Abstract
Helioseismology is a very powerful tool that allows us to explore the interior of the Sun. Here we give particular emphasis to the justification for the likely location of the zone that is most sensitive to cycle-related changes. For the low degree modes we find that more than one timescale for changes in the oscillations is discovered. We also note the successive cycles have differing sensitivities to the activity. We end with a warning of the risk of being misled with short datasets such as are seen with stellar data.
Original language | English |
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Pages (from-to) | 77-87 |
Number of pages | 11 |
Journal | Proceedings of the International Astronomical Union |
Volume | 7 |
Issue number | S286 |
DOIs | |
Publication status | Published - 1 Oct 2011 |
Event | Proceedings of the International Astronomical Union - Symposium S286 Comparative Magnetic Minima: Characterizing quiet times in the Sun and Stars - Mendoza, Argentina Duration: 3 Oct 2011 → 7 Oct 2011 |