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Dummy tides inequality, convergence robustness, docs #326

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Jan 21, 2025
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Dummy tides inequality, convergence robustness, docs #326

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6eb6800
Apply dummy tides based on inequality
nichollsh Jan 19, 2025
ef33e37
Criteria must be satisfied for 2 sequential iterations for convergenc…
nichollsh Jan 19, 2025
aaa9596
Citation info
nichollsh Jan 19, 2025
1c6de89
Update citations in readme. Update printing to log
nichollsh Jan 19, 2025
9d8f0fa
Add rheological transition location and width variables to config. Ad…
nichollsh Jan 20, 2025
eed85cf
Update configs
nichollsh Jan 20, 2025
51d76f0
Update tests
nichollsh Jan 20, 2025
966a065
Style
nichollsh Jan 20, 2025
87ef163
Merge branch 'main' into hn/tideineq
nichollsh Jan 20, 2025
e0b2869
Fix test
nichollsh Jan 20, 2025
0f1ddde
Remove temp file
nichollsh Jan 20, 2025
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26 changes: 13 additions & 13 deletions README.md
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Original file line number Diff line number Diff line change
Expand Up @@ -56,20 +56,24 @@ If you make use of PROTEUS, please reference the following manuscripts, and stat
author = {{Nicholls}, Harrison and {Pierrehumbert}, Raymond T. and {Lichtenberg}, Tim and {Soucasse}, Laurent and {Smeets}, Stef},
title = "{Convective shutdown in the atmospheres of lava worlds}",
journal = {Monthly Notices of the Royal Astronomical Society},
year = 2024,
month = dec,
doi = {10.1093/mnras/stae2772},
url = {https://arxiv.org/abs/2412.11987}
year = 2025,
month = jan,
volume = {536},
number = {3},
pages = {2957-2971},
doi = {10.1093/mnras/stae2772},
}

@ARTICLE{Nicholls2024JGRP,
author = {{Nicholls}, Harrison and {Lichtenberg}, Tim and {Bower}, Dan J. and and {Pierrehumbert}, Raymond T.},
title = "{Magma ocean evolution at arbitrary redox state}",
author = {{Nicholls}, Harrison and {Lichtenberg}, Tim and {Bower}, Dan J. and {Pierrehumbert}, Raymond},
title = "{Magma Ocean Evolution at Arbitrary Redox State}",
journal = {Journal of Geophysical Research (Planets)},
year = 2024,
month = nov,
doi = {10.1029/2024JE008576},
url = {https://arxiv.org/abs/2411.19137}
month = dec,
volume = {129},
number = {12},
pages = {2024JE008576},
doi = {10.1029/2024JE008576},
}

