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Please go here if you want to suggest other nice physics videos, and here if I mistakingly infringed your copyrights. If you understand French, you'll find a huge selection of physics videos in French in my other blog Vidéos de Physique.
Showing posts with label Fluids and Thermodynamics. Show all posts
Showing posts with label Fluids and Thermodynamics. Show all posts
Thursday, 24 December 2015
The Physics of Hot Air Balloons
Monday, 7 September 2015
How to Escape Quicksand
You probably won’t get stuck in quicksand. But if you do, you can use physics to get yourself out.
Libellés :
Fluids and Thermodynamics,
The Sci Show
Monday, 15 June 2015
Why Raindrops Are Mathematically Impossible
Rain shouldn't happen, according to basic physics.
Libellés :
Fluids and Thermodynamics,
Minute Physics
Friday, 10 April 2015
How Do Airplanes Fly?
How do airplanes fly?
Libellés :
Classical Mechanics,
Fluids and Thermodynamics,
Minute Physics
Sunday, 25 January 2015
Using Lasers to Create Super-hydrophobic Materials
Scientists at the University of Rochester have used lasers to transform metals into extremely water repellent, or super-hydrophobic, materials without the need for temporary coatings.
Libellés :
Fluids and Thermodynamics,
Laser
Sunday, 16 November 2014
How a Crookes radiometer works
A Crookes radiometer is driven by a thermal gas effect, and not "light pressure" as often thought. Ben Krasnow demonstrates the radiometer in a vacuum chamber and explain its optimal running pressure.
Libellés :
Applied Science,
Fluids and Thermodynamics,
Radiometer
Sunday, 31 August 2014
Air Pressure Can Crush with Physics Girl and Walter Lewin
Can crushed by atmospheric pressure.
Libellés :
Fluids and Thermodynamics,
Physics Girl,
Pressure
Friday, 22 August 2014
Why do ice cubes crack in drinks?
Dropping ice cubes in water (and liquid nitrogen) produce interesting results. Differential expansion.
Libellés :
Fluids and Thermodynamics,
Periodic Videos
Thursday, 21 August 2014
Magnetic Hair
MIT engineers have fabricated a new elastic material coated with microscopic, hairlike structures that tilt in response to a magnetic field. (Learn more about these structures: http://bit.ly/1y2E8SX)
Depending on the field's orientation, the microhairs can tilt to form a path through which fluid can flow; the material can even direct water upward, against gravity.
Libellés :
Electricity and Magnetism,
Fluids and Thermodynamics,
Magnetism
Wednesday, 20 August 2014
How do tornadoes form? - James Spann
Tornadoes are the most violent storms on Earth, with wind velocities that can exceed 200 miles per hour. How do these terrifying cyclones form? Meteorologist James Spann sheds light on the lifespan of tornadoes as they go from supercell thunderstorms to terrible twisters before eventually dissolving back into thin air.
Lesson by James Spann, animation by Província Studio.
Lesson by James Spann, animation by Província Studio.
Libellés :
Fluids and Thermodynamics,
TED
Monday, 16 June 2014
Why is ketchup so hard to pour? - George Zaidan
Ever go to pour ketchup on your fries...and nothing comes out? Or the opposite happens, and your plate is suddenly swimming in a sea of red? George Zaidan describes the physics behind this frustrating phenomenon, explaining how ketchup and other non-Newtonian fluids can suddenly transition from solid to liquid and back again.
Lesson by George Zaidan, animation by TOGETHER.
Lesson by George Zaidan, animation by TOGETHER.
Libellés :
Fluids and Thermodynamics,
TED
Saturday, 3 May 2014
A Baffling Balloon Behavior - Smarter Every Day 113
Helium balloon in an accelerating car.
Libellés :
Classical Mechanics,
Dynamics,
Fluids and Thermodynamics,
Inertia,
Smarter Every Day
Monday, 10 February 2014
Hewitt-Drew-it! PHYSICS 93. Water and Electron Circuits
The similarities and differences between electric and hydraulic circuits.
Libellés :
Electric current,
Electric Potential,
Electricity,
Electricity and Magnetism,
Fluids and Thermodynamics,
Hewitt-Drew-it
Sunday, 19 January 2014
NASA | Jewel Box Sun
This video of the sun based on data from NASA's Solar Dynamics Observatory, or SDO, shows the wide range of wavelengths -- invisible to the naked eye -- that the telescope can view. SDO converts the wavelengths into an image humans can see, and the light is colorized into a rainbow of colors.
