Skip to content

Commit

Permalink
updaupdated student projects
Browse files Browse the repository at this point in the history
  • Loading branch information
Sven Kiefer committed Oct 30, 2023
1 parent 3a050e5 commit a518bc1
Showing 1 changed file with 42 additions and 1 deletion.
43 changes: 42 additions & 1 deletion outreach-teaching.html
Original file line number Diff line number Diff line change
Expand Up @@ -76,7 +76,48 @@ <h1>Teaching &amp; Outreach</h1>
<section>
<h2>Supervised projects</h2>
<button class="collapsible">
2022 &nbsp;|&nbsp; <strong>Reduction of reactions in the cluster formation of TiO2</strong>
2023 &nbsp;|&nbsp; <strong>Trajectory of cloud particles in exoplanet atmospheres</strong>
<br /><i>Open project</i>
<br /> -
<!--
<div class="collapsible-title">2021</div>
<div class="collapsible-title">
<strong>Spectral and angular differential imaging with SPHERE/IFS. Assessing the performance of various PCA-based approaches to PSF subtraction.</strong>
<br /><i>Kiefer, S. ; Bohn, A. J. ; Quanz, S. P. ; Kenworthy, M. ; Stolker, T.</i></div>
-->
<!--<ul class="collapsible-title">
<li>2021</li>
<li>Spectral and angular differential imaging with SPHERE/IFS. Assessing the performance of various PCA-based approaches to PSF subtraction.<br />Kiefer, S. ; Bohn, A. J. ; Quanz, S. P. ; Kenworthy, M. ; Stolker, T.</li>
</ul>-->
</button>
<div class="collapsible-content">
<div class="row gtr-200">
<div class="col-8 col-12-large">
<p> Clouds are present in 7 of 8 Solar System planets with the only exception being Mercury.
The cloud structure of these planets can be vastly different. Earth clouds are patchy,
Jupiter clouds from rings, and Venus is continuously covert with clouds. Similarly, we
expect a variety of cloud structures in exoplanets. Among the exoplanets, tidally locked
hot Jupiters are the best observable and belong to a class of planets unknown to our Solar
System. Their strong equatorial wind jets, hot day side, and cold night side make them
fascinating objects to study.

In this project, you will study the trajectories and timescales of cloud particles within
exoplanet atmospheres. First, you will familiarize yourself with global circulation models
(GCMs) and cloud modelling. From there, you will study the size dependent trajectory
of cloud particles within gas giant exoplanets. If time allows, you can also study the size
dependent differentiation of the cloud particles.
</div>
<div class="col-4 col-12-large">
<span class="image fit">
<a class="img">
<img src="IMG/teachingNoutreach/trajectory.jpg" alt="" />
</a>
</span>
</div>
</div>
</div>
<button class="collapsible">
2023 &nbsp;|&nbsp; <strong>Reduction of reactions in the cluster formation of TiO2</strong>
<br /><i>Bachelor Thesis of Dominik Haberz</i>
<br /><a href="docs/netred_report.pdf" target="_blank">&nearr;&nbsp;report</a>
<!--
Expand Down

0 comments on commit a518bc1

Please sign in to comment.