Wiki User
∙ 13y ago3.125 x 10 ^ 13
Wiki User
∙ 13y agoTo calculate the frequency of radiation with a wavelength of 9.6 μm, you can use the equation v = c/λ, where v is the frequency, c is the speed of light (3.00 x 10^8 m/s), and λ is the wavelength in meters. First, convert 9.6 μm to meters (1 μm = 1 x 10^-6 m), then plug the values into the equation to find the frequency in s^-1. The frequency corresponding to a wavelength of 9.6 μm is approximately 3.125 x 10^13 s^-1.
The Earth's atmosphere absorbs different amounts of radiation depending on the wavelength. It absorbs most of the sun's harmful ultraviolet radiation and some infrared radiation, helping to regulate the Earth's temperature. Overall, the atmosphere acts as a protective shield, allowing only a small portion of harmful radiation to reach the Earth's surface.
A perfect absorber or emitter of radiation is called a blackbody. It absorbs all incident radiation regardless of wavelength or direction, and emits radiation at the maximum possible level for a given temperature.
If the gamma rays and X-rays have the same frequency, the electron will have the same energy regardless of which type of radiation is interacting with it. The energy of the electron is determined by the frequency of the radiation it absorbs, not the type of radiation.
The upper atmosphere absorbs harmful ultraviolet (UV) radiation from the sun. This absorption occurs mainly in the ozone layer, which absorbs UVB and UVC wavelengths. Absorption of these wavelengths protects life on Earth from the damaging effects of excessive UV radiation.
It has different wavelengths
When matter absorbs a photon, the energy of the matter increases by an amount equal to the energy of the absorbed photon. The frequency and wavelength of the absorbed radiation depend on the energy of the photon and are inversely related - higher energy photons have higher frequencies and shorter wavelengths.
The wavelength of 275 nm is used to measure absorbance of caffeine because it corresponds to the maximum absorbance peak for caffeine. By using a wavelength where caffeine absorbs strongly, we can accurately measure its concentration in a sample based on the amount of light absorbed at 275 nm.
The Earth's atmosphere absorbs different amounts of radiation depending on the wavelength. It absorbs most of the sun's harmful ultraviolet radiation and some infrared radiation, helping to regulate the Earth's temperature. Overall, the atmosphere acts as a protective shield, allowing only a small portion of harmful radiation to reach the Earth's surface.
A perfect absorber or emitter of radiation is called a blackbody. It absorbs all incident radiation regardless of wavelength or direction, and emits radiation at the maximum possible level for a given temperature.
Absorption spectroscopy refers to spectroscopic techniques that measure the absorption of radiation, as a function of frequency or wavelength, due to its interaction with a sample. The sample absorbs energy, i.e., photons, from the radiating field. The intensity of the absorption varies as a function of frequency, and this variation is the absorption spectrum. Absorption spectroscopy is performed across the electromagnetic spectrum.
The Earth emits longer wavelength infrared radiation because it absorbs sunlight and re-radiates it as heat. The Sun, on the other hand, emits shorter wavelength radiation in the form of visible light because it is much hotter than the Earth.
The color of an object is the frequency/wavelength of the light it reflects. The light it reflects is the light it receives minus the light it absorbs.
Ozone is the substance present in the atmosphere that absorbs solar radiation with a wavelength less than 242 nm. This absorption helps protect living organisms from the harmful effects of ultraviolet radiation.
The wavelength of maximum absorbance corresponds to the color of a substance because it denotes the specific wavelength of light that the substance absorbs most strongly. This wavelength is complementary to the color that the substance appears, meaning that if a substance absorbs light most strongly at a certain wavelength (such as red light), it will appear as the complementary color (in this case, green).
A wave with a high frequency has a low wavelength. Wavelength lambda and frequency f are connected by the speed cof the medium. c can be air = 343 m/s at 20 degrees celsius or water at 0 dgrees = 1450 m/s. c can be light waves or electromagnetic waves = 299 792 458 m/s. The formulas are: c = lambda x f f = c / lambda lambda = c / f
Molecular fluoroscene often occurs at a longer wavelength than the exciting radiation due to energy loss during the fluorescence process. When a fluorophore absorbs energy and transitions to an excited state, it releases this energy as fluorescence emission, typically at a longer wavelength than the excitation wavelength. This phenomenon is known as the Stokes shift.
The upper atmosphere absorbs harmful ultraviolet (UV) radiation from the sun. This absorption occurs mainly in the ozone layer, which absorbs UVB and UVC wavelengths. Absorption of these wavelengths protects life on Earth from the damaging effects of excessive UV radiation.