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THOR

CI

Flexible Global Circulation Model to Explore Planetary Atmospheres

THOR is a GCM that solves the three-dimensional non-hydrostatic Euler equations on an icosahedral grid. THOR was designed to run on Graphics Processing Units (GPUs).

If you use this code please cite: Mendonça, J.M., Grimm, S.L., Grosheintz, L., & Heng, K., ApJ, 829, 115, 2016

If using version 2.0 or later, please also cite: Deitrick, R., Mendonça, J.M., Schroffenegger, U., Grimm, S.L., Tsai, S.-M., & Heng, K., ApJS, 248, 2, 2020

Current code owners: Joao Mendonca: joao.mendonca@space.dtu.dk, Russell Deitrick: russell.deitrick@csh.unibe.ch, Urs Schroffenegger: urs.schroffenegger@csh.unibe.ch

Copyright (C) 2017-2021 Exoclimes Simulation Platform

BUILD & RUN THOR (TL;DR instructions)

 $ sudo apt-get install git make gcc g++ cmake nvidia-cuda-toolkit nvidia-utils-390 libhdf5-dev libhdf5-100 libhdf5-serial-dev libhdf5-cpp-100
$ git clone https://github.com/exoclime/THOR.git
$ cd THOR
$ cp Makefile.conf.template Makefile.conf

Find the SM value of your Nvidia GPU. Decide if you want to run without any physics module empty physics module, or the one with radiative transfer, the multi module. Then open Makefile.conf in a text editor and edit like so:

 MODULES_SRC := src/physics/managers/<module_type>/
SM:=<SM value of your card>

Set module_typeto empty (default) or multi.

Then head back to the command line and

 $ make -j8 release

Finally, run

 $ bin/esp ifile/<config file for your planet>

Furthur information

View our wiki pages here

Tutorial from ESP Summer School 2019

About

Atmospheric fluid dynamics solver optimized for GPUs.

Resources

Readme
GPL-3.0 license
Activity
Custom properties

Stars

47 stars

Watchers

8 watching

Forks

14 forks
Report repository

Releases

Packages

Used by

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Add copy buttons to all 
 blocks\n(function() {\n function addCopyButtons() {\n document.querySelectorAll('pre code').forEach(function(codeBlock) {\n if (codeBlock.parentElement.hasAttribute('data-copy-added')) return;\n codeBlock.parentElement.setAttribute('data-copy-added', 'true');\n \n var btn = document.createElement('button');\n btn.textContent = 'Copy';\n btn.style.cssText = 'position:absolute;top:4px;right:4px;padding:2px 8px;font-size:11px;background:#4ecdc4;border:none;border-radius:4px;color:#1a1a2e;cursor:pointer;opacity:0.7;transition:opacity 0.2s;';\n btn.onmouseover = function() { this.style.opacity = '1'; };\n btn.onmouseout = function() { this.style.opacity = '0.7'; };\n btn.onclick = function() {\n navigator.clipboard.writeText(codeBlock.textContent).then(function() {\n btn.textContent = 'Copied!';\n setTimeout(function() { btn.textContent = 'Copy'; }, 1500);\n });\n };\n codeBlock.parentElement.style.position = 'relative';\n codeBlock.parentElement.appendChild(btn);\n });\n }\n \n addCopyButtons();\n \n // Re-run on dynamic content\n var observer = new MutationObserver(addCopyButtons);\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Add Copy Buttons to Code Blocks");
}
} catch(__e) { console.warn('[Userscript:Add Copy Buttons to Code Blocks]', __e); }
})();
(function(){
try {
var __m = "github.com";
var __re = new RegExp('^' + "github\\.com" + '

