Talk:Atomic emission spectrum

This redirect is within the scope of WikiProject Physics, a collaborative effort to improve the coverage of Physics on Wikipedia. If you would like to participate, please visit the project page, where you can join the discussion and see a list of open tasks.PhysicsWikipedia:WikiProject PhysicsTemplate:WikiProject Physicsphysics articles

Spectroscopy (inactive)

This redirect is within the scope of WikiProject Spectroscopy, a project which is currently considered to be inactive.SpectroscopyWikipedia:WikiProject SpectroscopyTemplate:WikiProject SpectroscopySpectroscopy articles

A new spectral line intensity formula for optical emission spectroscopy was presented by Dr:s Bo Thelin (experimental physicist) and Sten Yngström (theoretical physicist) at the beginning of the 1980:s. This formula has shown very good agreement between experiments (ref 1) and the new theory (ref 2). These references are summaries of earlier papers.

I = K \ left (frac { v^2 }{ c^2 }\ right ) \ e^left (\ frac { -J}{ k \ T \ right )} \

\ left (\ e^left ( \ frac { h \ v }{ k \ T \right -  \ 1)^-1

K includes transition rates and element concentration,v=frequency,J=ionisation energy and T=temperature —Preceding unsigned comment added by 79.138.138.183 (talk) 00:32, 9 March 2008 (UTC)[reply]

--79.138.179.27 (talk) 21:16, 10 March 2008 (UTC)[reply]

Many independent experimental methods strongly support the new formula, while the standard intensity formula with the Boltzmann term (upper energy level), deviates very much from experiments. Ref 1 Yngström,S and Thelin,B (1990) Applied Spectroscopy ,44, 1566 Ref 2 Yngström,S International Journal of Theoretical Physics Vol. 33, No. 7, 1994 --79.138.179.27 (talk) 21:22, 10 March 2008 (UTC)79.138.179.27 (talk) 21:16, 10 March 2008 (UTC) —Preceding unsigned comment added by 79.138.135.97 (talk) 22:13, 8 March 2008 (UTC)[reply]