DocumentCode
3376914
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
fYear
2013
fDate
23-28 June 2013
Firstpage
492
Lastpage
494
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;
fLanguage
English
Publisher
ieee
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
Type
conf
DOI
10.1109/MSMW.2013.6622110
Filename
6622110
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