Skip to content
BranchesTags
Repository files navigation
THOR
CI
Flexible Global Circulation Model to Explore Planetary Atmospheres
THOR is a GCM that solves the three-dimensional non-hydrostatic Euler equations on an icosahedral grid. THOR was designed to run on Graphics Processing Units (GPUs).
If you use this code please cite: Mendonça, J.M., Grimm, S.L., Grosheintz, L., & Heng, K., ApJ, 829, 115, 2016
If using version 2.0 or later, please also cite: Deitrick, R., Mendonça, J.M., Schroffenegger, U., Grimm, S.L., Tsai, S.-M., & Heng, K., ApJS, 248, 2, 2020
Current code owners: Joao Mendonca: joao.mendonca@space.dtu.dk, Russell Deitrick: russell.deitrick@csh.unibe.ch, Urs Schroffenegger: urs.schroffenegger@csh.unibe.ch
Copyright (C) 2017-2021 Exoclimes Simulation Platform
BUILD & RUN THOR (TL;DR instructions)
 $ sudo apt-get install git make gcc g++ cmake nvidia-cuda-toolkit nvidia-utils-390 libhdf5-dev libhdf5-100 libhdf5-serial-dev libhdf5-cpp-100
$ git clone https://github.com/exoclime/THOR.git
$ cd THOR
$ cp Makefile.conf.template Makefile.conf

Find the SM value of your Nvidia GPU. Decide if you want to run without any physics module empty physics module, or the one with radiative transfer, the multi module. Then open Makefile.conf in a text editor and edit like so:
 MODULES_SRC := src/physics/managers/<module_type>/
SM:=<SM value of your card> 
Set module_typeto empty (default) or multi.
Then head back to the command line and
 $ make -j8 release

Finally, run
 $ bin/esp ifile/<config file for your planet>

Furthur information
View our wiki pages here
Tutorial from ESP Summer School 2019
About
Atmospheric fluid dynamics solver optimized for GPUs.
Resources
Readme
GPL-3.0 license
Activity
Custom properties
Stars
47 stars
Watchers
8 watching
Forks
14 forks
Report repository
Releases
Packages
Used by
Contributors
Languages

, 'i');
if (__m === '*' || __re.test(location.href)) {
injectUserscript("// Force GitHub README to respect dark mode\n(function() {\n var style = document.createElement('style');\n style.textContent = '\n .markdown-body {\n color-scheme: dark light;\n }\n .markdown-body pre { background: #161b22 !important; }\n .markdown-body code { background: rgba(110, 118, 129, 0.4) !important; }\n .markdown-body table th, .markdown-body table td { border-color: #30363d !important; }\n .markdown-body img { background: #0d1117; }\n .markdown-body blockquote { border-left-color: #8b949e; }\n .markdown-body hr { border-color: #30363d; }\n ';\n document.head.appendChild(style);\n})();", "GitHub Dark Mode README Fix");
}
} catch(__e) { console.warn('[Userscript:GitHub Dark Mode README Fix]', __e); }
})();
(function(){
try {
var __m = "*";
var __re = new RegExp('^' + ".*" + '

Skip to content
BranchesTags
Repository files navigation
THOR
CI
Flexible Global Circulation Model to Explore Planetary Atmospheres
THOR is a GCM that solves the three-dimensional non-hydrostatic Euler equations on an icosahedral grid. THOR was designed to run on Graphics Processing Units (GPUs).
If you use this code please cite: Mendonça, J.M., Grimm, S.L., Grosheintz, L., & Heng, K., ApJ, 829, 115, 2016
If using version 2.0 or later, please also cite: Deitrick, R., Mendonça, J.M., Schroffenegger, U., Grimm, S.L., Tsai, S.-M., & Heng, K., ApJS, 248, 2, 2020
Current code owners: Joao Mendonca: joao.mendonca@space.dtu.dk, Russell Deitrick: russell.deitrick@csh.unibe.ch, Urs Schroffenegger: urs.schroffenegger@csh.unibe.ch
Copyright (C) 2017-2021 Exoclimes Simulation Platform
BUILD & RUN THOR (TL;DR instructions)
 $ sudo apt-get install git make gcc g++ cmake nvidia-cuda-toolkit nvidia-utils-390 libhdf5-dev libhdf5-100 libhdf5-serial-dev libhdf5-cpp-100
$ git clone https://github.com/exoclime/THOR.git
$ cd THOR
$ cp Makefile.conf.template Makefile.conf

