2. The entire range of different types of electromagnetic waves, extending from the very long, low-frequency radio waves, through infrared and light waves, to the very short, high-frequency cosmic rays and X-rays which can be generated physically.
This range of electromagnetic wavelengths extends almost from zero to infinity and includes the visible portion of the spectrum known as light.
3. A list, chart, graph, or diagram showing the relationships among all known types or range of electromagnetic radiation including the range of frequencies and wavelengths.4. The total range of wavelengths, extending from the shortest to the longest wavelength or conversely, that can be generated physically.
This range of electromagnetic wavelengths extends practically from zero to infinity and includes the visible portion of the spectrum known as light.
2. A visual display, photograph, or graphical plot of the intensity of electrons emitted from a substance bombarded by X-rays or other radiation as a function of the kinetic energy of the electrons.
2. Bands of spectral lines connected with a change of electronic state of a molecule.
Each band is corresponding to vibrational energies in the initial and final conditions and each band consists of numerous rotational lines.
2. A spectrum resulting from the emission of electromagnetic radiation by ions, atoms, and molecules following excitations of their electrons.
2. The spectrum resulting from emission or absorption of electromagnetic radiation during changes in the electron configuration of atoms, ions, or molecules, as opposed to vibrational, rotational, fine-structure, or hyperfine spectra.
With metal electrodes, a spectrum of the metallic vapor is obtained.
2. The splitting up of electromagnetic radiations into the constituent wavelengths.
Atoms can exist in a number of discreet energy levels and they emit or absorb photons when they make transitions from one level to another.
The energies of the photons emitted or absorbed by one atom are different from those of all of the other atoms.
The photon energies are directly related to their frequencies, which set their colors in the spectrum, so by observing the colors of the photons, it is possible to determine which atoms are being observed.
This can be done in a laboratory, and it can also be done with the light reaching us from stars, near or distant, which enables us to identify the atoms that stars are made of.
The result is a series of dark bands crossing the spectrum, known as absorption lines.
2. The range of wavelengths, or frequencies, over which electromagnetic radiation is propagated.
The longest wavelengths, or lowest frequencies, are those of radio waves, and the shortest wavelengths are those of gamma rays.