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Observations of magnetic fields on the Sun II

Title , AM (LMSAL, Palo Alto)
Wednesday 08 September 2004, 11:25-12:35

Seminar Room 1, Newton Institute


New and old techniques allow us to observe sunspots in a range of wavelengths, to determine the associated flow systems at a range of heights, to detect oscillations and waves and to determine the strength and angular distributions of their magnetic fields. This lecture will provide a selection of examples of processes associated with the sunspot phenomena. But rather that providing a comprehensive review, the goal of the talk is to raise questions


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