The Sun spectra is considered continuous.
A continuous spectrum is seen in a rainbow.
The best place for information on the Polaroid Spectra cameras is camerapedia.org.
NOESY spectra provide information on through-space interactions between protons, showing correlations between protons that are close in space. NOE difference spectra compare two spectra to highlight differences in nuclear Overhauser effect (NOE) intensities between two conditions, such as before and after a perturbation, revealing changes in molecular structure or dynamics.
They have different packaged particles.
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.
an emission spectrum that consists of a continuum of wavelengths.
Different elements have different line spectra because each has a unique arrangement of energy levels for its electrons. When electrons transition between these energy levels, they emit or absorb specific wavelengths of light, creating distinct lines in the spectrum. This results in discrete lines rather than a continuous spectrum.
Well... that sort of depends on the viewer whether they liked the new vestroia spectra phantom or the mechtanium surge spectra phantom. The only difference between the two is that spectra changes clothing, from red to black and purple. His helios is a different story.
Continuous spectra of light are formed by all forms of white light. This includes light produced by common light bulbs like incandescent and fluorescents.
A continuous spectrum of a star is a broad range of electromagnetic radiation emitted across all wavelengths. It results from the thermal energy of the star's interior, causing atoms to vibrate and emit photons at various energies. Continuous spectra can be used to determine a star's temperature.
Paul Francis Buerger has written: 'Theoretical continuous and line spectra of stars in a close binary system' -- subject(s): Astronomical spectroscopy, Spectra, Double stars