@ARTICLE{Lichtenberg2021JGRP,
Expand All @@ -83,10 +87,6 @@ If you make use of PROTEUS, please reference the following manuscripts, and stat
eid = {e06711},
pages = {e06711},
doi = {10.1029/2020JE006711},
archivePrefix = {arXiv},
eprint = {2101.10991},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021JGRE..12606711L}
}
```

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4 changes: 3 additions & 1 deletion input/default.toml
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Expand Up @@ -109,7 +109,7 @@ author = "Harrison Nicholls, Tim Lichtenberg"

[orbit.dummy]
H_tide = 1e-11 # Fixed tidal power density [W kg-1]
Phi_tide = 0.3 # Maximum local melt fraction to which tides can be applied.
Phi_tide = "<0.3" # Tidal heating applied when inequality locally satisfied


# Planetary structure - physics table
Expand Down Expand Up @@ -179,6 +179,8 @@ author = "Harrison Nicholls, Tim Lichtenberg"
F_initial = 8.0E4 # Initial heat flux guess [W m-2]
radiogenic_heat = true # enable radiogenic heat production
tidal_heat = false # enable tidal heat production
rheo_phi_loc = 0.4 # Centre of rheological transition
rheo_phi_wid = 0.15 # Width of rheological transition

module = "spider" # Which interior module to use

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4 changes: 3 additions & 1 deletion input/demos/aragog.toml
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Expand Up @@ -109,7 +109,7 @@ author = "Harrison Nicholls, Tim Lichtenberg"

[orbit.dummy]
H_tide = 1e-7 # Fixed tidal power density [W kg-1]
Phi_tide = 0.3 # Maximum local melt fraction to which tides can be applied.
Phi_tide = "<0.3" # Tidal heating applied when inequality locally satisfied


# Planetary structure - physics table
Expand Down Expand Up @@ -179,6 +179,8 @@ author = "Harrison Nicholls, Tim Lichtenberg"
F_initial = 1e6 # Initial heat flux guess [W m-2]
radiogenic_heat = false # enable radiogenic heat production
tidal_heat = true # enable tidal heat production
rheo_phi_loc = 0.4 # Centre of rheological transition
rheo_phi_wid = 0.15 # Width of rheological transition

module = "aragog" # Which interior module to use

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4 changes: 3 additions & 1 deletion input/demos/dummy.toml
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Expand Up @@ -109,7 +109,7 @@ author = "Harrison Nicholls, Tim Lichtenberg"

[orbit.dummy]
H_tide = 1e-9 # Fixed tidal power density [W kg-1]
Phi_tide = 0.3 # Maximum local melt fraction to which tides can be applied.
Phi_tide = "<0.3" # Tidal heating applied when inequality locally satisfied


# Planetary structure - physics table
Expand Down Expand Up @@ -179,6 +179,8 @@ author = "Harrison Nicholls, Tim Lichtenberg"
F_initial = 1e6 # Initial heat flux guess [W m-2]
radiogenic_heat = false # enable radiogenic heat production
tidal_heat = true # enable tidal heat production
rheo_phi_loc = 0.4 # Centre of rheological transition
rheo_phi_wid = 0.15 # Width of rheological transition

module = "dummy" # Which interior module to use

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4 changes: 3 additions & 1 deletion input/demos/escape.toml
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Original file line number Diff line number Diff line change
Expand Up @@ -109,7 +109,7 @@ author = "Harrison Nicholls, Tim Lichtenberg"

[orbit.dummy]
H_tide = 1e-11 # Fixed tidal power density [W kg-1]
Phi_tide = 0.3 # Maximum local melt fraction to which tides can be applied.
Phi_tide = "<0.3" # Tidal heating applied when inequality locally satisfied


# Planetary structure - physics table
Expand Down Expand Up @@ -179,6 +179,8 @@ author = "Harrison Nicholls, Tim Lichtenberg"
F_initial = 8.0E4 # Initial heat flux guess [W m-2]
radiogenic_heat = true # enable radiogenic heat production
tidal_heat = false # enable tidal heat production
rheo_phi_loc = 0.4 # Centre of rheological transition
rheo_phi_wid = 0.15 # Width of rheological transition

module = "spider" # Which interior module to use

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261 changes: 0 additions & 261 deletions input/demos/spider_tides.toml
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This file was deleted.

4 changes: 3 additions & 1 deletion input/planets/hd63433d.toml
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Original file line number Diff line number Diff line change
Expand Up @@ -109,7 +109,7 @@ author = "Harrison Nicholls, Tim Lichtenberg"

[orbit.dummy]
H_tide = 1e-11 # Fixed tidal power density [W kg-1]
Phi_tide = 0.3 # Maximum local melt fraction to which tides can be applied.
Phi_tide = "<0.3" # Tidal heating applied when inequality locally satisfied


# Planetary structure - physics table
Expand Down Expand Up @@ -179,6 +179,8 @@ author = "Harrison Nicholls, Tim Lichtenberg"
F_initial = 1e5 # Initial heat flux guess [W m-2]
radiogenic_heat = true # enable radiogenic heat production
tidal_heat = false # enable tidal heat production
rheo_phi_loc = 0.4 # Centre of rheological transition
rheo_phi_wid = 0.15 # Width of rheological transition

module = "spider" # Which interior module to use

Expand Down
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