear Accelerator
Astronomy.
Presentation transcript:

Richard Wade PSD 2007 PPARC Science Challenges. Position sensitive detectors and PPARC Technology Challenges. Big Questions, Big Projects. Developing technology, working with industry.

PPARC Science Challenges How did the Universe begin and how (and when) will it end? How do stars, planets and galaxies form? Are we alone in the Universe or is there life elsewhere? What is the Universe made of and what holds it together? Where does mass come from? How does the Sun work and how does it affect the Earth? Why does there seem to be much more matter in the Universe than anti-matter?

Position Sensitive Detectors and PPARC Detector Systems key to PPARC Science Virtually every conceivable form of detector employed in PPARC science area –CCDs –Silicon strip –Wire chambers –Hybrid photomultipliers –TES

Position Sensitive Detectors and PPARC Gamma rays to radio waves Particles (charged particles, neutrinos, WIMPS, …….) Gravitational Waves

WHT Wide Field Camera

CFHT MegaCam 40 e2v CCDs, 377 Mpixels

SLAC vertex detector

XMM-EPIC Focal Plane Array

SCUBA

SCUBA 2 10,000 pixels 100 times faster than SCUBA

VISTA IR Camera

VISTA Camera 16 Raytheon VIRGO 2048x2048 HgCdTe arrays

Big Questions, Big Projects

Big Questions Big Projects (large capital projects) Extremely Large telescopes Future European Gravitational Wave Detectors Linear Collider Neutrino Factory Double Beta Decay

Big Questions Big Projects Aurora (Mars exploration) XEUS (Next Generation X-ray observatory) DARWIN (search for planets) LISA (space based gravitational wave observatory) LHC upgrades, super LHC? CLIC

Big Questions Big Projects Extremely Large Telescopes

Big Questions Big Projects Aurora

Big Questions Big Projects LHC

Big Questions Big Projects Linear Collider

Enabling Technology Development and Knowledge Transfer. Technology Development Working with industry Knowledge transfer and exploitation

Technology Development Project based technology road-mapping. Single fund for Project R&D. Project funded studentships. Four year studentships available.

Working With Industry Opening up funding to industry. Trial scheme being run by PPARC –initially for AURORA but then for Project R&D.

Knowledge Transfer and Exploitation News PIPSS –Focus on knowledge transfer Extended brokerage scheme

Science and Innovation Investment Framework World class research at the UKs strongest centres of excellence. Greater responsiveness to the needs of the economy (knowledge transfer) Increased business investment in R&D and increased business engagement in drawing on the UK science base for ideas and talent. A strong supply of scientists, engineers and technologists. Sustainable and financially robust universities.

Science and Innovation Investment Framework PPARC is well placed to deliver the governments goals and is in a fantastic position to inspire the next generation of scientist and engineers.

“There are no such things as applied sciences, only applications of science”. Louis Pasteur Science and Innovation Investment Framework