
Modeling nightglow in atomic oxygen red and green lines under moderate disturbed geomagnetic conditions at midlatitudes
Author(s) -
A. V. Tashchilin,
A. V. Tashchilin,
L. A. Leonovich,
L. A. Leonovich
Publication year - 2017
Publication title -
solar-terrestrial physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.11
H-Index - 2
ISSN - 2500-0535
DOI - 10.12737/24276
Subject(s) - airglow , middle latitudes , dissociative recombination , atomic physics , atomic oxygen , earth's magnetic field , oxygen , atmospheric sciences , electron , atmosphere (unit) , excitation , ion , thermal , physics , recombination , environmental science , chemistry , meteorology , magnetic field , biochemistry , quantum mechanics , gene
We present results of a study of mid-latitude auroras. The study is based on optical measurements and theoretical modeling. The modeling shows that precipitation can indirectly generate airglow in red and green lines of atomic oxygen by increasing rates of ion formation and heating of thermal electrons. This causes an increase in the rate of dissociative recombination and thermal-electron-collision excitation of the 1D and 1S levels.