Atomic emission spectroscopy involves converting a sample into excited gaseous atoms and ions that emit light at characteristic wavelengths. The sample is identified by its emission wavelengths and concentration is determined from emission intensity. Samples can be excited by high temperatures from flames or plasmas. Emission lines are analyzed using monochromators and detected using photomultiplier tubes. An internal standard method is often used to compensate for fluctuations in emission intensity. Common excitation sources include flames, plasma torches, and electrical arcs or sparks.