KC6033 - Solar Physics

A wide range of learning and teaching approaches are used in this module. The module is delivered using a combination of lectures and seminars. Lectures are used to introduce essential theory and to work through example problems. Seminars will be used to analyse and discuss additional example problems. Problems will be set in advance of seminars, and these are of a similar nature to the examples provided in lectures. Lectures are used to allow you to develop knowledge of two main concepts of solar physics: the Sun as a star, and the physics of the Sun. You will be introduced to unanswered questions in solar physics, such as the coronal heating problem and the formation of sunspots. You will also learn about recently resolved issues, such as neutrino production inside the Sun’s core. Seminars support this process through worked examples and virtual demonstrations using multimedia resources. You will gain greater autonomy and independence through this module and are directed to seminal references which provide a basis for further student-led exploration of the state-of-the-art knowledge base. This process helps you to develop critical thinking skills for example forming judgements on the credibility and authority of a reference. It also provides valuable sector knowledge thereby increasing students’ employability.

Students will be assessed by coursework (40%) and a formal examination (60%). Coursework (an assignment/written report) will cover one chosen topic from the syllabus, for example the solar wind. The examination will cover all topics from the module.

Formative feedback will be provided on seminar work which will include problems designed to aid your understanding.

Written feedback will be provided on the coursework. Exam feedback will provided individually and also generically to indicate where the cohort has a strong or a weaker answer to examination questions.

In addition to direct contact with the module team during lectures and seminars, you are encouraged to develop your curiosity by making direct contact with the module team either via email or the open door policy operated throughout the programme. You will also be regularly referred to supporting resources including relevant texts and multimedia relevant to the module. References to these resources will be made available through the e-learning portal and in lectures and seminars.

All modules at Northumbria include a range of reading materials that students are expected to engage with. Online reading lists (provided after enrolment) give you access to your reading material for your modules. The Library works in partnership with your module tutors to ensure you have access to the material that you need.

Knowledge & Understanding:
1. Analyse and critically evaluate the fundamental solar properties and processes, such as magnetic-plasma interactions.
2. Evaluate the Sun’s effect on the Earth.

Intellectual / Professional skills & abilities:
3. Construct and apply mathematical models of solar physical concepts, including models of the solar wind.

Personal Values Attributes (Global / Cultural awareness, Ethics, Curiosity) (PVA):
4. Manage their own learning, through knowledge of available reading sources, including advanced texts and research papers and scientific databases.
5. Effectively and concisely communicate solar physics-based ideas in written form.

SUMMATIVE
1. Coursework (40%) – 1, 2, 3, 4
2. Examination (60%) – 1, 2, 3, 5

FORMATIVE
1. Seminars KU1, KU2, KU3


Students will be assessed by coursework (40%) and a formal examination (60%). Coursework (an assignment/written report) will cover one topic from the syllabus. The examination will cover all topics from the module.

Formative feedback will be provided on seminar work which will include problems designed to aid student understanding. Written feedback will be provided on the coursework.

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In ‘Solar Physics’ you will investigate the Sun, our nearest star, as the energy powerhouse of our solar system. You will consider the physical processes of the solar interior and atmosphere, as well as learning about solar observations such as sunspots, solar flares and coronal mass ejections. This you will do by constructing and applying mathematical models to describe fundamental solar observations and processes, which include the interaction between magnetic fields and plasma (hot charged gas).

You will be attending formal lectures during which you will become conversant with solar observations and theory. A written assignment during the course will cover one aspect about the Sun and will count 40% towards the final mark. The other 60% comes from a final written examination. ‘Solar Physics’ provides you with useful preparation for employment, for example in the increasingly important space sector, or as preparation for further study.