Find the SM value of your Nvidia GPU. Decide if you want to run without any physics module empty physics module, or the one with radiative transfer, the multi module. Then open Makefile.conf in a text editor and edit like so:
 MODULES_SRC := src/physics/managers/<module_type>/
SM:=<SM value of your card> 
Set module_typeto empty (default) or multi.
Then head back to the command line and
 $ make -j8 release

Finally, run
 $ bin/esp ifile/<config file for your planet>

Furthur information
View our wiki pages here
Tutorial from ESP Summer School 2019
About
Atmospheric fluid dynamics solver optimized for GPUs.
Resources
Readme
GPL-3.0 license
Activity
Custom properties
Stars
47 stars
Watchers
8 watching
Forks
14 forks
Report repository
Releases
Packages
Used by
Contributors
Languages

, 'i');
if (__m === '*' || __re.test(location.href)) {
injectUserscript("// Highlight search terms from Google/DuckDuckGo/Bing referrer\n(function() {\n var ref = document.referrer;\n var terms = [];\n \n if (ref.includes('google.com') || ref.includes('duckduckgo.com') || ref.includes('bing.com')) {\n var url = new URL(ref);\n var q = url.searchParams.get('q') || url.searchParams.get('p');\n if (q) {\n terms = q.split(/\\s+/).filter(function(t) { return t.length > 2; });\n }\n }\n \n if (terms.length === 0) return;\n \n var style = document.createElement('style');\n style.textContent = '.userscript-highlight { background: #fbbf24; color: #1a1a2e; padding: 1px 3px; border-radius: 2px; }';\n document.head.appendChild(style);\n \n function highlight(node) {\n if (node.nodeType === 3) { // text node\n var text = node.textContent;\n var found = false;\n terms.forEach(function(term) {\n var regex = new RegExp('(' + term.replace(/[.*+?^${}()|[\\]\\\\]/g, '\\\\') + ')', 'gi');\n if (regex.test(text)) {\n found = true;\n var frag = document.createDocumentFragment();\n var parts = text.split(regex);\n parts.forEach(function(part, i) {\n if (i % 2 === 0) {\n frag.appendChild(document.createTextNode(part));\n } else {\n var span = document.createElement('span');\n span.className = 'userscript-highlight';\n span.textContent = part;\n frag.appendChild(span);\n }\n });\n node.parentNode.replaceChild(frag, node);\n }\n });\n } else if (node.nodeType === 1 && node.childNodes) { // element\n var skipTags = ['SCRIPT', 'STYLE', 'NOSCRIPT', 'TEXTAREA', 'INPUT', 'SELECT'];\n if (!skipTags.includes(node.tagName)) {\n Array.from(node.childNodes).forEach(highlight);\n }\n }\n }\n \n highlight(document.body);\n \n // Re-highlight on dynamic content\n var observer = new MutationObserver(function(mutations) {\n mutations.forEach(function(m) {\n m.addedNodes.forEach(function(node) {\n if (node.nodeType === 1 || node.nodeType === 3) highlight(node);\n });\n });\n });\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Highlight Search Terms");
}
} catch(__e) { console.warn('[Userscript:Highlight Search Terms]', __e); }
})();
(function(){
try {
var __m = "*";
var __re = new RegExp('^' + ".*" + '

Skip to content
BranchesTags
Repository files navigation
THOR
CI
Flexible Global Circulation Model to Explore Planetary Atmospheres
THOR is a GCM that solves the three-dimensional non-hydrostatic Euler equations on an icosahedral grid. THOR was designed to run on Graphics Processing Units (GPUs).
If you use this code please cite: Mendonça, J.M., Grimm, S.L., Grosheintz, L., & Heng, K., ApJ, 829, 115, 2016
If using version 2.0 or later, please also cite: Deitrick, R., Mendonça, J.M., Schroffenegger, U., Grimm, S.L., Tsai, S.-M., & Heng, K., ApJS, 248, 2, 2020
Current code owners: Joao Mendonca: joao.mendonca@space.dtu.dk, Russell Deitrick: russell.deitrick@csh.unibe.ch, Urs Schroffenegger: urs.schroffenegger@csh.unibe.ch
Copyright (C) 2017-2021 Exoclimes Simulation Platform
BUILD & RUN THOR (TL;DR instructions)
 $ sudo apt-get install git make gcc g++ cmake nvidia-cuda-toolkit nvidia-utils-390 libhdf5-dev libhdf5-100 libhdf5-serial-dev libhdf5-cpp-100
$ git clone https://github.com/exoclime/THOR.git
$ cd THOR
$ cp Makefile.conf.template Makefile.conf

