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The Solar Activity Cycle pp 457–489Cite as

Observing Dynamos in Cool Stars

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Part of the book series: Space Sciences Series of ISSI ((SSSI,volume 53))

Abstract

The main aim of this paper is to introduce the most important observables that help us to investigate stellar dynamos and compare those to the modeling results. We give an overview of the available observational methods and data processing techniques that are suitable for such purposes, with touching upon examples of inadequate interpretations as well. Stellar observations are compared to the solar data in such a way, which ensures that the measurements are comparable in dimension, wavelength, and timescale. A brief outlook is given to the future plans and possibilities. A thorough review of this topic was published nearly a decade ago (Berdyugina in Living Rev. Sol. Phys. 2:8, 2005), now we focus on the experiences that have been gathered since that time.

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Authors and Affiliations

  1. Konkoly Observatory of the Hungarian Academy of Sciences, Konkoly Thege út 15-17, 1121, Budapest, Hungary

    Z. Kővári & K. Oláh

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  1. Z. Kővári
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Correspondence to Z. Kővári .

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  1. The Blackett Laboratory, Imperial College London, Hertfordshire, United Kingdom

    André Balogh

  2. Space Sciences Lab, University of California, Berkeley, California, USA

    Hugh Hudson

  3. Department of Astronomy, Eötvös University, Budapest, Hungary

    Kristóf Petrovay

  4. International Space Science Institute, Bern, Switzerland

    Rudolf von Steiger

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Kővári, Z., Oláh, K. (2015). Observing Dynamos in Cool Stars. In: Balogh, A., Hudson, H., Petrovay, K., von Steiger, R. (eds) The Solar Activity Cycle. Space Sciences Series of ISSI, vol 53. Springer, New York, NY. https://doi.org/10.1007/978-1-4939-2584-1_16

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