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<!DOCTYPE html>
<html lang="en">
<head>
<meta charset="utf-8">
<meta name="apple-mobile-web-app-capable" content="yes" />
<meta name="apple-mobile-web-app-status-bar-style" content="black-translucent" />
<meta name="viewport" content="width=device-width, initial-scale=1.0, maximum-scale=1.0, user-scalable=no">
<title>Overview of the Trappist-1e case</title>
<meta name="author" content="Denis Sergeev" />
<!-- Bootstrap core CSS -->
<link href="page/vendor/bootstrap/css/bootstrap.min.css" rel="stylesheet">
<!-- Bootstrap custom CSS -->
<link href="page/custom.css" rel="stylesheet">
</head>
<body>
<nav class="navbar navbar-expand-lg navbar-light bg-light static-top mb-5 shadow">
<span class="navbar-text">Supplement to "Atmospheric convection plays a key role in the climate of tidally-locked terrestrial exoplanets: insights from high-resolution simulations" by Sergeev <i>et al.</i> (2020)
</span>
<div class="collapse navbar-collapse">
<ul class="navbar-nav ml-auto">
<li class="nav-item">
<a class="nav-link" href="https://doi.org/10.3847/1538-4357/ab8882">Published article</a>
</li>
<li class="nav-item">
<a class="nav-link" href="https://arxiv.org/abs/2004.03007">arXiv preprint</a>
</li>
<li class="nav-item">
<a class="nav-link" href="https://github.com/dennissergeev/exoconvection-apj-2020">Source code</a>
</li>
</ul>
</div>
</nav>
<header>
<div class="container h-100">
<div class="row h-100 align-items-center">
<div class="col-12 text-center">
<h1 class="font-weight-light">Overview of the Trappist-1e case</h1>
<p class="lead">Interactive zoom and rotatable 3D visualisation (it may take a few minutes to load)</p>
</div>
</div>
</div>
</header>
<div class="pretty container-fluid d-flex justify-content-center">
<div class="row">
<div class="col-36">
<div class="card">
<div class="card-body" align="center">
<iframe class="iframe3d col-lg-36" src="page/view_scene.html?fileURL=../plots/trap1e_grcs_110d_view3d.vtkjs"></iframe>
<div>
The <i>MassFlux</i> simulation covers the whole sphere, while the <i>HighRes</i> simulation is shown by superimposing a high-resolution grid that covers only the substellar region. The graphic shows cloud condensate (white isosurfaces), surface temperature (shading), and free troposphere wind vectors (arrows). The cloud condensate is shown using a threshold of total cloud condensate (liquid water plus ice).
</div>
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</div>
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</div>
<footer class="footer">
<div class="container">
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<div class="row text-center d-flex justify-content-center pt-5 mb-3">
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<div class="col-md-6">
<h6>
<a href="https://github.com/dennissergeev/exoconvection-apj-2020/blob/master/code/Fig01-Model-Set-Up-3D.ipynb">Code for this figure</a>
</h6>
</div>
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<div class="col-md-6">
<h6>
<a href="https://docs.pyvista.org/">Made with PyVista</a>
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