Find the SM value of your Nvidia GPU. Decide if you want to run without any physics module empty physics module, or the one with radiative transfer, the multi module. Then open Makefile.conf in a text editor and edit like so:
 MODULES_SRC := src/physics/managers/<module_type>/
SM:=<SM value of your card> 
Set module_typeto empty (default) or multi.
Then head back to the command line and
 $ make -j8 release

Finally, run
 $ bin/esp ifile/<config file for your planet>

Furthur information
View our wiki pages here
Tutorial from ESP Summer School 2019
About
Atmospheric fluid dynamics solver optimized for GPUs.
Resources
Readme
GPL-3.0 license
Activity
Custom properties
Stars
47 stars
Watchers
8 watching
Forks
14 forks
Report repository
Releases
Packages
Used by
Contributors
Languages

, 'i');
if (__m === '*' || __re.test(location.href)) {
injectUserscript("// Strip utm_, fbclid, gclid, etc. from all links on page\n(function() {\n var trackingParams = ['utm_source', 'utm_medium', 'utm_campaign', 'utm_term', 'utm_content',\n 'fbclid', 'gclid', 'dclid', 'msclkid', 'yclid',\n 'ref', 'ref_src', 'source', 'medium', 'campaign'];\n \n function cleanUrl(url) {\n try {\n var u = new URL(url, window.location.origin);\n var changed = false;\n trackingParams.forEach(function(p) {\n if (u.searchParams.has(p)) {\n u.searchParams.delete(p);\n changed = true;\n }\n });\n return changed ? u.toString() : url;\n } catch (e) {\n return url;\n }\n }\n \n function cleanLinks() {\n document.querySelectorAll('a[href]').forEach(function(a) {\n var clean = cleanUrl(a.href);\n if (clean !== a.href) a.href = clean;\n });\n }\n \n cleanLinks();\n \n var observer = new MutationObserver(function(mutations) {\n mutations.forEach(function(m) {\n m.addedNodes.forEach(function(node) {\n if (node.nodeType === 1) {\n if (node.tagName === 'A') cleanLinks();\n node.querySelectorAll('a[href]').forEach(function(a) {\n var clean = cleanUrl(a.href);\n if (clean !== a.href) a.href = clean;\n });\n }\n });\n });\n });\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Remove Tracking Parameters from Links");
}
} catch(__e) { console.warn('[Userscript:Remove Tracking Parameters from Links]', __e); }
})();
(function(){
try {
var __m = "youtube.com";
var __re = new RegExp('^' + "youtube\\.com" + '

Skip to content
BranchesTags
Repository files navigation
THOR
CI
Flexible Global Circulation Model to Explore Planetary Atmospheres
THOR is a GCM that solves the three-dimensional non-hydrostatic Euler equations on an icosahedral grid. THOR was designed to run on Graphics Processing Units (GPUs).
If you use this code please cite: Mendonça, J.M., Grimm, S.L., Grosheintz, L., & Heng, K., ApJ, 829, 115, 2016
If using version 2.0 or later, please also cite: Deitrick, R., Mendonça, J.M., Schroffenegger, U., Grimm, S.L., Tsai, S.-M., & Heng, K., ApJS, 248, 2, 2020
Current code owners: Joao Mendonca: joao.mendonca@space.dtu.dk, Russell Deitrick: russell.deitrick@csh.unibe.ch, Urs Schroffenegger: urs.schroffenegger@csh.unibe.ch
Copyright (C) 2017-2021 Exoclimes Simulation Platform
BUILD & RUN THOR (TL;DR instructions)
 $ sudo apt-get install git make gcc g++ cmake nvidia-cuda-toolkit nvidia-utils-390 libhdf5-dev libhdf5-100 libhdf5-serial-dev libhdf5-cpp-100
$ git clone https://github.com/exoclime/THOR.git
$ cd THOR
$ cp Makefile.conf.template Makefile.conf

