A/Prof. Michael S. Wheatland
Sydney Institute for Astronomy
School of Physics
The University of Sydney
NSW 2006
Email: michael.wheatland@sydney.edu.au
Tel: +61 2 9351 5965
Fax: +61 2 9351 7726
My office is Rm 355 in the School of Physics

(Image credit: Bill Webster)

Teaching, research and administration
My research is mostly in solar astrophysics (the physics of events at the Sun). Specific research interests include solar flares and solar activity, the statistics of that activity, coronal magnetic fields, solar-terrestrial relations, and Bayesian probability. An up-to-date list of my publications is maintained here, and overheads for a number of recent talks are collected here. I maintain this page with recent contributions to the popular media related to my research.

I have worked on the problem of modelling magnetic fields in the Sun's corona using nonlinear force-free fields.

I currently teach PHYS 1001 Physics 1 (Mechanics), PHYS 1902 Physics 1B Advanced (Quantum), the Senior Physics Computational Physics module, and COSC 3011/3911 Scientific Computing. I have a YouTube channel (Mike's PhysFest) with clips of lecture demos and computer simulations from my Junior physics lectures.

A small sunspot region goes flare mad (Image Credit: NASA/EIT)

Various links
My Profile page on the Science Faculty's web pages
Research opportunities - Senior/Hons/PhD projects
My publications
What's new on the Sun? - solar links
Teaching-related links
Additional research links
Modeling the fall of a slinky
The double pendulum
Double square pendulum - a model for the pendulum in the SoP corridor
Solar flare prediction - a statistical method for flare prediction
Mike's PhysFest - YouTube channel with my lecture demos
Popular media stories - a scrapbook of media contributions

Modeling the fall of a slinky

Page maintained by m.wheatland@physics.usyd.edu.au Page last updated Thursday, 13-Oct-2016 05:33:43 AEDT