As the colors sweep around the sun in the movie, viewers should note how different the same area of the sun appears. This happens because each wavelength of light represents solar material at specific temperatures. Different wavelengths convey information about different components of the sun's surface and atmosphere, so scientists use them to paint a full picture of our constantly changing and varying star.
Yellow light of 5800 Angstroms, for example, generally emanates from material of about 10,000 degrees F (5700 degrees C), which represents the surface of the sun. Extreme ultraviolet light of 94 Angstroms, which is typically colorized in green in SDO images, comes from atoms that are about 11 million degrees F (6,300,000 degrees C) and is a good wavelength for looking at solar flares, which can reach such high temperatures. By examining pictures of the sun in a variety of wavelengths -- as is done not only by SDO, but also by NASA's Interface Region Imaging Spectrograph, NASA's Solar Terrestrial Relations Observatory and the European Space Agency/NASA Solar and Heliospheric Observatory -- scientists can track how particles and heat move through the sun's atmosphere.
The 2.9 minute movie was created by NASA's Scientific Visualization Studio or SVS at NASA's Goddard Space Flight Center in Greenbelt, Maryland, and is available at the SVS website: http://svs.gsfc.nasa.gov/goto?11385
As the colors sweep around the sun in the movie, viewers should note how different the same area of the sun appears. This happens because each wavelength of light represents solar material at specific temperatures. Different wavelengths convey information about different components of the sun's surface and atmosphere, so scientists use them to paint a full picture of our constantly changing and varying star.
Yellow light of 5800 Angstroms, for example, generally emanates from material of about 10,000 degrees F (5700 degrees C), which represents the surface of the sun. Extreme ultraviolet light of 94 Angstroms, which is typically colorized in green in SDO images, comes from atoms that are about 11 million degrees F (6,300,000 degrees C) and is a good wavelength for looking at solar flares, which can reach such high temperatures. By examining pictures of the sun in a variety of wavelengths -- as is done not only by SDO, but also by NASA's Interface Region Imaging Spectrograph, NASA's Solar Terrestrial Relations Observatory and the European Space Agency/NASA Solar and Heliospheric Observatory -- scientists can track how particles and heat move through the sun's atmosphere.
The 2.9 minute movie was created by NASA's Scientific Visualization Studio or SVS at NASA's Goddard Space Flight Center in Greenbelt, Maryland, and is available at the SVS website: http://svs.gsfc.nasa.gov/goto?11385
Libellés :
Astrophysics,
Fluids and Thermodynamics,
NASA,
Waves-Optics-Acoustics
Thursday, 9 January 2014
How to float a ping pong ball on air - The Coandă Effect
Widely explained using the Bernoulli principle, this phenomenon is actually dominated by the Coanda effect.
Libellés :
Coanda Effect,
Fluids and Thermodynamics,
Physics Girl
Wednesday, 8 January 2014
ScienceCasts: Starting Fire in Water
Astronauts on the ISS are experimenting with a form of water that has a strange property: it can help start fire. This fundamental physics investigation could have down-to-Earth benefits such as clean-burning municipal waste disposal and improved saltwater purification.
Libellés :
Chemistry,
Fluids and Thermodynamics,
NASA
Thursday, 5 December 2013
Hewitt-Drew-it! 81. Thermodynamics
The three laws of thermodynamics are cited and explained.
Libellés :
Fluids and Thermodynamics,
Hewitt-Drew-it,
Thermodynamics
Wednesday, 4 December 2013
Hewitt-Drew-it! 79. Energy of Phase Changes
The roles of heat of fusion, and vaporization, in changes in phase.
Libellés :
Energy,
Fluids and Thermodynamics,
Hewitt-Drew-it,
Thermodynamics
Tuesday, 3 December 2013
Hewitt-Drew-it! 75. Heat Transfer
Conduction, convection, and radiation.
Libellés :
Fluids and Thermodynamics,
Heat,
Hewitt-Drew-it
Tuesday, 26 November 2013
Hewitt-Drew-it! 80. More on Phase Changes
Phase changes are explained and expressed in equation form.
Libellés :
Fluids and Thermodynamics,
Hewitt-Drew-it
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