1 nm = 1e-9m (1 times 10 to the power -9); the basic formula for wavelenght and frequency is: (speed of the wave) = (wavelength) x (frequency); therefore, since the speed of light is 300e6 m/s, the frequency is 300e6 / 400e-9 = 0.75e15 or 750e12 (750 trillion cycles per second).
the frequency of any light can be calculated by the distance that light travles divided by its wavelength in the same unit, in this case, it is
299792458 m/s / 0.00000004m = 7494811450000000 Hz
The frequency of 435nm is f= c/w = 3e8/436e-9 = 6.88e14 hertz.
c = lambda x nu3x10^8 m/sec = 436x10^-9 m x nu
nu = frequency = 3x10^8 ms^-1/4.36x10^-7 m = 6.88 s^14 Hz
687.59738 Thz
731.7 Terahertz= 300M/.410u
6.9x10^14
blue
Neon signs give off a characteristic bright red to reddish-orange light. Other colors are created by using argon and mercury, and coating the inside of the tube with phosphors that emit the desired color when ionized. The mercury ionizes and emits ultraviolet (UV) radiation. The UV light slams into the phosphor coating, and the phosphor emits light. The color of that light will be determined by the composition of the phosphor coating.
Solar radiation mostly passes through the atmosphere without heating it, due to its wavelength. It does not pass through the ground, however, and it heats the ground. The ground emits radiation at a wavelength dependent on its temperature. This radiation happens to be in the thermal infrared part of the spectrum, or in other words, sensible heat. Therefore, the atmosphere is heated by the surface, whereupon the heat tends to rise and heat the lower atmosphere.
It emits Beta radiation.
according to the wave theory of light,we have the relation that wavelength is inversely proportional to the frequency,therefore the electromagnetic wave with the lower wavelength will have higher frequency..
radiation
The Sun emits most of its radiation in a wavelength band between 0.1 and 4.0 micrometers (µm).
just had this on a test, the answer is Temperature
A low temp source emits low-frequency, long wavelength waves. A medium temp source emits medium frequency, medium wavelength waves. A high temp source emits high frequency, short wavelength waves.
The temperature of the radiating body determines the intensity and characteristics of the radiation it emits. Two electromagnetic radiation principles describe the relationship between a radiating body�s temperature and the radiation it emits. 1. Stefan-Boltzmann�s Law: Hotter objects emit more total energy per unit area than colder objects. 2. Wein�s Displacement Law: The hotter the radiating body, the shorter the wavelength of maximum radiation.
...because the colour of an object depends on the wavelength of light it reflects, or the wavelength of light it emits.
The Sun emits infrared radiation, as well as a broad spectrum of other rays of electromagnetic radiation. It is the infrared band, that just beyond (and just longer in wavelength) what we see as the color red, which reacts with matter to increase its temperature. Infrared from sunlight heats the Earth's surface and atmosphere.
Neon signs give off a characteristic bright red to reddish-orange light. Other colors are created by using argon and mercury, and coating the inside of the tube with phosphors that emit the desired color when ionized. The mercury ionizes and emits ultraviolet (UV) radiation. The UV light slams into the phosphor coating, and the phosphor emits light. The color of that light will be determined by the composition of the phosphor coating.
The colder a star is the longer the light waves it emits. Light wavelength is what we perceive as color.
The Sun emits radiation in all parts of the Electromagnetic Spectrum. However, the strongest intensity radiation is at wavelength of around 450 nanometers. This is in the visible region.
The Earth emits infrared radiation at greatest intensity
The sun emits its greatest intensity of radiation in a spectral region. The spectral region the sun's radiation emits to is the visible region of the spectrum.
You're probably thinking of frequency and wavelength. If that's true, then you onlyneed one or the other. They're tightly connected, so if you know one of them, thenyou can always calculate the other one.