The Need, Evolution, and Detail of WLAN Security
Computer science, engineering, software, hardware, computer science, PC, IT, processor, parallelism, silicon implementation, chip architecture, circuit design, CAD, computer aided design, embedded, programming languages, compilers, numerical analysis, tec
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10. Elements of a Wireless Sensor Architecture (June 3, 2009)
science, biology, history, energy, physics, technology, engineering, mathematics, design, computer science, habitat monitoring, data center, driver, transistor, power, RAM, ROM, flash, microcontroller, communication, computation, sensing, database, abioti
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7. Accelerating Computation in Seismic Data Processing (May 13, 2009)
science, physics, technology, engineering, mathematics, design, computer science, seismic computation, geophysics, research, application, acceleration, circuit, function, scalar approach, hardware, software, memory, computation, multicolor processor, stre
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Cosmology Lecture 7 (March 9, 2009)
Science, physics, Albert Einstein, matter-dominated universe, expansion, vacuum energy, Hubble constant, scale factor, horizon, surface of last scattering, Heisenberg uncertainty principle, harmonic oscillator, kinetic energy, ground state energy, zero-po
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Cosmology Lecture 4 (February 2, 2009)
Science, physics, cosmology, cosmic wavelength, photons, Doppler effect, Hubble law, speed of light, light rays, sound waves, expanding space, wave equations, scale factor, surface of last scattering, cosmic horizon, velocity of recession, Doppler shift,
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Cosmology Lecture 2 (January 19, 2009)
science, physics, Newton, Hubble constant, homogeneous, space-time, metric, force, velocity, galaxy, kinetic energy, potential energy, Big Bang, Big Crunch, isotropy, mass, sphere, escape velocity, cosmology, universe, gravity, curvature, relativity
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Statistical Mechanics Lecture 4 (April 20, 2009)
classical quantum physics, science, biology, engineering, theory, thermodynamics, math, formula, space, statistics, variable, methodology, probability distribution, entropy, Helm-Holtz free energy, control parameter, ideal gas, calculate system pressure,
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30. Fourier Transforms Lecture 30
Electrical, engineering, computers, math, physics, formulas, geometry, algebra, calculus, technology, functions, linear operations, sin, cosin, Fourier transformations, Fourier series, tomography, inverting, radon transform, medical imaging, circular symm
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Episode 3: Nuclear Power: Cure or Curse

Associate Professor Martin Sevior speaks with Jacky Angus and weighs up nuclear power in an energy-hungry and rapidly warming world.

Guest: Assoicate Professor Martin Sevior, School of Physics.
Topic: Nuclear power: Cure or Curse

Duration: 19 min 38 sec
Author(s): up-close@unimelb.edu.au (University of Melbourne)

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2.7 Reconsideration of the models and their suitability
From Rome to Pompeii and Ephesus the excavation of Roman remains is well known, but what of Roman remains in Africa? This unit looks at the Roman city of Thugga and examines the influence that Roman architecture and art had on Africa and its people.
Author(s): The Open University

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Licensed under a Creative Commons Attribution - NonCommercial-ShareAlike 2.0 Licence - see http://creativecommons.org/licenses/by-nc-sa/2.0/uk/ - Original copyright The Open University

2.6 Houses at Carthage, Bulla Regia and Thugga
From Rome to Pompeii and Ephesus the excavation of Roman remains is well known, but what of Roman remains in Africa? This unit looks at the Roman city of Thugga and examines the influence that Roman architecture and art had on Africa and its people.
Author(s): The Open University

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Licensed under a Creative Commons Attribution - NonCommercial-ShareAlike 2.0 Licence - see http://creativecommons.org/licenses/by-nc-sa/2.0/uk/ - Original copyright The Open University

2.5 African mosaics: things Roman and things African?
From Rome to Pompeii and Ephesus the excavation of Roman remains is well known, but what of Roman remains in Africa? This unit looks at the Roman city of Thugga and examines the influence that Roman architecture and art had on Africa and its people.
Author(s): The Open University

