Changes between Version 3 and Version 4 of Talks/Fall2006/Colloquium/061004


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Timestamp:
09/15/06 12:48:25 (19 years ago)
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kvj@…
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  • Talks/Fall2006/Colloquium/061004

    v3 v4  
     1= Astronomy Colloquium / Fall 2006 =
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     3 '''October 4th''' 
     4
     5 '''Dr. Sarbani Basu'''
     6
     7 '''Yale University'''
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    19''Journey to the Centre of the Sun''
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    3 '''Sarbani Basu (Yale University)'''
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    512Helioseismology has allowed us to study the Sun in unprecedented detail. Using this tool we had been able to determine the structure of the Sun well enough to know that the solar neutrino problem did not arise because of deficiencies in solar models long before the neutrino experiments found that some of the solar neutrinos change flavour. The current thrust of helioseismology is in studying how the Sun changes over short time-scales that are related to the solar activity cycle. We now know, for example, that solar rotation rate changes with time and that the changes mimic the butterfly diagram, pointing to a link between solar dynamics and solar activity.