Theoretical astrophysics laboratory 3 0800-PA-THEOASTLA3
The computational projects will be realized with the aid of the magnetohydrodynamical code PIERNIK
Students perform and analyze a series of numerical experiments including: supernova explosions, accretion disks, astrophysical jets and selected hydrodynamical instabilities (gravitational instability, thermal instability, Kelvin-Helmholtz instability) of astrophysical relevance.
Total student workload
Learning outcomes - knowledge
Learning outcomes - skills
Learning outcomes - social competencies
Teaching methods
Observation/demonstration teaching methods
Exploratory teaching methods
Online teaching methods
Prerequisites
Course coordinators
Assessment criteria
Assessment methods:
Students prepare written reports on the performed experiments in the form of short articles. The learning outcomes (W1-W3, U1-U5, K1) are verified by evaluation of the reports.
Evaluation of the reports includes the following aspects:
- the level of understanding of the investigated phenomena,
- completeness and logical consistency of the experiment analysis,
- activity, initiative and independent working on numerical experiments and on the reports.
Assessment criteria:
fail: < 50%
satisfactory: 50-59%
satisfactory plus: 60-69%
good: 70-79%
good plus: 80-89%
very good: 90-100%
Practical placement
„not applicable”
Additional information
Additional information (registration calendar, class conductors, localization and schedules of classes), might be available in the USOSweb system: