The merry-go-round analogy to explain Coriolis effect.
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Wednesday, 31 August 2011
Tuesday, 30 August 2011
Faraday's Law: Levitator
This Apparatus is a magnetic levitator, illustrating Lenz's law. The levitator can support an aluminum bowl about a foot in mid air in stable equilibrium.
Monday, 29 August 2011
Eureka! Episode 29 - Radiation Waves
Viewers learn that one of the chief ways in which heat energy moves is in the form of waves. This kind of heat transfer is called radiation.
Other Eureka episodes
Other Eureka episodes
Sunday, 28 August 2011
Saturday, 27 August 2011
Physics of the trumpet 1
Resonance, standing waves in a string with both ends fixed, penny whistle.
With Nick Drozdoff.
Other videos in this series
With Nick Drozdoff.
Other videos in this series
Friday, 26 August 2011
Sean Carroll: Distant time and the hint of a multiverse
At TEDxCaltech, cosmologist Sean Carroll attacks -- in an entertaining and thought-provoking tour through the nature of time and the universe -- a deceptively simple question: Why does time exist at all? The potential answers point to a surprising view of the nature of the universe, and our place in it.
Other TED Talks
Other TED Talks
Thursday, 25 August 2011
How Does a Van de Graaff Generator Work?
The inner workings of a Van de Graaff generator are revealed!
Other Frostbite Theater demonstrations
Other Frostbite Theater demonstrations
Wednesday, 24 August 2011
What is a Force?
Force is a central concept in physics. By analysing the forces on an object, its resulting motion can be determined. But what exactly is a force? The word force is used in everyday language in a variety of contexts, only some of which reflect the scientific definition of force. In this video, people at Victoria Park in Sydney are interviewed on their ideas of force and the forces that act on them.
Other Veritasium videos
Other Veritasium videos
Tuesday, 23 August 2011
Monday, 22 August 2011
Sunday, 21 August 2011
Reflection from an impedance discontinuity
Two segments of the Bell Labs apparatus are connected. The segments have different impedance. When a pulse travels from high impedance to low impedance, it is reflected with positive polarity and transmitted with positive polarity. When a pulse travels from low impedance to high impedance, it is reflected with negative polarity and transmitted with positive polarity.
Source: MIT TechTV
See other MIT physics demos
Source: MIT TechTV
See other MIT physics demos
Saturday, 20 August 2011
MIT 8.01 Classical Mechanics Lecture 23
MIT Physics Course
Professor Walter Lewin
Doppler effect, binary stars, x-ray binaries, neutron Stars and black holes
See other videos in this series.
Friday, 19 August 2011
Thursday, 18 August 2011
Wednesday, 17 August 2011
Eureka! Episode 28 - Heat as Energy
Heat is produced whenever there is movement and friction between two objects. Since movement is a form of energy, it follows that heat must also be a form of energy.
Other Eureka episodes
Other Eureka episodes
Tuesday, 16 August 2011
How Far Away is the Moon? (The Scale of the Universe)
If the Earth were the size of a basketball and the moon a tennis ball, how far apart would they be? Diagrams that are not to scale make us think that they're closer than they really are.
Other Veritasium videos
Other Veritasium videos
Monday, 15 August 2011
Sunday, 14 August 2011
MIT 8.02 Electricity and Magnetism Lecture 4
MIT 8.02 Electricity and Magnetism, Spring 2002
Professor Walter Lewin
Electrostatic potential, electric energy, conservative field, equipotential surfaces.
Saturday, 13 August 2011
Steel Ball Dropped in a Viscous Fluid
Five steel balls of different sizes are dropped into corn syrup. The balls reach a constant velocity shortly after entering the fluid. The velocity is constrained due to the drag balancing the force of gravity in the fluid. This demonstrates the relationship between the size of the ball and the maximum velocity it can obtain.
Source: MIT TechTV
See other MIT physics demos
Source: MIT TechTV
See other MIT physics demos
Big Numbers - Sixty Symbols
Big numbers: Avogadro's Number, number of protons in the universe, Dirac large numbers hypothesis.
Other Sixty Symbols videos
Other Sixty Symbols videos
Friday, 12 August 2011
Electric Generator
This is an alternating current generator: a conducting coil (shown in yellow) rotates inside a magnetic field (the field lines are green here). The vector "A" is perpendicular to the area of the coil (its magnitude is the area of the coil). During rotation of the coil, the magnetic flux changes and an alternating current is induced in the coil. The first graph show the magnetic flux, the other graph shows current intensity.
Other animations by Yves Pelletier
Other animations by Yves Pelletier
Thursday, 11 August 2011
Eureka! Episode 27 - Convection
This program explains how the principle of buoyancy is responsible for the process of heat transfer called convection.
Other Eureka episodes
Other Eureka episodes
Wednesday, 10 August 2011
Egg Experiment to Demonstrate Inertia
If you spin a raw egg and then stop it, it will start spinning again without you having to touch it. A boiled egg, on the other hand, stops and stays stopped. Why is this? Well a raw egg contains a yolk that moves inside the egg independently of the shell. If you stop the shell, the yolk inside continues to move due to its inertia and it therefore gets the egg spinning again.
Other Veritasium videos
Other Veritasium videos
Tuesday, 9 August 2011
Exploring the universe: Schools Lecture 2009
The Institute of Physics Schools and Colleges Lecture 2009 is delivered by astronomer Dr Andrew Newsam. This lecture will reveal how:
- Modern telescopes can be used by astronomers to look at the universe in ever greater detail;
- Progress in technology allows astronomers to observe things further and further away and therefore further back in time;
- Astronomical observations can be used to learn more about the origins and future of the universe.
