In this course you will learn about flows of neutral fluids and plasma in astrophysics.
You will study the dynamics of magnetised gases, also known as the theory of magnetohydrodynamics (MHD). Such magnetised flows are common in astrophysics, for example in the Sun and the solar wind, but also in accretion disks around stars, and in the interstellar medium. Through the course you will explore the basic equations of MHD, the different types of waves and instabilities which occur in such flows, turbulence and the dynamo effect in which magnetised flows amplify their magnetic fields. You will also apply these concepts to the Sun and other astrophysical systems.
The course is given during day time, at 50% pace. It is part of the Master’s program in Astronomy, but can also be taken as a free-standing course. The course is normally given in English.
Blackboard lectures and tutorials.
Dhrubaditya Mitra. Correspondence via the course page in Athena.
Short quizzes in class, homework and a final written exam. The final exam may be an open-book or a take-home exam.
ScheduleThis is a preliminary schedule and is subject to continuous change. For this reason, we do not recommend print-outs. At the start of the course, your institution will advise where you can find your schedule during the course.
Course literatureNote that the course literature can be changed up to two months before the start of the course.
The Physics of Fluids and Plasmas: An Introduction for Astrophysicists,
By Arnab Rai Choudhuri
Publisher:Cambridge University Press
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