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Electron impact study of the 100 eV emission cross section and lifetime of the Lyman‐Birge‐Hopfield band system of N 2 : Direct excitation and cascade
Author(s) -
Ajello J. M.,
Malone C. P.,
Holsclaw G. M.,
Hoskins A. C.,
Eastes R. W.,
McClintock W. E.,
Johnson P. V.
Publication year - 2017
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1002/2017ja024087
Subject(s) - atomic physics , excitation , physics , electron ionization , cross section (physics) , electron , emission spectrum , ionization , electron excitation , optics , spectral line , ion , nuclear physics , quantum mechanics , astronomy
We have measured the 100 eV emission cross section of the optically forbidden Lyman‐Birge‐Hopfield (LBH) band system ( a 1 Π g → X 1 Σ + g ) of N 2 by electron‐impact‐induced fluorescence. Using a large (1.5 m diameter) vacuum chamber housing an electron gun system and the Mars Atmosphere and Volatile EvolutioN mission Imaging Ultraviolet Spectrograph optical engineering model, we have obtained calibrated spectral measurements of the LBH band system from 115 to 175 nm over a range of lines of sight to capture all of the optical emissions. These measurements represent the first experiment to directly isolate in the laboratory single‐scattering electron‐impact‐induced fluorescence from both direct excitation of the a 1 Π g state and cascading contributions to the a 1 Π g state ( a ′ 1 Σ − u and w 1 Δ u → a 1 Π g → X 1 Σ + g ). The determination of the total LBH emission cross section is accomplished by measuring the entire cylindrical glow pattern of the metastable emission from electron impact by imaging lines of sight that measure the glow intensity from zero to ~400 mm radial distance and calculating the ratio of the integrated intensity from the LBH glow pattern to that of a simultaneously observed optically allowed transition with a well‐established cross section: N i 120.0 nm. The “direct” emission cross section of the a 1 Π g state at 100 eV was determined to be σ em dir = (6.41 ± 1.3) × 10 −18 cm 2 . An important observation from the glow pattern behavior is that the total (direct + cascading) emission cross section is pressure dependent due to collision‐induced cascade transitions between close‐lying electronic states.