Astrophysics (Index)About

Pfund series

(hydrogen lines for electrons settling from n > 5 to n = 5)

The Pfund series is the set of emission lines from atomic hydrogen gas, due to electrons descending from an electron shell of number n greater than 5 down to that of n = 5, or the analogous absorption lines when absorbed electromagnetic radiation (EMR) makes electrons do the opposite. It is one of the hydrogen line series, such as the Lyman series and Balmer series, and is named after August Herman Pfund. The lines are within infrared and some are within atmospheric windows, so given no redshift, some of the lines in astronomical sources may be viewed from ground telescopes while others are blocked. Lines:

Formula for the wavelengths:

1/wavelength = RH ( 1/25 - 1/n² )

(hydrogen,line series,lines,spectrum)
Further reading:
https://en.wikipedia.org/wiki/Hydrogen_spectral_series
http://hyperphysics.phy-astr.gsu.edu/hbase/Tables/hydspec.html
https://www.chemeurope.com/en/encyclopedia/Pfund_series.html
https://www.nist.gov/system/files/documents/srd/jpcrd382009565p.pdf
WaveLFreqPhoton
Energy
  
2279nm132THz544meVbeginPfund series
7460nm40THz166meVendPfund series

Referenced by pages:
hydrogen (H)
spectral line

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