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Mechanisms for varying non-LTE contributions to OH rotational temperatures from measurements and modelling. II. Kinetic model

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Proxauf,  Bastian
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;
IMPRS for Solar System Science at the University of Göttingen, Max Planck Institute for Solar System Research, Max Planck Society;

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Noll, S., Proxauf, B., Kausch, W., & Kimeswenger, S. (2018). Mechanisms for varying non-LTE contributions to OH rotational temperatures from measurements and modelling. II. Kinetic model. Journal of Atmospheric and Solar-Terrestrial Physics, 175, 100-119. doi:10.1016/j.jastp.2018.05.005.


Cite as: https://hdl.handle.net/21.11116/0000-0003-5053-5
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