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Differential Rotation in Sun-like Stars from Surface Variability and Asteroseismology [[electronic resource] /] / by Martin Bo Nielsen



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Autore: Nielsen Martin Bo Visualizza persona
Titolo: Differential Rotation in Sun-like Stars from Surface Variability and Asteroseismology [[electronic resource] /] / by Martin Bo Nielsen Visualizza cluster
Pubblicazione: Cham : , : Springer International Publishing : , : Imprint : Springer, , 2017
Edizione: 1st ed. 2017.
Descrizione fisica: 1 online resource (XVI, 101 p. 29 illus., 18 illus. in color.)
Disciplina: 523.01
Soggetto topico: Astrophysics
Observations, Astronomical
Astronomy—Observations
Astrophysics and Astroparticles
Astronomy, Observations and Techniques
Nota di bibliografia: Includes bibliographical references and index.
Nota di contenuto: Introduction -- Rotation Periods of 12 000 Main-sequence Kepler Stars -- Rotational Splitting as a Function of Mode Frequency for Six Sunlike Stars -- Constraining Differential Rotation of Sun-like Stars from Asteroseismic and Starspot Rotation Periods -- Discussion: Constraining Interior Rotational Shear -- Appendices.
Sommario/riassunto: In his PhD dissertation Martin Bo Nielsen performs observational studies of rotation in stars like the Sun. The interior rotation in stars is thought to be one of the driving mechanisms of stellar magnetic activity, but until now this mechanism was unconstrained by observational data. NASA’s Kepler space mission provides high-precision observations of Sun-like stars which allow rotation to be inferred using two independent methods: asteroseismology measures the rotation of the stellar interior, while the brightness variability caused by features on the stellar surface trace the rotation of its outermost layers. By combining these two techniques Martin Bo Nielsen was able to place upper limits on the variation of rotation with depth in five Sun-like stars. These results suggest that the interior of other Sun-like stars also rotate in much the same way as our own Sun.
Titolo autorizzato: Differential Rotation in Sun-like Stars from Surface Variability and Asteroseismology  Visualizza cluster
ISBN: 3-319-50989-6
Formato: Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione: Inglese
Record Nr.: 9910163006203321
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Serie: Springer Theses, Recognizing Outstanding Ph.D. Research, . 2190-5053