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Clique du Soleil
[ Clique Publications ]
Solar Physics
Researchers:
Paul Cally
Alina Donea
Jesse Andries
Diana Besliu-Ionescu
Marie Gibbon
John McCloughan
Juan Carlos Martinez Oliveros
Hamed Moradi
Shelley Hansen
The Solar Physics group at Monash University is predominantly concerned
with the local helioseismology of magnetic activity. It leads the field
in sunquake research, having discovered 15 of the 16 known quakes. A
major theme is the development of a detailed theoretical understanding
of how surface magnetism blurs our helioseismic view of the solar
interior -- the ``showerglass effect''. The group uses data from a wide
range of space and ground-based observatories, and is expert in various
numerical data analysis techniques and in numerical simulations.
Modelling of particle emission from flares and tachocline instabilities
are amongst other current interests.
Specific advances in recent years include:
- Discovery of a wide range of 2D and 3D magneto-rotational instabilities in the solar
tachocline -- the shear layer at the base of the Sun's convection zone;
- Development of a new technique using Helioseismic Holography to find and explore
sunquakes; all but one of the known quakes were discovered at Monash using this
technique;
- Discovery that magnetic field inclination is the long-sought "missing ingredient" in
understanding the absorption of helioseismic waves by sunspots;
- Development of a new Generalized Ray Theory for MHD waves in solar active regions
which allows quantitative calculation of mode conversion between magnetic and
acoustic waves in helioseismology, allowing us to understand the seismology of
magnetic activity.
CSPA Sunquake Database
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A helioseismic acoustic ray coming up underneath a sunspot in inclined magnetic
field splits into acoustic and magnetic parts at the level (horizontal line) where the
sound and Alfven speeds are equal. |
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This composite image combines EIT images from three wavelengths (171Å, 195Å and 284Å) into one that reveals solar features unique to each wavelength. Since the EIT images come to us from the spacecraft in black and white, they are color coded for easy identification. For this image, the nearly simultaneous images from May 1998 were each given a color code (red, yellow and blue) and merged into one. (Image credit: SOHO) |
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