Article
Plasma Investigations
2017. V. 55. № 2. P. 165–173
Atrazhev V.M., Shakhatov V.A., Boltnev R.E., Bonifaci N., Aitken F., Eloranta J.
Spectra, line intensities of the C1Σ+g→A1Σ+u and the c3Σ+g→a3Σ+u transitions in liquid normal He, and rotational level populations of the C1Σ+u and the c3Σ+u terms
Annotation
We observed the rotational spectral lines of the excimer within the range of 910–930 nm in the corona discharge in normal liquid He at the temperature of 4.2 K and the pressure of 1 atm. The spectral range is filled with the rotational lines of the C1Σ+g→A1Σ+u singlet and the c3Σ+g→a3Σ+u triplet transitions. These transitions end at the rotational levels of the lowest metastable terms, A1Σ+u и a3Σ+u and of the excimer. Then, the population of the rotational levels with the K′ number of the upper C1Σ+u and c3Σ+u terms (the quantity of the molecules with the rotational moment of K′ in the excited molecule ensemble in the discharge) is proportional to the intensity of the rotational lines marked K′ of the C1Σ+g→A1Σ+u singlet and the c3Σ+g→a3Σ+u triplet. The populations might be calculated according to the experimental intensities of the rotational spectral lines. The emitting corona plasma in the liquid He is nonequilibrium and the rotational level populations do not correspond to the Boltzmann distribution. The efficient rotational temperature exceeds the liquid He temperature, 4.2 K.
Article reference:
Atrazhev V.M., Shakhatov V.A., Boltnev R.E., Bonifaci N., Aitken F., Eloranta J. Spectra, line intensities of the C1Σ+g→A1Σ+u and the c3Σ+g→a3Σ+u transitions in liquid normal He, and rotational level populations of the C1Σ+u and the c3Σ+u terms, High Temp., 2017. V. 55. № 2. P. 165
Atrazhev V.M., Shakhatov V.A., Boltnev R.E., Bonifaci N., Aitken F., Eloranta J. Spectra, line intensities of the C1Σ+g→A1Σ+u and the c3Σ+g→a3Σ+u transitions in liquid normal He, and rotational level populations of the C1Σ+u and the c3Σ+u terms, High Temp., 2017. V. 55. № 2. P. 165