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Version 0.8.3. Now uses F_int rather than T_int for internal flux. Updated docs and paper. New notebooks
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CITATION.cff

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given-names: "Harrison"
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orcid: "https://orcid.org/0000-0002-8368-4641"
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title: "AGNI"
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version: 0.8.2
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version: 0.8.3
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doi: 10.xx/xx.xx
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date-released: 2024-09-13
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date-released: 2024-09-20
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url: "https://github.com/nichollsh/AGNI"

Project.toml

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name = "AGNI"
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uuid = "ede838c1-9ec3-4ebe-8ae8-da4091b3f21c"
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authors = ["Harrison Nicholls <harrison.nicholls@physics.ox.ac.uk>"]
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version = "0.8.2"
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version = "0.8.3"
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[deps]
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ArgParse = "c7e460c6-2fb9-53a9-8c5b-16f535851c63"

README.md

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</p>
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<p align="center">
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<b>A radiative-convective atmosphere model designed for interior coupling.</b>
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<b>A radiative-convective model for lava planet atmospheres.</b>
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</p>
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codemeta.json

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"datePublished": "2024-09-13",
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"dateModified": "2024-09-13",
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"dateCreated": "2024-09-13",
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"description": "A radiative-convective model for the atmospheres of rocky planets",
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"description": "A radiative-convective model for lava planet atmospheres.",
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"keywords": "physics, radiative transfer, exoplanets, astronomy, convection, radiation, planets, atmospheres",
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"license": "GPL v3.0",
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"title": "AGNI",
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"version": "0.8.2"
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"version": "0.8.3"
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}

docs/paper/paper.md

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---
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title: 'AGNI: A radiative-convective model for the atmospheres of rocky planets'
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title: 'AGNI: A radiative-convective model for lava planet atmospheres.'
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tags:
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- astronomy
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- physics,
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index: 1
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- name: Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700 AV Groningen, The Netherlands
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index: 2
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date: 16 September 2024
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date: 20 September 2024
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bibliography: paper.bib
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---

docs/src/usage.md

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* `execution.solution_type` tells the model which state to solve for. The allowed values (integers) are...
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- 1 : zero flux divergence at fixed `tmp_surf`
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- 2 : zero flux divergence, with `tmp_surf` set such that the conductive skin (CBL) conserves energy flux
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- 3 : the net upward flux at each layer is equal to `flux_int = sigma * tmp_int^4`
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- 3 : the net flux (up minus down) at each layer is equal to `flux_int`
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* `execution.solvers` tells the model which solvers to use. This is a list of strings, so multiple solvers can be applied sequentially. An empty string is always appended to the end of this list. Allowed solvers are...
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- [empty string] : no solving takes place, so the model just calculates fluxes using the initial state

misc/L98-59d.ipynb

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res/config/55cnce_chem.toml

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surface_material= "res/surface_albedos/basalt_tuff.dat"
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radius = 1.1959e7
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gravity = 22.304
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tmp_int = 0.0
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flux_int = 0.0
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turb_coeff = 0.001
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wind_speed = 2.0
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res/config/L-98-59d.toml

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surface_material= "res/surface_albedos/lunar_marebasalt.dat"
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radius = 6.59051e6
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gravity = 16.73
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tmp_int = 0.0
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flux_int = 0.0
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turb_coeff = 0.001
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wind_speed = 2.0
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res/config/condense.toml

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albedo_s = 0.2
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radius = 6.37e6
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gravity = 9.81
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tmp_int = 0.0
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flux_int = 0.0
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turb_coeff = 1.0e-4
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wind_speed = 10.0
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skin_k = 2.0

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