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September 7, 2025Open Access

A reversed Monte Carlo radiative transfer model for Titan PCM

Anthony Arfaux Sandrine Vinatier Vincent Eymet Vincent Forest zili he Bruno de Batz de Trenquelléon P. Rannou Ehouarn Millour Sébastien Lebonnois

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Key Points

To develop a reversed Monte Carlo model to simulate radiative transfer on Titan.
Utilized a Monte Carlo approach for radiative transfer modeling.
Focused on the specifics of Titan's atmospheric conditions.
Incorporated the effects of PCM in the simulations.
The model effectively simulates radiative transfer processes in Titan's atmosphere.
Demonstrated how PCM influences radiative behavior.
Provided insights into atmospheric interactions on Titan.

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Implication

Model demonstrates radiative transfer in Titan's atmosphere, highlighting the role of PCM.

Abstract

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Cite This Study

Arfaux et al. (2025) studied this question.

synapsesocial.com/papers/695d855e3483e917927a4cb8 https://doi.org/10.5194/epsc-dps2025-1294epsc-dps

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Keep reading

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1A spherical and heterogeneous radiative transfer code for near-infrared remote sensing: application to Titan2024 · 1 citations
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3Update of the thermal radiative transfer in the Venus PCM2024
4The DIRTY Model. I. Monte Carlo Radiative Transfer through DustOriginal Research · 2001 · 170 citations
5MONKI: a three-dimensional Monte Carlo simulator of total and polarised radiation reflected by planetary atmospheres2025

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