This course provides an introduction to the physical processes that underlie almost all astrophysical phenomena: radiation and fluid dynamics. The course is split evenly between those two topics, with an emphasis on basic physical processes rather than astrophysical applications. The radiation portion of the class covers the statistical mechanics of radiation fields, radiative transfer, plasma emission processes (free and synchotron radiation), and line formation. The fluid dynamics portion includes derivation of the theory of fluids from gas kinetics, calculation of flows in simple geometry, stability analysis, and supersonic flows and shocks. The overall goal is to provide a grounding in physics suitable for continuing research in astrophysics in more specialised classes at the undergraduate and post-graduate level.
This course can be taken as an HPO, please discuss with course convener.
Learning Outcomes
Upon successful completion, students will have the knowledge and skills to:
- Explain the physical processes of radiation emission and radiative transfer, and be able to apply these principles to solve quantitative problems using a variety of mathematical and numerical approaches;
- Explain the fluid approximation and its validity, and be able to solve quantitative problems in fluid mechanics;
- Clearly communicate the results of physical analysis in the areas of radiation and fluid dynamics;
- Work effectively as part of a group on problems in these areas.
Indicative Assessment
- 6 problem sets (60) [LO 1,2,3,4]
- final exam (40) [LO 1,2,3]
- HPO option: written report on research project (20%, LO1-4); weight of problem sets reduced to 40% (null) [LO 1,2,3,4]
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Workload
The expected workload will consist of approximately 130 hours throughout the semester including:
- Face-to face component which may consist of 2 x 2 hour lectorials per week (48 hours per semester).
- Approximately 82 hours of self directed study which will include preparation for lectures, and other assessment tasks.
Inherent Requirements
To be determined
Requisite and Incompatibility
Prescribed Texts
Radiative Processes in Astrophysics, by G. B. Rybicki and A. P. LightmanThe Physics of Astrophysics, Vol. II: Gas Dynamics, by F. H. Shu
Assumed Knowledge
Recommended: PHYS2016, PHYS2201Fees
Tuition fees are for the academic year indicated at the top of the page.
Commonwealth Support (CSP) Students
If you have been offered a Commonwealth supported place, your fees are set by the Australian Government for each course. At ANU 1 EFTSL is 48 units (normally 8 x 6-unit courses). More information about your student contribution amount for each course at Fees.
- Student Contribution Band:
- 2
- Unit value:
- 6 units
If you are a domestic graduate coursework student with a Domestic Tuition Fee (DTF) place or international student you will be required to pay course tuition fees (see below). Course tuition fees are indexed annually. Further information for domestic and international students about tuition and other fees can be found at Fees.
Where there is a unit range displayed for this course, not all unit options below may be available.
| Units | EFTSL |
|---|---|
| 6.00 | 0.12500 |
Course fees
- Domestic fee paying students
| Year | Fee |
|---|---|
| 2023 | $4320 |
- International fee paying students
| Year | Fee |
|---|---|
| 2023 | $6180 |
Offerings, Dates and Class Summary Links
ANU utilises MyTimetable to enable students to view the timetable for their enrolled courses, browse, then self-allocate to small teaching activities / tutorials so they can better plan their time. Find out more on the Timetable webpage.
Class summaries, if available, can be accessed by clicking on the View link for the relevant class number.
First Semester
| Class number | Class start date | Last day to enrol | Census date | Class end date | Mode Of Delivery | Class Summary |
|---|---|---|---|---|---|---|
| 2929 | 20 Feb 2023 | 27 Feb 2023 | 31 Mar 2023 | 26 May 2023 | In Person | View |
