One-million Kelvin coronal loops obsered with TRACE
Lecture 1-2: Solar atmosphere: introduction.
Lecture 3: Magnetohydrodynamic (MHD) equations.
Lecture 4: Consequences of the induction equation. - 14/11/2016: added figures and sketches, fixed a misprint.
Lecture 6: Coronal loop equilibria. - 01/02/2017: a misprint under Eq. (22) is fixed.
Lecture 7: Parker's solar wind model.
Lecture 8: Potential and force-free fields.
Lecture 9-10: Prominences.
Lecture 11: Magnetic reconnection
Lecture 12-13: Solar flares.
Lecture 14: Helioseismology (Guest lecturer Dr A.-M. Broomhall)
Lecture 15: MHD seismology.
Additional material (not examinable in 2016-17)
Lecture: MHD modes of a magnetic interface.
Lecture: Oscillations in prominences.