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2011 (v1)Journal articleUploaded on: December 3, 2022
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2011 (v1)Journal article
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2022 (v1)Journal article
Since the asteroseismic revolution, the availability of efficient and reliable methods to extract stellar-oscillation mode parameters has been an important part of modern stellar physics. In the fields of helio- and asteroseismology, these methods are usually referred to as peakbagging. Here, we introduce the apollinaire module, a new Python 3...
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2012 (v1)Journal article
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2007 (v1)Journal article
Science, 316, pp. 1591-, http://dx.doi.org./10.1126/science.1140598
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2008 (v1)Journal article
Astronomische Nachrichten, 329, p. 476, http://dx.doi.org./10.1002/asna.200710980
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2004 (v1)Journal article
Solar Physics, 220, pp. 269-285 (2004)
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2012 (v1)Journal article
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2011 (v1)Journal article
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2011 (v1)Journal article
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April 2005 (v1)Conference paper
The solar magnetism is no more considered as a purely superficial phenomenon. The SoHO community has shown that the length of the solar cycle depends on the transition region between radiation and convection. Nevertheless, the internal solar (stellar) magnetism stays poorly known. Starting in 2008, the American instrument HMI/SDO and the...
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August 2006 (v1)Conference paper
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2013 (v1)Journal article
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Uploaded on: December 2, 2022 -
2012 (v1)Journal article
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Uploaded on: December 3, 2022