摘要
We observed the spectra within the wavelength range of 910-990 nm of emission of the corona discharge in supercritical helium gas at 6-11 K. This spectral range contains the molecular bands of the He*(2) excimer radiative transitions (c I-3 pound (g) (+) ac' a I-3 pound (u) (+) ) between the electron-vibrational-rotational levels of the c I-3 pound (g) (+) and the a I-3 pound (u) (+) triplet states. We have determined the populations of the rotational levels (quantity of molecules in the given excited state among the excited molecules of the discharge) of the c I-3 pound (g) (+) excited state from experimental values of the intensity of the respective electron-vibrational-rotational lines. The calculated population distribution is nonmonotonous. The population of the level with the rotation quantum number K' = 18 (the level number) is higher than those of the levels with the other K' values.
- 出版日期2017-5