Laboratory measurement of the solar OH lines in the 10 μm region

✍ Scribed by B. Lemoine; M. Bogey; J.L. Destombes

• Publisher: Elsevier Science
• Year: 1985
• Tongue: English
• Weight: 498 KB
• Volume: 117
• Category: Article
• ISSN: 0009-2614
• DOI: 10.1016/0009-2614(85)80297-9

✦ Synopsis

Thirty-nine pure rotational uansitions of OH in u = 0 and u = 1 vlbrahonal smles have been observed in a laboratory glow discharge by uing n laser diode spectiometer. They have been interpreted within the framework of the Brown Hamil~onian The fir which includes also the u = C.l rmuowave spectra, Lhe u = 0.1 solar rolalional spectra and Lhe O-l vlbratron-rotation spectrum. leads to a set of parameters in good agreement wilh the parameters previously determined from a more restricted range of 1 values, demonstraling the validrty of the effective Hamilronian concept. Lines in quasi-coincidence with N,O and CO, laser bnes are also given.