Presentation Open Access

A new seismic diagnostics of stellar activity cycles

Valeriy Vasilyev


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  <identifier identifierType="DOI">10.5281/zenodo.5578911</identifier>
  <creators>
    <creator>
      <creatorName>Valeriy Vasilyev</creatorName>
    </creator>
  </creators>
  <titles>
    <title>A new seismic diagnostics of  stellar activity cycles</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2021</publicationYear>
  <dates>
    <date dateType="Issued">2021-10-18</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Presentation</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/5578911</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.5575744</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/plato2021</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;&amp;nbsp;Magnetic activity affects the observed properties of solar p modes:&lt;br&gt;
mode frequencies and linewidths increase with solar activity. Using VIRGO/SPM&lt;br&gt;
data from solar cycles 23 and 24 we show that solar-cycle variations are&lt;br&gt;
measurable in the temporal autocorrelation function of the p modes. Following&lt;br&gt;
a method developed for local helioseismology, we measure the p-mode travel&lt;br&gt;
times for multiple skips and propose to average these to enhance the&lt;br&gt;
signal-to-noise ratio. This method is robust to noise, simpler to implement&lt;br&gt;
than peak bagging in the frequency domain, and promising for asteroseismology&lt;br&gt;
applications. We estimate that the activity cycles of Sun-like stars may be&lt;br&gt;
detectable in long photometric time series.&lt;/p&gt;</description>
  </descriptions>
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