Strong Lines of Carbon ( C ) - NIST
Carbon (C) Strong Lines of Carbon ( C ) Intensity : Vacuum Wavelength (Å) Spectrum : Reference : 600 P: 687.0526
Spectral line - Wikipedia
A spectral line is a weaker or stronger region in an otherwise uniform and continuous spectrum. It may result from emission or absorption of light in a narrow frequency range, compared with the nearby frequencies. Spectral lines are often used to identify atoms and molecules.
NIST: Atomic Spectra Database - Spectral Lines Help File
List of spectra of neutral, singly-ionized, and doubly-ionized elements between carbon and oxygen.
Chapter 7 Spectral Lines - National Radio Astronomy Observatory
Spectral lines are narrow (Δ ν ≪ ν) emission or absorption features in the spectra of gaseous and ionized sources. Examples of radio spectral lines include recombination lines of ionized hydrogen and heavier atoms, rotational lines of polar molecules such as carbon monoxide (CO), and the λ = 21 cm hyperfine line of interstellar H i .
NIST Atomic Spectra Database Lines Form
Values like '1' or '1P' are allowed to select only specific groups of terms. Selecting this option would generate spectral lines distribution for one or several ions. All lines within a specific ion stage are given the same intensity in order to indicate their positions. The links to the plots will be provided below the final line output.
The Emission Spectra of Various Atoms - Ohio State University
Representative Visible-Light Emission-Line Spectra of Various Chemical Elements ... Carbon (6 electrons) Nitrogen (7 electrons) Oxygen (8 electrons) Neon (10 electrons) Argon (18 electrons) Iron (26 electrons) Krypton (36 electrons) Xenon (54 electrons) Mercury (80 electrons) Data to create these graphs is from the NIST Atomic Spectra Database.
Element Carbon - AtomTrace
The three atomic emission spectra for Carbon can be shown on graph bellow: NIST Atomic Spectra Database [1], gfall.dat file from Kurucz CD-ROM No. 23 [2] and AtomTrace database. Lines in the AtomTrace list were observed in the optical emission of laser induced plasmas, and the respective values of spectroscopic constants are taken from [1].
In this critical compilation, all experimental data on the spectrum of neutral carbon known to us were methodically evaluated and supplemented by parametric calculations with Cowan’s codes.
Why spectral line -mode? First and foremost Science driven Spectral Line Science –This lecture and Wide -field imaging –Lecture on tuesday
Carbon dioxide (CO - University of Washington
Highly Sensitive Absorption Spectroscopy of Carbon Dioxide by ICLAS-VeCSEL Between 8800 and 9530 cm-1; Y. Ding, A. Campargue, E. Bertseva, S. Tashkun, and V.I. Perevalov; J.Mol.Spec. 231:117-123 (2005).