2004
DOI: 10.1021/jp049718h
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Photodissociation Rate Constants for VUV Processes of CF3Cl and CF2Cl2 in the Upper Atmosphere. A MQDO Study

Abstract: The availability of data concerning the upper atmosphere is essential for an understanding of both the change in solar activity and the different processes that have direct effects on the biosphere, in particular, those with harmful environmental consequences. The main goal of the present work is the theoretical analysis of the photodissociation of two chlorofluorocarbon (CFC) compounds that play an important role in the chemical and energetic balance of the upper atmosphere, CF3Cl and CF2Cl2. Given that the m… Show more

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Cited by 8 publications
(4 citation statements)
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“…8 Although a large percentage of these molecules photodissociate in the stratosphere via this low-lying channel, the surviving molecules can reach the ionosphere, where vacuum UV (VUV) opens new dissociation channels after excitation into higher states. 9 Moreover, because some of these high excitations have large transition moments, 10,11 the action spectrum is shifted to high energies, making them specially relevant from the photochemical point of view.…”
Section: ■ Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…8 Although a large percentage of these molecules photodissociate in the stratosphere via this low-lying channel, the surviving molecules can reach the ionosphere, where vacuum UV (VUV) opens new dissociation channels after excitation into higher states. 9 Moreover, because some of these high excitations have large transition moments, 10,11 the action spectrum is shifted to high energies, making them specially relevant from the photochemical point of view.…”
Section: ■ Introductionmentioning
confidence: 99%
“…The lowest photodissociation channel of clorofluorcarbons (CFCs) and halocarbons usually involves excitations from chlorine lone pairs ( n ) into C–Cl antibonding (σ*) orbitals induced by UVB or low UVC radiation . Although a large percentage of these molecules photodissociate in the stratosphere via this low-lying channel, the surviving molecules can reach the ionosphere, where vacuum UV (VUV) opens new dissociation channels after excitation into higher states . Moreover, because some of these high excitations have large transition moments, , the action spectrum is shifted to high energies, making them specially relevant from the photochemical point of view.…”
Section: Introductionmentioning
confidence: 99%
“…7 Although a large percentage of these molecules photodissociate while in the stratosphere, the surviving molecules can reach the ionosphere, where vacuum UV (VUV) is present, and in this case the Rydberg states play a very important role. 8 Thus, a detailed knowledge of its excited states is of fundamental importance to understand its photochemistry.…”
Section: Introductionmentioning
confidence: 99%
“…[10] The theoretical tool employed in the calculation of the photoabsorption cross sections has been the Molecular Orbital Quantum Defect (MQDO) approach, formulated within our group a decade ago [Martı ´n et al, 1996a]. This methodology has proved, in a number of works [Velasco et al, 2003a[Velasco et al, , 2003bMayor et al, 2004Mayor et al, , 2005aBustos et al, 2004], to yield quantitative intensities for electronic transitions involving one or two Rydberg states. Very recently, rotational resolution has been accurately introduced in the procedure [Mayor et al, 2005b].…”
Section: Introductionmentioning
confidence: 99%