Ra. Armstrong et al., PHOTOMETRIC MEASUREMENTS IN THE SPRITES-95 AND SPRITES-96 CAMPAIGNS OF NITROGEN 2ND POSITIVE (399.8 NM) AND FIRST NEGATIVE (427.8 NM) EMISSIONS, Journal of atmospheric and solar-terrestrial physics, 60(7-9), 1998, pp. 787-799
We have obtained blue photometric measurements of the N-2 second posit
ive 399.8 nm and the N-2(+) first negative 427.8 nm emission from spri
tes, elves and lightning, along with supporting video images. The puls
e width and intensity results for sprites are consistent with those of
Suszcynsky et al. (1998). The red emission from sprites has been inde
pendently and unambiguously identified by Hampton et al. (1996) and Me
nde et al. (1995) as the nitrogen first positive band. The source has
been attributed to electron impact excitation from low energy electron
s(approximate to 1 eV) in the sprite. The short pulse width of the 427
.8 nm and 399.8 nm photometer rime traces obtained in this investigati
on are probably not from the same source that produces the red emissio
n. The results reported here indicate an initial energetic ionizing ev
ent sufficient to ionize and excite nitrogen followed by secondary ele
ctron processes which give rise to the dominant red emission. The phot
ometer results for elves are consistent with the EMP mechanism suggest
ed by Inan et al. (1996). The photometer traces obtained for lightning
indicate emissions consistent with a 'continuing current' as the char
ge redistributes within the thunderstorm cloud. We find that the ratio
of the intensity of the 399.8 nm N-2(2P) emission to that of 427.8 nm
N-2(+) (1N) emission can be used to discriminate among sprites, elves
and lightning. (C) 1998 Elsevier Science Ltd. All rights reserved.