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Solar Physics & upper-Atmosphere Research Group University of Sheffield Linear and non-linear waves and oscillations L1: Examples for waves Robert von Fáy-Siebenbürgen Robertus@sheffield.ac.uk SPARG, Department of Applied Mathematics, The University of Sheffield (UK) http://www.shef.ac.uk/~robertus
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Water waves
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Water waves
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Longitudinal waves
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Transverse waves
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Shock waves
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Sonic boom
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield The dynamic Sun Movie: SOHO/EIT (ESA/NASA)
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Helioseismology ¤ more than 100,000 pulsation modes ¤ single mode ¤ three modes ¤ many modes
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield ¤ n=14 (radial nodes) ¤ m=16 (poloidal nodes) ¤ l=20 (spherical harmonic degree) ¤ The frequency of this mode determined from the MDI data is 2935.88 0.2 µHz. Helioseismology
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Helioseismology
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Photosphere: sunspots
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Running penumbral waves
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Solar storms: Sun quakes Solar quakes: high energy electrons slam the solar surface
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Solar quakes: high energy electrons slam the solar surface Solar storms: Sun quakes
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Chromospheric spicules spicules
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Solar spicules (tornadoes) (BBSO) Earth Peter & von der Lühe (1999)
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Solar spicules (tornadoes)
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Moreton waves
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Coronal loops
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Coronal loops by TRACE
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield SOHO/TRACE examples Solar atmospheric oscillations
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield TRACE: Loop oscillation excited by M4.6 flare (14 July 1998) Movie in TRACE 171 A Solar atmospheric oscillations
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Surfing magnetic loops Difference image in brightness out from the loop base
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield Space Weather
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Solar Physics & upper-Atmosphere Research Group http://www.shef.ac.uk/~robertusKULUniversity of Sheffield The end
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