University of St Andrews

Key information

SCOTCAT credits : 15

ECTS credits : 7

Level : SCQF level 10

Semester: 2

Availability restrictions: Not automatically available to General Degree students

Planned timetable: 11.00 am Mon (odd weeks), Wed and Fri

The object of this module is to describe the basic dynamic processes at work in the Sun, a subject which is being enlivened by dramatic new results from space missions.

Relationship to other modules

Pre-requisite(s): Before taking this module you must pass MT2506 and pass MT3504

Learning and teaching methods and delivery

Weekly contact: 2.5 lectures (x 10 weeks) and 1 tutorial (x 10 weeks).

Scheduled learning hours: 35

Guided independent study hours: 115

Assessment pattern

As used by St Andrews: 2-hour Written Examination = 100%

As defined by QAA
Written examinations : 100%
Practical examinations : 0%
Coursework: 0%

Re-assessment: Oral examination = 100%

Personnel

Module coordinator: Dr T W Elsden
Module coordinator email te55@st-andrews.ac.uk

Intended learning outcomes

• Demonstrate a basic understanding of different physical processes occurring in the Sun's atmosphere
• Demonstrate an understanding of the assumptions underlying the MHD equations and an appreciation of the different, relevant timescales
• Develop simple mathematical models based on the MHD equations to describe physical processes in the Sun's atmosphere and solve the relevant equations using standard techniques
• Demonstrate the ability to analyse and interpret mathematical results in a physically-relevant context, in particular with regard to solar applications
• Solve unseen standard problems based on the MHD equations