Poster Open Access
Sowmya, Krishnamurthy;
Shapiro, Alexander I.;
Witzke, Veronika;
Nèmec, Nina-E.;
Chatzistergos, Theodosis;
Yeo, Kok Leng;
Krivova, Natalie A.;
Solanki, Sami K.
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Despite the broad usage of the S-index, the link between the coverage of a stellar disk by magnetic features and Ca II H&K emission is not fully understood. In order to fill this gap we developed a physics-based model to calculate the solar S-index. To this end, we made use of the distributions of the solar magnetic features derived from the simulations of magnetic flux emergence and surface transport, together with the Ca II H&K spectra synthesized using a non-local thermodynamic equilibrium (non-LTE) radiative transfer code.</p>\n\n<p>We show that the value of the solar S-index is influenced by the inclination angle between the solar rotation axis and the observer’s line-of-sight, i.e. the solar S-index values obtained by an out-of-ecliptic observer are different from those obtained by an ecliptic-bound observer. This is important for comparing the magnetic activity of the Sun to other stars. We computed time series of the S-index as they would be observed at various inclinations dating back to 1700. We find that depending on the inclination and period of observations, the activity cycle in solar S-index can appear weaker or stronger than in stars with a solar-like level of magnetic activity. We show that there is nothing unusual about the solar chromospheric emission variations in the context of stars with near-solar magnetic activity.</p>", "contributors": [ { "type": "Editor", "name": "Wolk, Scott" } ], "title": "Modelling Solar Ca II H&K Emission Variations", "language": "eng", "relations": { "version": [ { "count": 1, "index": 0, "parent": { "pid_type": "recid", "pid_value": "4564795" }, "is_last": true, "last_child": { "pid_type": "recid", "pid_value": "4564796" } } ] }, "access_right": "open", "communities": [ { "id": "coolstars20half" } ], "grants": [ { "code": "797715", "links": { "self": "https://zenodo.org/api/grants/10.13039/501100000780::797715" }, "title": "Impact of Magnetic field on Emergent solar spectra", "acronym": "IMagE", "program": "H2020", "funder": { "doi": "10.13039/501100000780", "acronyms": [], "name": "European Commission", "links": { "self": "https://zenodo.org/api/funders/10.13039/501100000780" } } } ], "keywords": [ "The Sun and the Heliosphere", "Solar activity", "Solar chromosphere", "Stellar activity" ], "publication_date": "2021-02-26", "creators": [ { "orcid": "0000-0002-3243-1230", "affiliation": "Max Planck Institute for Solar System Research", "name": "Sowmya, Krishnamurthy" }, { "orcid": "0000-0002-8842-5403", "affiliation": "Max Planck Institute for Solar System Research", "name": "Shapiro, Alexander I." }, { "orcid": "0000-0002-0929-1612", "affiliation": "Max Planck Institute for Solar System Research", "name": "Witzke, Veronika" }, { "orcid": "0000-0001-6090-1247", "affiliation": "Max Planck Institute for Solar System Research", "name": "N\u00e8mec, Nina-E." }, { "orcid": "0000-0002-0335-9831", "affiliation": "Max Planck Institute for Solar System Research", "name": "Chatzistergos, Theodosis" }, { "orcid": "0000-0003-3851-7323", "affiliation": "Max Planck Institute for Solar System Research", "name": "Yeo, Kok Leng" }, { "orcid": "0000-0002-1377-3067", "affiliation": "Max Planck Institute for Solar System Research", "name": "Krivova, Natalie A." }, { "orcid": "0000-0002-3418-8449", "affiliation": "Max Planck Institute for Solar System Research", "name": "Solanki, Sami K." } ], "meeting": { "acronym": "CS20.5", "url": "http://coolstars20.cfa.harvard.edu/cs20half/", "dates": "March 2-4, 2021", "place": "virtually anywhere", "title": "The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun" }, "license": { "id": "CC-BY-4.0" }, "resource_type": { "type": "poster", "title": "Poster" }, "related_identifiers": [ { "scheme": "doi", "identifier": "10.5281/zenodo.4564795", "relation": "isVersionOf" } ] } }
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Data volume | 85.6 MB | 85.6 MB |
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Unique downloads | 34 | 34 |