
<script type="text/javascript">
<!--
document.write('<div id="oa_widget"></div>');
document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=undefined&type=result"></script>');
-->
</script>handle: 11245/1.381814
AbstractIn this review we will discuss the current standing and open questions of seismology in active stars. With the longer photometric time series data that are, and will become, available from space‐missions such asKeplerwe foresee significant progress in our understanding of stellar internal structures and processes, including interactions between them, taking place in active stars in the next few years (© 2012 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
Astrophysics - Solar and Stellar Astrophysics, FOS: Physical sciences, 530, 520, Solar and Stellar Astrophysics (astro-ph.SR)
Astrophysics - Solar and Stellar Astrophysics, FOS: Physical sciences, 530, 520, Solar and Stellar Astrophysics (astro-ph.SR)
| citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 1 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
