Title :
New measurements of Rydberg spectrum of singlet Mg I in the 120–150 GHz frequency range
Author :
Kutsenko, A.S. ; Pogrebnyak, N.L. ; Dyubko, S.F.
Author_Institution :
Inst. of Radio Astron., Kharkov, Ukraine
Abstract :
Several dozens of Rydberg recombination lines of Mg I were detected in emission spectrum of the Sun [1]. The lines were observed in far infrared and were assigned to the transitions between n = 5 - 8 and L <; 8 states but the assignment was tentative. This inspired a number of works on microwave spectroscopy of states with high L. In laboratory conditions Lyon et al. [2] observed and measured frequencies of Rydberg microwave transitions of Mg I for n = 17 - 23 between f-,g-,h-,i- states also determining dipole polarizability of Mg+. Snow et al. [3] for n = 17 measured transition frequencies between 6 ≤ L ≤ 11 states. There was a number of spectroscopic investigations of Mg in optic range published after analysis of Mg I spectrum performed by Martin and Zalubas for NIST database in 1980 [4]. Beigang and Schmidt performed an optic spectroscopic investigation of D state of Mg I for principal quantum number n range from 15 to 43 [5]. In the works of Ficher [6] and Lu [7] it was found that 3snd1D2 term is highly perturbed by doubly excited configuration 3p21D23. The largest interaction is observed for n = 3 and the perturbation decreases with increase of principal quantum number. Using methods of high precision infrared laser spectroscopy Lemoine et al. have recorded 23 Rydberg transitions of Mg I in the infrared range 740 ÷ 1126 cm-1 [8]. It was found that fine structure of f-states with n = 5 - 7 is inverted. In addition this work as well as the calculations performed in [1] gave an opportunity to explain some previously unassigned lines in the Sun emission. Beigang et al. [9] have undertaken investigation of Rydberg F state of Mg using method of Doppler free laser spectroscopy that resulted in determination of isotopic shifts, magnitude of singlet-triplet splitting and hyperfine structure splitting of 25Mg isotope in the range of principal quantum number n= 14-84. In this ra- ge of principal quantum number the inversion of the fine structure was not observed anymore. Rafiq et al. [10] have determined quantum defects for S,P,D and F states measuring in the course of optic range investigation also the energies of S, P, D, F terms up to n = 24,61,62,66 respectively. Nevertheless the calculations of microwave transition frequencies using results from [10] and comparison with our experimental results reveals differences up to several GHz. Aim of our work is to obtain reliable accurate data on microwave Rydberg spectra of Mg I.
Keywords :
Sun; infrared spectroscopy; luminescence; polarisability; quantum theory; solar radiation; Doppler free laser spectroscopy; NIST database; Rydberg F state; Rydberg microwave transitions; Rydberg recombination lines; Rydberg spectrum; Sun emission; dipole polarizability; emission spectrum; far infrared; frequency 120 GHz to 150 GHz; high precision infrared laser spectroscopy; hyperfine structure splitting; microwave Rydberg spectra; microwave spectroscopy; microwave transition frequencies; optic spectroscopic investigation; principal quantum number; singlet Mg I; singlet-triplet splitting; Atom optics; Frequency measurement; Laser excitation; Microwave measurement; Physics; Pump lasers; Resonant frequency;
Conference_Titel :
Physics and Engineering of Microwaves, Millimeter and Submillimeter Waves (MSMW), 2013 International Kharkov Symposium on
Conference_Location :
Kharkiv
Print_ISBN :
978-1-4799-1066-3
DOI :
10.1109/MSMW.2013.6622110