Monday, 8 August 2011
Field Lines in a Toroidal Solenoid
This animation illustrates the magnetic field lines created by a series of loops that form a torus. The animation shows how increasing number of current loops confines the magnetic field to the interior of the torus.
Other animations by Penn State Schuylkill
Other animations by Penn State Schuylkill
Sunday, 7 August 2011
MIT 8.01 Classical Mechanics Lecture 22
MIT Physics Course
Professor Walter Lewin
Kepler's Laws - Elliptical Orbits - Satellites - Change of Orbits - Orbiting Ham Sandwich!
See other videos in this series.
Saturday, 6 August 2011
Magnetic Field - Sixty Symbols
Check out this super powerful magnet - just don't get too close with a video camera!
Other Sixty Symbols videos
Other Sixty Symbols videos
Friday, 5 August 2011
Circuit Skills: Fiber Optics
Not all electronic signals are communicated via electricity. By transmitting information in the form of light, we can avoid many limitations inherent to traditional wiring. And on top of all that - fiber optics are just straight-up cool!
Sport vs Physics
2004 lecture by Dr Dave James (Sheffield University) as part of the Institute of Physics Schools and Colleges Lecture Tour.
Physics applied to sprint, pole vault, javelin, wheelchair racing, soccer and tennis.
(Found in Physics and Physicists)
Other videos by Institute of Physics
Physics applied to sprint, pole vault, javelin, wheelchair racing, soccer and tennis.
(Found in Physics and Physicists)
Other videos by Institute of Physics
Thursday, 4 August 2011
MIT 8.02 Electricity and Magnetism Lecture 3
MIT 8.02 Electricity and Magnetism, Spring 2002
Professor Walter Lewin
Electric flux and Gauss law.
Wednesday, 3 August 2011
Eureka! Episode 26 - Buoyancy
Showing viewers that objects immersed in a liquid are buoyed up by a force equal to the weight of the liquid displaced, this program explains the principle of buoyancy.
Other Eureka episodes
Other Eureka episodes
Tuesday, 2 August 2011
The Difference Between Mass and Weight
There is a common perception that weight and mass are basically the same thing. This video aims to tease out the difference between mass and weight by asking people what makes a car difficult to push. The standard answer is that it is difficult to push because it's heavy. But heaviness is a measure of weight, the gravitational pull of the Earth attracting the car to Earth's center. When the car is pushed on a flat road, the force of gravity does not oppose the motion. Instead the resistance felt is an indication of the car's mass which determines its inertia. Inertia is the property of matter that means it tends to resist acceleration - the greater the mass, the less the acceleration for a given amount of force.
Other Veritasium videos
Other Veritasium videos
Julius Sumner Miller - Pascal Principle
Sciences demonstrations #14: Pascal Principle
Pascal principle, hydraulic press...
Other physics demonstrations by Julius Sumner Miller
Pascal principle, hydraulic press...
Other physics demonstrations by Julius Sumner Miller
Monday, 1 August 2011
Degrees of Angle - Sixty Symbols
We look at astronomy and nanotechnology in this film about angles, focusing especially on the tilt of the Earth's axis and the pole star (aka polaris). More at http://www.sixtysymbols.com/
Other Sixty Symbols videos
Other Sixty Symbols videos
Yale: Frontiers and Controversies in Astrophysics, Lecture 16
Source: Yale University, Open Yale Courses
Lecture 16: Hubble's Law and the Big Bang
The third and final part of the course begins, consisting of a series of lectures on cosmology. A brief history of how cosmology developed into a scientific subject is offered. The discovery of dark energy, along with dark matter, played a crucial role in the development of cosmology. The lecture then discusses the discovery of spiral nebulae in 1920, as well as the "Great Debate" over what they were. Hubble's famous redshift diagram is presented as the basis for Hubble's Constant and Big Bang cosmology. The difficulty of measuring distance of objects in space, and how to do it using the parallax method and the standard candle method, are discussed. Measure brightness using the magnitude scale is explained. Class ends with a review of logarithms.
00:00 - Chapter 1. Introduction to Cosmology
03:34 - Chapter 2. Spiral Nebulae and Hubble's Redshift Diagram
17:35 - Chapter 3. Measuring the Distance of a Star: The Parallax Method
25:13 - Chapter 4. Measuring Brightness: The Standard Candle Method
38:06 - Chapter 5. Absolute and Apparent Magnitude
48:04 - Chapter 6. Conclusion
Other lectures from this course
Lecture 16: Hubble's Law and the Big Bang
The third and final part of the course begins, consisting of a series of lectures on cosmology. A brief history of how cosmology developed into a scientific subject is offered. The discovery of dark energy, along with dark matter, played a crucial role in the development of cosmology. The lecture then discusses the discovery of spiral nebulae in 1920, as well as the "Great Debate" over what they were. Hubble's famous redshift diagram is presented as the basis for Hubble's Constant and Big Bang cosmology. The difficulty of measuring distance of objects in space, and how to do it using the parallax method and the standard candle method, are discussed. Measure brightness using the magnitude scale is explained. Class ends with a review of logarithms.
00:00 - Chapter 1. Introduction to Cosmology
03:34 - Chapter 2. Spiral Nebulae and Hubble's Redshift Diagram
17:35 - Chapter 3. Measuring the Distance of a Star: The Parallax Method
25:13 - Chapter 4. Measuring Brightness: The Standard Candle Method
38:06 - Chapter 5. Absolute and Apparent Magnitude
48:04 - Chapter 6. Conclusion
Other lectures from this course