Pfund series

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:

• 6 -> 5: 7460 nm
• 7 -> 5: 4654 nm
• 8 -> 5: 3741 nm
• 9 -> 5: 3297 nm
• 10 -> 5: 3039 nm
• ...
• infinity -> 5: 2279 nm

Formula for the wavelengths:

1/wavelength = RH ( 1/25 - 1/n² )

• wavelength is the wavelength within the Pfund series.
• R_H is the Rydberg constant for hydrogen, 1.0973731568160 × 10⁷m^-1 ≈ 13.6⁠eV / (hc)
• n is the higher electron shell number.
• h - Planck constant.
• c - speed of light in a vacuum.