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DTSTART;TZID=Europe/London:20190204T193000
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DTSTAMP:20190127T112146Z
CREATED:20180722T121642Z
LAST-MODIFIED:20190127T112146Z
UID:554-1549308600-1549315800@wvtest.opuselite.com
SUMMARY:Dr Leon Hicks - Sample return missions\, including Hayabusa 2 and Osiris Rex
DESCRIPTION:Dr Leon Hicks’ research focusses primarily on meteorites and samples returned by space missions\, identifying\, analysing\, and classifying them. Studying meteorites is important in understanding the origins and evolution of the Solar System.
URL:https://wvtest.opuselite.com/event/2018-19-meeting10/
LOCATION:Highfields Environmental Centre\, Boundary Way\, Penn\, Wolverhampton\, WV4 4NT\, United Kingdom
CATEGORIES:Talks
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DTSTART;TZID=Europe/London:20190218T193000
DTEND;TZID=Europe/London:20190218T213000
DTSTAMP:20190120T130044Z
CREATED:20180722T121724Z
LAST-MODIFIED:20190120T130044Z
UID:556-1550518200-1550525400@wvtest.opuselite.com
SUMMARY:Dr Andrew Gascoyne - Sunspots\, Sunquakes and Solar Storms:  An Introduction to Solar Physics
DESCRIPTION:Solar physics is the branch of astrophysics that specialises in the study of the Sun. It deals with detailed measurements that are possible only for our closest star. It intersects with many disciplines of pure physics\, astrophysics\, and computer science\, including fluid dynamics\, plasma physics including magnetohydrodynamics\, seismology\, particle physics\, atomic physics\, nuclear physics\, stellar evolution\, space physics\, spectroscopy\, radiative transfer\, applied optics\, signal processing\, computer vision\, computational physics\, stellar physics and solar astronomy. \nDr Andrew Gascoyne is a lecturer in the School of Mathematics and Computer Science at the University of Wolverhampton. Prior to that I worked as a postdoctoral research associate at The University of Sheffield on the STFC funded project entitled “Magnetic Features and Local Helioseismology”.  My research area is focused on Helioseismology\, the study of acoustic wave propagation within the interior of the Sun\, and MHD (magnetohydrodynamics) wave propagation.  Mathematical modelling is a vital part of this research in order to compare and predict observational signatures and understand the many complex mechanisms and processes involved in the interaction of the solar acoustic modes with magnetic elements on the Sun i.e.\, Sunspots and Plage regions.
URL:https://wvtest.opuselite.com/event/2018-19-meeting11/
LOCATION:Highfields Environmental Centre\, Boundary Way\, Penn\, Wolverhampton\, WV4 4NT\, United Kingdom
CATEGORIES:Talks
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