An improved model of radiative transfer for the NLTE problem in the NIR bands of CO2 and CO molecules in the daytime atmosphere of Mars. 1. Input data and calculation method

Ogibalov, V. P.; Shved, G. M.

doi:10.1134/s003809461605004x

Cited by 5 publications

(2 citation statements)

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“…As shown in red in Figure C1b, for temperatures T in the 100-500 K range, Equation C2c returns 𝐴𝐴 k𝑘01 1 0 O values that decrease with increasing temperature. The orange curve shows results from a slightly different fit proposed by Ogibalov and Shved (2016), which is very similar. We adopt the original Castle et al (2012) fit in our parameterization.…”

Section: Appendix C: Parameterized Co 2 Cooling Rates At 15 µMmentioning

confidence: 73%

“…(2006), whereas the second is based on the newer temperature‐dependent rates measured by Castle et al. (2012) (see also Ogibalov & Shved, 2016). This change from an earlier temperature‐independent rate to a new temperature‐dependent rate that drops off markedly with increasing temperature in Figure C1b is very similar to the changes for the NO‐O collisional deactivation rate that we have parameterized in Figure 2, based on the theoretical work of Caridade et al.…”

Section: Comparison To O(3p) and Co2 Cooling Ratesmentioning

confidence: 99%

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Augmented Non‐LTE Parameterization of NO Infrared Radiative Cooling Rates

Eckermann

2023

JGR Space Physics

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The radiation of 5.3 μm photons by NO molecules is one of the more important processes for permanently removing energy from the thermosphere, and thus in controlling temperature and density responses to impulsive extraterrestrial energy inputs (e.g., Mlynczak et al., 2018). An accurate parameterization of NO cooling rates is therefore an indispensable component of any credible whole-atmosphere climate model, as well as of future whole-atmosphere numerical weather prediction models that seek to provide accurate forecasts of the thermosphere to drive physics-based ionospheric models used for space weather applications (Zawdie et al., 2020).As extraterrestrial energy is deposited within the thermosphere-ionosphere system, heat is thermally conducted by viscous processes to lower altitudes, where NO emissions can permanently remove some of this energy via radiation to space (see Figure 1 of Mlynczak et al., 2018). On long time scales, this NO cooling maintains and regulates thermospheric climate states, while on short time scales, it plays an important role in predicting thermospheric temperature and density responses to impulsive extraterrestrial energy inputs (

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Section: Appendix C: Parameterized Co 2 Cooling Rates At 15 µMmentioning

confidence: 73%