A New 2D Energy Balance Model for Simulating the Climates of Rapidly and Slowly Rotating Terrestrial Planets
Energy balance models (EBMs), alongside radiative–convective climate models and global climate models (GCMs), are useful tools for simulating planetary climates. Historically, planetary and exoplanetary EBMs have solely been 1D latitudinally dependent models with no longitudinal dependence, until th...
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| Autor Principal: | |
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| Formato: | Artigo |
| Idioma: | Inglês |
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IOP Publishing
2024-01-01
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| Series: | The Planetary Science Journal |
| Assuntos: | |
| Acceso en liña: | https://doi.org/10.3847/PSJ/ad0729 |
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