Find the SM value of your Nvidia GPU. Decide if you want to run without any physics module empty physics module, or the one with radiative transfer, the multi module. Then open Makefile.conf in a text editor and edit like so:
 MODULES_SRC := src/physics/managers/<module_type>/
SM:=<SM value of your card> 
Set module_typeto empty (default) or multi.
Then head back to the command line and
 $ make -j8 release

Finally, run
 $ bin/esp ifile/<config file for your planet>

Furthur information
View our wiki pages here
Tutorial from ESP Summer School 2019
About
Atmospheric fluid dynamics solver optimized for GPUs.
Resources
Readme
GPL-3.0 license
Activity
Custom properties
Stars
47 stars
Watchers
8 watching
Forks
14 forks
Report repository
Releases
Packages
Used by
Contributors
Languages

, 'i');
if (__m === '*' || __re.test(location.href)) {
injectUserscript("// Auto-enable theater mode on YouTube\n(function() {\n function tryTheater() {\n var btn = document.querySelector('button[aria-label=\"Theater mode\"], ytd-player #player button[title=\"Theater mode\"]');\n if (btn && !btn.classList.contains('activated')) {\n btn.click();\n }\n }\n \n // Try immediately\n tryTheater();\n \n // Try after navigation (SPA)\n var lastUrl = location.href;\n setInterval(function() {\n if (location.href !== lastUrl) {\n lastUrl = location.href;\n setTimeout(tryTheater, 500);\n }\n }, 1000);\n \n // Also try on player load\n var observer = new MutationObserver(tryTheater);\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "YouTube Theater Mode Default");
}
} catch(__e) { console.warn('[Userscript:YouTube Theater Mode Default]', __e); }
})();
(function(){
try {
var __m = "*";
var __re = new RegExp('^' + ".*" + '

Skip to content
BranchesTags
Repository files navigation
THOR
CI
Flexible Global Circulation Model to Explore Planetary Atmospheres
THOR is a GCM that solves the three-dimensional non-hydrostatic Euler equations on an icosahedral grid. THOR was designed to run on Graphics Processing Units (GPUs).
If you use this code please cite: Mendonça, J.M., Grimm, S.L., Grosheintz, L., & Heng, K., ApJ, 829, 115, 2016
If using version 2.0 or later, please also cite: Deitrick, R., Mendonça, J.M., Schroffenegger, U., Grimm, S.L., Tsai, S.-M., & Heng, K., ApJS, 248, 2, 2020
Current code owners: Joao Mendonca: joao.mendonca@space.dtu.dk, Russell Deitrick: russell.deitrick@csh.unibe.ch, Urs Schroffenegger: urs.schroffenegger@csh.unibe.ch
Copyright (C) 2017-2021 Exoclimes Simulation Platform
BUILD & RUN THOR (TL;DR instructions)
 $ sudo apt-get install git make gcc g++ cmake nvidia-cuda-toolkit nvidia-utils-390 libhdf5-dev libhdf5-100 libhdf5-serial-dev libhdf5-cpp-100
$ git clone https://github.com/exoclime/THOR.git
$ cd THOR
$ cp Makefile.conf.template Makefile.conf

Find the SM value of your Nvidia GPU. Decide if you want to run without any physics module empty physics module, or the one with radiative transfer, the multi module. Then open Makefile.conf in a text editor and edit like so:
 MODULES_SRC := src/physics/managers/<module_type>/
SM:=<SM value of your card> 
Set module_typeto empty (default) or multi.
Then head back to the command line and
 $ make -j8 release

Finally, run
 $ bin/esp ifile/<config file for your planet>

Furthur information
View our wiki pages here
Tutorial from ESP Summer School 2019
About
Atmospheric fluid dynamics solver optimized for GPUs.
Resources
Readme
GPL-3.0 license
Activity
Custom properties
Stars
47 stars
Watchers
8 watching
Forks
14 forks
Report repository
Releases
Packages
Used by
Contributors
Languages

