Titlebook: Differential Rotation in Sun-like Stars from Surface Variability and Asteroseismology; Martin Bo Nielsen Book 2017 Springer International

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賄賂

János Tóth,Attila László Nagy,Dávid Papp, Denmark. The final section of the chapter is a summary of the progress that has been made in the field since the publication of Nielsen et?al. (.), with respect to measuring surface differential rotation and understanding the effects of spots on the observed light curves.

征服

Book 2017to 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: asteroseismolo

向外供接觸

Book 2017 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..

容易懂得

SAGE

Discussion: Constraining Interior Rotational Shear,any radial or latitudinal differential rotation is likely small. In this section we will use forward modeling with a simple radial step rotation profile and investigate how well the above mentioned measurements can constrain such a model. This will allow us to estimate the upper limits of the radial shear at the tachocline.

SAGE

,Paper I—Rotation Periods of 12,000 Main-Sequence , Stars,, Denmark. The final section of the chapter is a summary of the progress that has been made in the field since the publication of Nielsen et?al. (.), with respect to measuring surface differential rotation and understanding the effects of spots on the observed light curves.

貧窮地活

János Tóth,Attila László Nagy,Dávid Pappally on what is currently known about radial and latitudinal differential rotation in other stars. This last section also covers rotation on the post-main-sequence as these are some of the few stars for which we have clear signs of radial differential rotation.

座右銘

ABASH

Differential Rotation in Sun-like Stars from Surface Variability and Asteroseismology978-3-319-50989-1Series ISSN 2190-5053 Series E-ISSN 2190-5061