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Licensed under a Creative Commons Attribution - NonCommercial-ShareAlike 2.0 Licence - see http://creativecommons.org/licenses/by-nc-sa/2.0/uk/ - Original copyright The Open University

2.4 African Red Slip ware
From Rome to Pompeii and Ephesus the excavation of Roman remains is well known, but what of Roman remains in Africa? This unit looks at the Roman city of Thugga and examines the influence that Roman architecture and art had on Africa and its people.
Author(s): The Open University

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Licensed under a Creative Commons Attribution - NonCommercial-ShareAlike 2.0 Licence - see http://creativecommons.org/licenses/by-nc-sa/2.0/uk/ - Original copyright The Open University

2.2 Modelling cultural interaction
From Rome to Pompeii and Ephesus the excavation of Roman remains is well known, but what of Roman remains in Africa? This unit looks at the Roman city of Thugga and examines the influence that Roman architecture and art had on Africa and its people.
Author(s): The Open University

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Licensed under a Creative Commons Attribution - NonCommercial-ShareAlike 2.0 Licence - see http://creativecommons.org/licenses/by-nc-sa/2.0/uk/ - Original copyright The Open University

2.1 Looking in detail at Thugga
From Rome to Pompeii and Ephesus the excavation of Roman remains is well known, but what of Roman remains in Africa? This unit looks at the Roman city of Thugga and examines the influence that Roman architecture and art had on Africa and its people.
Author(s): The Open University

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Licensed under a Creative Commons Attribution - NonCommercial-ShareAlike 2.0 Licence - see http://creativecommons.org/licenses/by-nc-sa/2.0/uk/ - Original copyright The Open University

1 Thugga
From Rome to Pompeii and Ephesus the excavation of Roman remains is well known, but what of Roman remains in Africa? This unit looks at the Roman city of Thugga and examines the influence that Roman architecture and art had on Africa and its people.
Author(s): The Open University

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Licensed under a Creative Commons Attribution - NonCommercial-ShareAlike 2.0 Licence - see http://creativecommons.org/licenses/by-nc-sa/2.0/uk/ - Original copyright The Open University

1.6.3 The acceleration due to gravity
Motion is vital to life, and to science. This unit will help you to understand why classical motion is probably the most fundamental part of physics. You will examine motion along a line and the ways in which such motion can be represented, through the use of graphs, equations and differential calculus.
Author(s): The Open University

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Except for third party materials and otherwise stated (see http://www.open.ac.uk/conditions terms and conditions), this content is made available under a http://creativecommons.org/licenses/by-nc-sa/2

The Large Hadron Collider, the moon and some space scientists' heroes of science
In this physics and astronomy episode we chat to Dr Tara Shears just before the LHC was switched on in September 2008; catch up with two space scientists to find out about their heroes of science; and eavesdrop on a fascinating conversation between Dr Dave Rothery and Dr Mahesh Anand about the moon. The interviews are recorded by OU staff and the programme is hosted by Dr Mike Bullivant from the OU/BBC television series Rough Science.
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Lawrence Bailey - Market Research Valedictory Lecture - slides (as PDF)
A pdf of the slides used in Lawrence Bailey's guest lecture on Market Segmentation, Qualitative Research and Conversations Across the Garden Wall at Leeds Metropolitan University on 27 January 2011.
Author(s): Lawrence Bailey,Leeds Metropolitan University

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http://creativecommons.org/licenses/by-nc-sa/2.0/uk/

Physics Games: Liquid Crystals
Play a game and find out about a Nobel Prize awarded discovery or work! A liquid crystal is a substance that flows like a liquid but maintains some of the ordered structure characteristic of crystals. In the 1960s, a French theoretical physicist, Pierre-Gilles de Gennes turned his interest to liquid crystals and soon found fascinating analogies between liquid crystals and superconductors as well as magnetic materials. His work would later be rewarded with the Nobel Prize in Physics 1991. Today,
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