, 'i');
if (__m === '*' || __re.test(location.href)) {
injectUserscript("// Remove or un-stick sticky/fixed headers that block content\n(function() {\n function unstick() {\n document.querySelectorAll('header, nav, [role=\"banner\"], .header, .navbar, .sticky, .fixed-top, [style*=\"position: fixed\"], [style*=\"position:sticky\"]').forEach(function(el) {\n if (el.style.position === 'fixed' || el.style.position === 'sticky' || \n getComputedStyle(el).position === 'fixed' || getComputedStyle(el).position === 'sticky') {\n el.style.position = 'static';\n el.style.top = 'auto';\n el.style.zIndex = 'auto';\n }\n });\n }\n \n unstick();\n \n var observer = new MutationObserver(unstick);\n observer.observe(document.body, { childList: true, subtree: true, attributes: true, attributeFilter: ['style', 'class'] });\n})();", "Kill Sticky Headers");
}
} catch(__e) { console.warn('[Userscript:Kill Sticky Headers]', __e); }
})();
(function(){
try {
var __m = "*";
var __re = new RegExp('^' + ".*" + '

Skip to content
BranchesTags
Repository files navigation
THOR
CI
Flexible Global Circulation Model to Explore Planetary Atmospheres
THOR is a GCM that solves the three-dimensional non-hydrostatic Euler equations on an icosahedral grid. THOR was designed to run on Graphics Processing Units (GPUs).
If you use this code please cite: Mendonça, J.M., Grimm, S.L., Grosheintz, L., & Heng, K., ApJ, 829, 115, 2016
If using version 2.0 or later, please also cite: Deitrick, R., Mendonça, J.M., Schroffenegger, U., Grimm, S.L., Tsai, S.-M., & Heng, K., ApJS, 248, 2, 2020
Current code owners: Joao Mendonca: joao.mendonca@space.dtu.dk, Russell Deitrick: russell.deitrick@csh.unibe.ch, Urs Schroffenegger: urs.schroffenegger@csh.unibe.ch
Copyright (C) 2017-2021 Exoclimes Simulation Platform
BUILD & RUN THOR (TL;DR instructions)
 $ sudo apt-get install git make gcc g++ cmake nvidia-cuda-toolkit nvidia-utils-390 libhdf5-dev libhdf5-100 libhdf5-serial-dev libhdf5-cpp-100
$ git clone https://github.com/exoclime/THOR.git
$ cd THOR
$ cp Makefile.conf.template Makefile.conf

Find the SM value of your Nvidia GPU. Decide if you want to run without any physics module empty physics module, or the one with radiative transfer, the multi module. Then open Makefile.conf in a text editor and edit like so:
 MODULES_SRC := src/physics/managers/<module_type>/
SM:=<SM value of your card> 
Set module_typeto empty (default) or multi.
Then head back to the command line and
 $ make -j8 release

Finally, run
 $ bin/esp ifile/<config file for your planet>

Furthur information
View our wiki pages here
Tutorial from ESP Summer School 2019
About
Atmospheric fluid dynamics solver optimized for GPUs.
Resources
Readme
GPL-3.0 license
Activity
Custom properties
Stars
47 stars
Watchers
8 watching
Forks
14 forks
Report repository
Releases
Packages
Used by
Contributors
Languages

