Waves in the radiative zones of rotating, magnetized stars
Asteroseismology has reached a level of accuracy that may allow us to detect the effect of a deep magnetic field on oscillation modes. We thus aim to develop an asymptotic theory for short-wavelength waves in radiative zones of rotating stars with a general magnetic field topology (toroidal and polo...
Gespeichert in:
| Hauptverfasser: | , , , |
|---|---|
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext bestellen |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | |
| container_start_page | |
| container_title | |
| container_volume | |
| creator | Valade, Aurélien Prat, Vincent Mathis, Stéphane Augustson, Kyle |
| description | Asteroseismology has reached a level of accuracy that may allow us to detect
the effect of a deep magnetic field on oscillation modes. We thus aim to
develop an asymptotic theory for short-wavelength waves in radiative zones of
rotating stars with a general magnetic field topology (toroidal and poloidal).
A dispersion relation is derived for a uniformly rotating star with a
low-amplitude, axisymmetric magnetic field. The parameter space of this model
is explored with a Hamiltonian ray-tracing method. The features of the
gravito-inertial waves modified by the magnetic field are studied with
different magnetic topologies. |
| doi_str_mv | 10.48550/arxiv.1810.02279 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_1810_02279</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1810_02279</sourcerecordid><originalsourceid>FETCH-LOGICAL-a679-eef7091cc19b5e04b480e8bd0fba9a6bb21f6d8938b6fd8ce10a1338f1a0be9d3</originalsourceid><addsrcrecordid>eNotj71uwjAURr0wVNAH6IQfgITrOD82WxXRUgmpC1LH6Dq-BkuQIMeKWp6-KXT6pDN8OoexFwFprooC1hi-_ZgKNQHIsko_sc0XjjRw3_F4Ih7Qeox-JH7ruwn3joc-TqQ7rvgFjx1FfyPLh4hhWLCZw_NAz_87Z4e37aHeJfvP94_6dZ9gWemEyFWgRdsKbQqC3OQKSBkLzqDG0phMuNIqLZUpnVUtCUAhpXICwZC2cs6Wj9u7fHMN_oLhp_mLaO4R8hd28kKh</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Waves in the radiative zones of rotating, magnetized stars</title><source>arXiv.org</source><creator>Valade, Aurélien ; Prat, Vincent ; Mathis, Stéphane ; Augustson, Kyle</creator><creatorcontrib>Valade, Aurélien ; Prat, Vincent ; Mathis, Stéphane ; Augustson, Kyle</creatorcontrib><description>Asteroseismology has reached a level of accuracy that may allow us to detect
the effect of a deep magnetic field on oscillation modes. We thus aim to
develop an asymptotic theory for short-wavelength waves in radiative zones of
rotating stars with a general magnetic field topology (toroidal and poloidal).
A dispersion relation is derived for a uniformly rotating star with a
low-amplitude, axisymmetric magnetic field. The parameter space of this model
is explored with a Hamiltonian ray-tracing method. The features of the
gravito-inertial waves modified by the magnetic field are studied with
different magnetic topologies.</description><identifier>DOI: 10.48550/arxiv.1810.02279</identifier><language>eng</language><subject>Physics - Solar and Stellar Astrophysics</subject><creationdate>2018-10</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,777,882</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/1810.02279$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.1810.02279$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Valade, Aurélien</creatorcontrib><creatorcontrib>Prat, Vincent</creatorcontrib><creatorcontrib>Mathis, Stéphane</creatorcontrib><creatorcontrib>Augustson, Kyle</creatorcontrib><title>Waves in the radiative zones of rotating, magnetized stars</title><description>Asteroseismology has reached a level of accuracy that may allow us to detect
the effect of a deep magnetic field on oscillation modes. We thus aim to
develop an asymptotic theory for short-wavelength waves in radiative zones of
rotating stars with a general magnetic field topology (toroidal and poloidal).
A dispersion relation is derived for a uniformly rotating star with a
low-amplitude, axisymmetric magnetic field. The parameter space of this model
is explored with a Hamiltonian ray-tracing method. The features of the
gravito-inertial waves modified by the magnetic field are studied with
different magnetic topologies.</description><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotj71uwjAURr0wVNAH6IQfgITrOD82WxXRUgmpC1LH6Dq-BkuQIMeKWp6-KXT6pDN8OoexFwFprooC1hi-_ZgKNQHIsko_sc0XjjRw3_F4Ih7Qeox-JH7ruwn3joc-TqQ7rvgFjx1FfyPLh4hhWLCZw_NAz_87Z4e37aHeJfvP94_6dZ9gWemEyFWgRdsKbQqC3OQKSBkLzqDG0phMuNIqLZUpnVUtCUAhpXICwZC2cs6Wj9u7fHMN_oLhp_mLaO4R8hd28kKh</recordid><startdate>20181004</startdate><enddate>20181004</enddate><creator>Valade, Aurélien</creator><creator>Prat, Vincent</creator><creator>Mathis, Stéphane</creator><creator>Augustson, Kyle</creator><scope>GOX</scope></search><sort><creationdate>20181004</creationdate><title>Waves in the radiative zones of rotating, magnetized stars</title><author>Valade, Aurélien ; Prat, Vincent ; Mathis, Stéphane ; Augustson, Kyle</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a679-eef7091cc19b5e04b480e8bd0fba9a6bb21f6d8938b6fd8ce10a1338f1a0be9d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Valade, Aurélien</creatorcontrib><creatorcontrib>Prat, Vincent</creatorcontrib><creatorcontrib>Mathis, Stéphane</creatorcontrib><creatorcontrib>Augustson, Kyle</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Valade, Aurélien</au><au>Prat, Vincent</au><au>Mathis, Stéphane</au><au>Augustson, Kyle</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Waves in the radiative zones of rotating, magnetized stars</atitle><date>2018-10-04</date><risdate>2018</risdate><abstract>Asteroseismology has reached a level of accuracy that may allow us to detect
the effect of a deep magnetic field on oscillation modes. We thus aim to
develop an asymptotic theory for short-wavelength waves in radiative zones of
rotating stars with a general magnetic field topology (toroidal and poloidal).
A dispersion relation is derived for a uniformly rotating star with a
low-amplitude, axisymmetric magnetic field. The parameter space of this model
is explored with a Hamiltonian ray-tracing method. The features of the
gravito-inertial waves modified by the magnetic field are studied with
different magnetic topologies.</abstract><doi>10.48550/arxiv.1810.02279</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | DOI: 10.48550/arxiv.1810.02279 |
| ispartof | |
| issn | |
| language | eng |
| recordid | cdi_arxiv_primary_1810_02279 |
| source | arXiv.org |
| subjects | Physics - Solar and Stellar Astrophysics |
| title | Waves in the radiative zones of rotating, magnetized stars |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-19T19%3A27%3A16IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Waves%20in%20the%20radiative%20zones%20of%20rotating,%20magnetized%20stars&rft.au=Valade,%20Aur%C3%A9lien&rft.date=2018-10-04&rft_id=info:doi/10.48550/arxiv.1810.02279&rft_dat=%3Carxiv_GOX%3E1810_02279%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |