Light Source Spectrum Data

Full spectrum typically refers to the completeness of a light source s spectral energy particularly when compared to natural light sources such as natural daylight.

Light source spectrum data.

The sun is the most obvious. Relative spectral power distributions spds of cie illuminants a b and c from 380 nm to 780 nm. A standard illuminant is a theoretical source of visible light with a profile its spectral power distribution which is published. For example the sun and other stars are sources of white light.

This light is given different names depending on its wavelength and energy radio waves long wavelength low energy microwaves infrared visible light ultraviolet x rays and gamma rays short wavelength high energy. About light most objects in space give off radiate light. The wavelengths that humans are typically able to visualize lie in a very narrow range between approximately 400 and 700 nanometers. Click once on the name of a spectrum in the data input section to preview the spectrum in the plotting window in light gray.

The 175w xe light source xe spectrum is a compact and light weight high intensity light source. The emission spectrum for natural light generally follows the planck distribution in the visible part of the spectrum as we can see below. No color is dramatically favored over another although the intensity is highest in the light blue region around 460 nm. The emission spectrum of visible light arriving at the earth s surface from the sun.

It is especially suitable as a light source for spectroscopy microscopy optical scanning and industrial uses as well as for use with sp s popular digikröm monochromators and spectrographs. The exact spectral composition of a light source can only be determined by specialized photometric equipment such as a spectrometer. Visible light comprises only a tiny fraction of the entire electromagnetic radiation spectrum yet it contains the only region of frequencies to which the rods and cones of the human eye will respond.