Emission transitions in the Paschen series end at orbit n = 3 and start from orbit n and can be represented as v = 3.29 × 1015 (Hz) [1/32 – 1/n2]
Calculate the value of n if the transition is observed at 1285 nm. Find the region of the spectrum.
V = c/λ = 3x108/1285x10-9
= 3.29 x 1015(1/32 – 1/n2)
= 1/n2 = 1/9 - 3x108/1285x10-9 x (1 / 3.29 x 1015)
= 0.111- 0.071 = 0.04 or 1/25
Or
n2 = 25,
n= 5
The spectrum lies in the infra-red region.
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(d) n = 4; l =3.
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(iii) used to determine pressure volume work
(iv) whose value depends on temperature only.
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