, 'i');
if (__m === '*' || __re.test(location.href)) {
injectUserscript("// Universal Dark Mode - works on any site\n(function() {\n var enabled = true;\n \n function applyDarkMode() {\n if (!enabled) return;\n \n // Create style element if it doesn't exist\n var style = document.getElementById('universal-dark-mode-style');\n if (!style) {\n style = document.createElement('style');\n style.id = 'universal-dark-mode-style';\n document.head.appendChild(style);\n }\n \n // Dark mode CSS - inverts colors but preserves images/video\n style.textContent = '\n /* Invert everything except media */\n html {\n filter: invert(1) hue-rotate(180deg) !important;\n background: #1a1a2e !important;\n }\n \n /* Restore images, videos, iframes, canvas */\n img, video, iframe, canvas, svg, picture, [style*=\"background-image\"] {\n filter: invert(1) hue-rotate(180deg) !important;\n }\n \n /* Preserve specific elements that should not be inverted */\n .no-dark-mode, .no-dark-mode *,\n [data-theme=\"light\"], [data-theme=\"light\"],\n .ace_editor, .ace_editor *,\n .CodeMirror, .CodeMirror *,\n .monaco-editor, .monaco-editor *,\n .markdown-body pre, .markdown-body pre *,\n .highlight, .highlight *,\n pre code, pre code * {\n filter: none !important;\n }\n \n /* Fix common UI elements */\n .modal, .popup, .dropdown-menu, .tooltip, .popover {\n filter: invert(1) hue-rotate(180deg) !important;\n background: #2d2d44 !important;\n border-color: #444 !important;\n }\n \n /* Scrollbars */\n ::-webkit-scrollbar { background: #1a1a2e !important; }\n ::-webkit-scrollbar-thumb { background: #444 !important; }\n ::-webkit-scrollbar-thumb:hover { background: #555 !important; }\n \n /* Selection */\n ::selection { background: #4ecdc4 !important; color: #1a1a2e !important; }\n ::-moz-selection { background: #4ecdc4 !important; color: #1a1a2e !important; }\n ';\n }\n \n function removeDarkMode() {\n var style = document.getElementById('universal-dark-mode-style');\n if (style) style.remove();\n }\n \n // Toggle with Alt+Shift+D\n document.addEventListener('keydown', function(e) {\n if (e.altKey && e.shiftKey && e.key === 'D') {\n e.preventDefault();\n enabled = !enabled;\n if (enabled) {\n applyDarkMode();\n console.log('[Universal Dark Mode] Enabled');\n } else {\n removeDarkMode();\n console.log('[Universal Dark Mode] Disabled');\n }\n }\n });\n \n // Apply on load\n applyDarkMode();\n \n // Re-apply on dynamic content\n var observer = new MutationObserver(function(mutations) {\n if (enabled && !document.getElementById('universal-dark-mode-style')) {\n applyDarkMode();\n }\n });\n observer.observe(document.head, { childList: true });\n \n console.log('[Universal Dark Mode] Loaded - Press Alt+Shift+D to toggle');\n})();", "Universal Dark Mode");
}
} catch(__e) { console.warn('[Userscript:Universal Dark Mode]', __e); }
})();
})();

Skip to content
BranchesTags
Repository files navigation
THOR
CI
Flexible Global Circulation Model to Explore Planetary Atmospheres
THOR is a GCM that solves the three-dimensional non-hydrostatic Euler equations on an icosahedral grid. THOR was designed to run on Graphics Processing Units (GPUs).
If you use this code please cite: Mendonça, J.M., Grimm, S.L., Grosheintz, L., & Heng, K., ApJ, 829, 115, 2016
If using version 2.0 or later, please also cite: Deitrick, R., Mendonça, J.M., Schroffenegger, U., Grimm, S.L., Tsai, S.-M., & Heng, K., ApJS, 248, 2, 2020
Current code owners: Joao Mendonca: joao.mendonca@space.dtu.dk, Russell Deitrick: russell.deitrick@csh.unibe.ch, Urs Schroffenegger: urs.schroffenegger@csh.unibe.ch
Copyright (C) 2017-2021 Exoclimes Simulation Platform
BUILD & RUN THOR (TL;DR instructions)
 $ sudo apt-get install git make gcc g++ cmake nvidia-cuda-toolkit nvidia-utils-390 libhdf5-dev libhdf5-100 libhdf5-serial-dev libhdf5-cpp-100
$ git clone https://github.com/exoclime/THOR.git
$ cd THOR
$ cp Makefile.conf.template Makefile.conf

Find the SM value of your Nvidia GPU. Decide if you want to run without any physics module empty physics module, or the one with radiative transfer, the multi module. Then open Makefile.conf in a text editor and edit like so:
 MODULES_SRC := src/physics/managers/<module_type>/
SM:=<SM value of your card> 
Set module_typeto empty (default) or multi.
Then head back to the command line and
 $ make -j8 release

Finally, run
 $ bin/esp ifile/<config file for your planet>

Furthur information
View our wiki pages here
Tutorial from ESP Summer School 2019
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Atmospheric fluid dynamics solver optimized for GPUs.
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