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The optical spectrum of aircraft St. Elmo's fire
Author(s) -
Wescott E. M.,
Sentman D. D.,
Heavner M. J.,
Hallinan T. J.,
Hampton D. L.,
Osborne D. L.
Publication year - 1996
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/96gl03621
Subject(s) - spectrograph , lightning (connector) , altitude (triangle) , physics , population , meteorology , monochromatic color , jet (fluid) , environmental science , thunderstorm , remote sensing , atmospheric sciences , spectral line , optics , astronomy , geology , quantum mechanics , power (physics) , geometry , mathematics , demography , sociology , thermodynamics
On February 26, 1995, during a NASA sponsored mission to Peru to study red sprites and blue jets, the instrumented Westwind 2 jet aircraft encountered spectacular St. Elmo's fire from the wing pods, tail and nose while flying through a cloud at an altitude of 13.83 km (45,376 ft). The phenomenon was captured on low light level monochromatic and color television systems aboard the aircraft, and its spectrum was recorded on a low light level TV spectrograph with response from 395.0 to 750.0 nm. The cameras and spectrograph also recorded scattered intra‐cloud lightning and a possible lightning discharge near, or to, the aircraft. The spectrum of St. Elmo's fire was primarily the second (2nd) positive bands of N 2 . The data were consistent with a population of electrons having relatively low energy (<18 eV).