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--- seismology_overview [2024/07/15 22:49] – [Asteroseismology] jasonj
+++ seismology_overview [2024/08/02 19:32] (current) – [Helioseismology] jasonj
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-[{{:wiki:science:sun-meridional-zhao.jpg?nolink&200 |The possible structure of the meridional flows in the Sun's convection zone. Such a configuration is a puzzle for those who try to determine how the Sun generates its magnetic fields.}}]
+[{{:wiki:science:sun-meridional-zhao.jpg?direct&250 |The possible structure of the meridional flows in the Sun's convection zone. Such a configuration is a puzzle for those who try to determine how the Sun generates its magnetic fields. }}]
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 All of the above may be considered as a broad application of asteroseismic analysis of global observables. Some high-precision observations, such as those from [[http://astronomy.nmsu.edu/song-wiki/start|SONG]], will go much further than applying the scaling relations. They can provide very precise individual mode frequencies for more modes than space photometry can, including mixed modes, L=3 modes, and modes split into multiplets by internal rotation.  In fact, the relative amplitudes of the frequency multiplets can be used to measure the inclination of the stellar rotation axis {[gizon2003]}. In any case, the measured frequencies can then be confronted with the frequencies predicted from sophisticated numerical models. The result is a deeper understanding of all of the interior stellar properties and evolutionary state of stars.
+==== Giant-Planet Seismology ====
+A detailed discussion about this topic can be found on the [[jive_in_nm|JIVE]] page.
 ===== References =====