Computational astrophysics

Many astrophysical problems can be described (or at least approximated by) a set of equations that have analytical solution. However, more complex and realistic models usually require numerical resolution. Numerical modeling of astrophysical problems is a very powerful and commonly used tool, and it intersects with many other fields in physics and industry.
A flare at the solar limb.

A flare at the solar limb, calculated from a 3D magnetohydrodynamic simulation of the solar photosphere, chromosphere and corona. Image credits: Johan Pires Bjørgen and Jorrit Leenaarts (SU).

In this course, a selection of astrophysical problems (related to gravitation, hydrodynamics, nuclear reactions and observational data modeling) will be introduced to the students, who must implement numerical methods in a computer code in order to solve them.

The course is given during day time, and is part of the Master's programme in Astronomy. The lectures are given in English.


Teaching Format

This is a project oriented course. Introductory lectures will be given at the beginning of each project block. Afterwards, students are expected to work in their projects.


Assessment

After completing each project, the students must (individually) hand in a report and give an oral presentation.

Examiner

Jaime de la Cruz Rodriguez

The schedule will be available no later than one month before the start of the course. We do not recommend print-outs as changes can occur. At the start of the course, your department will advise where you can find your schedule during the course.


Note that the course literature can be changed up to two months before the start of the course.


Course reports are displayed for the three most recent course instances.








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