Diffusion of CO and CH molecules in the solar atmosphere

dc.contributor.author	Sinha, K.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2011-12-27T04:28:42Z
dc.date.available	2011-12-27T04:28:42Z
dc.date.issued	1973
dc.identifier.uri	http://hdl.handle.net/123456789/885
dc.description.abstract	The calculated rates of photodissoication, radiative association and the diffusion of CH and CO molecules show that the diffusion rates are many orders of magnitude smaller than the photodissociation and radiative association rates, both in the photosphere and spots. Moreover, the diffusion velocities are much smaller than the turbulence velocities in the photosphere and spots. Thus, the diffusion of diatomic molecules ( with dissociation energies in the range 3.47eV to 11·01eV) is not possible in the solar atmosphere.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	bac24-334
dc.subject	Solar Atmosphere	en_US
dc.title	Diffusion of CO and CH molecules in the solar atmosphere	en_US
dc.type	Article	en_US