Pregled bibliografske jedinice broj: 10376
Satellite Bands In The Quasi-Static Wings Of Tl And In Resonance Lines Broadened By Hg
Satellite Bands In The Quasi-Static Wings Of Tl And In Resonance Lines Broadened By Hg // Fizika A : a journal of experimental and theoretical physics : atomic and molecular physics, condensed matter physics, plasma physics, 5 (1996), 1; 1-10 (podatak o recenziji nije dostupan, članak, znanstveni)
CROSBI ID: 10376 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Satellite Bands In The Quasi-Static Wings Of Tl And In Resonance Lines Broadened By Hg
Autori
Henč-Bartolić, Višnja ; Pichler, Goran
Izvornik
Fizika A : a journal of experimental and theoretical physics : atomic and molecular physics, condensed matter physics, plasma physics (1330-0008) 5
(1996), 1;
1-10
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
satellite bands; quasi-static wings; tl; in; resonance lines
Sažetak
Using a high pressure metal-halide discharge lamps, we have measured the spectral positions of the satellite bands in the wings of Tl 535 nm and 377.6 nm, and In 451.1 nm and 410.2 nm resonance lines. The satellite bands in the red wings are attributed to the TlHg or InHg excimers, and those appearing in the near blue wings to the Tl2, and In2 molecules. Using the Abel inversion procedure, we obtained the relevant spatial temperature and spectral intensities distributions, from which we have concluded that the red satellite bands are due to the bound portion of the TlHg or InHg excited potential curves.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
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