Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...178..277s&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 178, no. 1-2, May 1987, p. 277-282.
Astronomy and Astrophysics
Astrophysics
11
Comets, Free Radicals, Gas Dissociation, Imides, Photodissociation, Life (Durability), Radial Velocity, Velocity Distribution, Comets, Photodissociation, Nh Radical, Solar Radiation, Calculations, Velocity, Distance, Parent Molecules, Nitrogen, Hydrogen, Bennett, Ammonia, Distribution
Scientific paper
The authors present photodissociation rates of NH by absorption of solar radiation into the υarcmin = 2 level of the A3Πi state as a function of radial velocity for a comet at a heliocentric distance of 1 AU. The photodissociation of NH results in velocity distributions of about 1 km s-1 and 15 km s-1 for nitrogen and hydrogen atoms, respectively, with respect to NH. By comparing the convolution model lifetime of the NH parent for comet Bennett (1970 II) with the photochemical lifetime of NH3 against solar photon flux at 1 AU the authors infer that NH3 is probably the parent of NH radical observed in comets.
Gruenwald Ruth B.
Singh Patan D.
No associations
LandOfFree
The photodissociation lifetimes of the NH radical in comets does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The photodissociation lifetimes of the NH radical in comets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The photodissociation lifetimes of the NH radical in comets will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-856247