Js. Morrill et al., TIME-RESOLVED N-2 TRIPLET-STATE VIBRATIONAL POPULATIONS AND EMISSIONSASSOCIATED WITH RED SPRITES, Journal of atmospheric and solar-terrestrial physics, 60(7-9), 1998, pp. 811-829
The results of a quasi-electrostatic electron heating model were combi
ned with a time dependent N-2 vibrational level population model to si
mulate the spectral distributions and absolute intensities observed in
red sprites. The results include both N-2 excited state vibrational l
evel populations and time profiles of excited electronic state emissio
n. Due to the long atmospheric paths associated with red sprite observ
ations, atmospheric attenuation has a strong impact on the observed sp
ectrum. We present model results showing the effect of atmospheric att
enuation as a function of wavelength for various conditions relevant t
o sprite observations. in addition, our model results estimate the var
iation in the relative intensities of a number of specific Nz emission
s in sprites (1PG, 2PG, and VK) in response to changes in observationa
l geometry. A recent sprite spectrum, measured from the Wyoming Infrar
ed Observatory (WIRO) on Jelm Mountain, during July, 1996, has been an
alyzed and includes N-2 IPG bands down to v' = 1. In addition to N-2 1
PG, our analysis of this spectrum indicates the presence of spectral f
eatures which are attributable to N-2(+) Meinel emission. However, due
to the low intensity in the observed spectrum and experimental uncert
ainties, the presence of the N-2(+)(A(2)II(u)) should be considered pr
eliminary. The importance of both the populations of the lower levels
of the N-2((BIIg)-I-3) and the N-2((BIIg)-I-3)/N-2(+)(A(2)II(g)) popul
ation ratio in the diagnosis of the electron energies present in red s
prites is discussed. While the current spectral analysis yields a vibr
ational distribution of the N-2((BIIy)-I-3) which requires an average
electron energy of only 1-2 eV, model results do indicate that the pop
ulations of the lower levels of the N-2((BIIg)-I-3) will increase with
increases in the electron energy primarily due to cascade. Considerin
g the importance of the populations of the lower vibrational levels, w
e are beginning to analyze additional sprite spectra, measured at high
er resolution, which contain further information on the population of
B(v = 1). (C) 1998 Elsevier Science Ltd. All rights reserved.