80 HZ is the frequency of a wave varying at 80 times per second.
It could be an acoustic wave (sound), or an electromagnetic wave. (radio or power line)
300 / 80 = 3.75 metres.
There are 1000 milliamperes in one ampere. Therefore, 800 milliamperes is equal to 800/1000 = 0.8 amperes.
800 feet = 0.1515 miles
800 meters is just under 1/2 of a mile.
A milligram of salt looks like a tiny white heap. You might get 5,000 such heaps into a teaspoons.
There are 25.4 mm in one inch. 800 mm divided by 25.4 mm/in is 31.49 inches. Direct Conversion Formula800 mm*1 in 25.4 mm=31.49606299 in
2240ms-1
Wavelength = (speed of light) divided by (frequency).In free space, wavelength = (3 x 108) / (800 x 106) = 0.375 meterNote that 800 MHz is in the same general frequency range as many cellular telephone systems.
The wavelength is .8 microns or 800 nanometers.
It is an electromagnetic wave, which means it is similar to light, but invisible to the human eye. Infrared light (or infrared waves) have a longer wavelength and a smaller frequency than visible light.
Everything outside of about 400-800 nm i.e. Radio mirco wave infrared ultraviolet x-ray gamma ray
Light and other electromagnetic waves do indeed travel as a wave. For that reason, light, radio waves and all other electromagnetic waves can be characterized by a wavelength. Different colors of light have different wavelengths in the range of around 400 nanometers to 800 nanometers. However, they can also be considered to be particles instead of waves. In some branches of physics, the concept of light as a particle can be very useful. For most of us, treating light as a wave is quite sufficient.
Radio Shack has an "800" number : 1-800-843-7422 .
600/cm to 800/cm
No. The higher the frequency of a wave, the higher the energy.
AM 800 CKLW radio station is known as 'The Information Station'. This station can be found on the AM radio dial as well as online. This station is located in Ontario, Canada.
Radio telescopes are much larger than optical telescopes because of wavelength. Earth's atmosphere has two major "windows" where it is transparent to photons: 300 nm - 800 nm: optical wavelength window (approximate) 30 mm - 30 m: radio wavelength window (approximate) Even the shortest-wavelengths used by radio telescopes at around 30 mm are still thousands of times longer than the longest wavelengths used by optical telescopes. The wavelength has 2 effects on the size of a telescope: * The angular resolution (in order to distinguish 2 nearby stars, FWHM) depends on the wavelength/aperture ratio. Radio-frequency photons require a wider aperture to focus than visible-light-frequency photons, so radio telescopes *must* be larger to get a reasonable resolution. * A telescope typically requires the collecting area to be aligned within 1/10 of the wavelength it is designed for. Because it is almost impossible to get all the parts of a sufficiently large telescope aligned to within 80 nm, radio telescopes *can* be built much larger.
800 kmh