GAS-PHASE SPECTRA OF RADIATIVE RECOMBINATION OF NITROGEN-ATOMS AT HELIUM TEMPERATURES Academic Article

abstract

• The lowering of temperature from 300 K to 10 K caused drastic changes in the spectral composition of the recombinational afterglow of N atoms: the glow due to the B3g | A 3+u transition with = 12-9 ( 580 nm and 540 nm) disappeared whereas levels with = 8-5 ( 560 nm) appeared. This effect is exlained in terms of Campbell and Thrush's recombination luminescence model (emitting B 3Hg state populated by radiationless transition from the lower A 3+u state of the N2 molecule). 1978.

authors

• Khmelenko, Vladimir

published proceedings

• CHEMICAL PHYSICS LETTERS

author list (cited authors)

• GORDON, E. B., MEZHOVDEGLIN, L. P., PUGACHEV, O. F., & KHMELENKO, V. V.

citation count

• 16

complete list of authors

• GORDON, EB||MEZHOVDEGLIN, LP||PUGACHEV, OF||KHMELENKO, VV

publication date

• January 1978

publisher

• Elsevier  Publisher

published in

• CHEMICAL PHYSICS LETTERS  Journal

Digital Object Identifier (DOI)

• 10.1016/0009-2614(78)80101-8

start page

• 282

end page

• 285

volume

• 54

issue

• 2

URL

• http://dx.doi.org/10.1016/0009-2614(78)80101-8