Journal
SPACE SCIENCE REVIEWS
Volume 186, Issue 1-4, Pages 437-456Publisher
SPRINGER
DOI: 10.1007/s11214-014-0090-2
Keywords
Stars: activity; Stars: oscillations
Categories
Funding
- UK Science and Technology Facilities Council (STFC)
- Danish National Research Foundation
- NSF [AST-1105930]
- NASA [NNX13AE70G]
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1105930] Funding Source: National Science Foundation
- NASA [475132, NNX13AE70G] Funding Source: Federal RePORTER
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The solar activity cycle can be studied using many different types of observations, such as counting sunspots, measuring emission in the Ca II H&K lines, magnetograms, radio emissions, etc. One of the more recent ways of studying solar activity is to use the changing properties of solar oscillations. Stellar activity cycles are generally studied using the Ca II lines, or sometimes using photometry. Asteroseismology is potentially an exciting means of studying these cycles. In this article we examine whether or not asteroseismic data can be used for this purpose, and what the asteroseismic signatures of stellar activity are. We also examine how asteroseismology may help in more indirect ways.
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