New Fit for the O <sup>+</sup> ‐O Collision Frequency Including Fine Structure Effects

Abstract A new fit is presented for the oxygen ion‐neutral collision frequency . The fit explicitly depends on the neutral temperature , which characterizes the thermal distribution of fine structure levels of O( 3 ,1,2), and the reduced temperature , where is the ion temperature. A physically realistic fitting function adapted from the exact solution of a two‐state system is constrained to approach plausible analytic models in the limits that is high (Dalgarno's model, ) or is low (Langevin's model, –50 K). The target data for the fit are determined from the cross sections calculated by Hickman et al. (1997, https://doi.org/10.1103/PhysRevA.56.4633 ) and their extrapolations to lower and higher energies using the Langevin and Dalgarno models. The fit reproduces the target data within 1% for any and for any in the range . The values of the fitting parameters suggest that the fine structure effect is more important than the effect of the long range ion‐quadrupole and polarization potentials for K. A relationship is derived between the parameters of the Dalgarno model and the exponent of the power law dependence () at high .

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Publication Details

Journal
Journal of Geophysical Research Space Physics
Published
2025-10-01
DOI
https://doi.org/10.1029/2025ja034494
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
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article

New Fit for the O + ‐O Collision Frequency Including Fine Structure Effects

A. P. Hickman
Journal of Geophysical Research Space Physics
Ionosphere and magnetosphere dynamics
article

New Fit for the O + ‐O Collision Frequency Including Fine Structure Effects

A. P. Hickman
article en

Abstract

Abstract A new fit is presented for the oxygen ion‐neutral collision frequency . The fit explicitly depends on the neutral temperature , which characterizes the thermal distribution of fine structure levels of O( 3 ,1,2), and the reduced temperature , where is the ion temperature. A physically realistic fitting function adapted from the exact solution of a two‐state system is constrained to approach plausible analytic models in the limits that is high (Dalgarno's model, ) or is low (Langevin's model, –50 K). The target data for the fit are determined from the cross sections calculated by Hickman et al. (1997, https://doi.org/10.1103/PhysRevA.56.4633 ) and their extrapolations to lower and higher energies using the Langevin and Dalgarno models. The fit reproduces the target data within 1% for any and for any in the range . The values of the fitting parameters suggest that the fine structure effect is more important than the effect of the long range ion‐quadrupole and polarization potentials for K. A relationship is derived between the parameters of the Dalgarno model and the exponent of the power law dependence () at high .

Journal of Geophysical Research Space PhysicsVol. 130(10)
Lehigh University (US)
Openalex Percentile: Top 79%
Ionosphere and magnetosphere dynamics
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New Fit for the O <sup>+</sup> ‐O Collision Frequency Including Fine Structure Effects — A. P. Hickman · Journal of Geophysical Research Space Physics (2025) | TGRS Research Map | TGRS