an emission spectrum that consists of a continuum of wavelengths.
The Sun spectra is considered continuous.
A continuous spectrum is seen in a rainbow.
Two common sources of continuous spectra used in emission spectroscopy are the electrical discharge lamps and the incandescent lamps. Electrical discharge lamps, such as the mercury vapor lamps, produce continuous spectra due to the excitation of atoms or molecules in the gas discharge. Incandescent lamps, on the other hand, produce continuous spectra because of the thermal emission from the hot filament.
Discontinuous Spectra, Fraunhofer lines
Continuous spectra of light are formed by all forms of white light. This includes light produced by common light bulbs like incandescent and fluorescents.
Paul Francis Buerger has written: 'Theoretical continuous and line spectra of stars in a close binary system' -- subject(s): Astronomical spectroscopy, Spectra, Double stars
You can use spectra to estimate the temperature of the star: astronomical thermometer
Yes, it is possible to use emission line spectra to determine the presence of metallic ions in the sun. Solids, liquids, and dense gases emit light of all wavelengths, without any gaps. We call this a continuous spectrum
characteristick x-ray are those which is emmited by the electron of target atom due to transition from higher energy state to lower energy state,while continuous x-ray are those which is emmited by the atoms present in a material.
Exponential Averaging - Generates a continuous running average where the most recently sampled spectra have more influence on the average than older ones. This provides a convenient form to examine changing data with the benefit of some averaging to smooth the spectra. The Vibration A to Z on the VibroNurse Website
There are three main types of infrared spectra: absorption spectra, emission spectra, and reflection spectra. Absorption spectra are produced when a material absorbs infrared energy, emission spectra are produced when a material emits infrared radiation, and reflection spectra result from the reflection of infrared radiation off a material.
There is no code for spectra