Multiple Scattering of Seismic Waves from Ensembles of Upwardly Lossy Thin Flux Tubes
Our previous semi-analytic treatment of f - and p -mode multiple scattering from ensembles of thin flux tubes (Hanson and Cally, Astrophys. J. 781 , 125, 2014a ; 791 , 129, 2014b ) is extended by allowing both sausage and kink waves to freely escape at the top of the model using a radiative boundary...
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| Veröffentlicht in: | Solar physics 2015-07, Vol.290 (7), p.1889-1896 |
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| container_title | Solar physics |
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| creator | Hanson, Chris S. Cally, Paul S. |
| description | Our previous semi-analytic treatment of
f
- and
p
-mode multiple scattering from ensembles of thin flux tubes (Hanson and Cally,
Astrophys. J.
781
, 125,
2014a
;
791
, 129,
2014b
) is extended by allowing both sausage and kink waves to freely escape at the top of the model using a radiative boundary condition there. As expected, this additional avenue of escape, supplementing downward loss into the deep solar interior, results in substantially greater absorption of incident
f
- and
p
-modes. However, less intuitively, it also yields mildly to substantially smaller phase shifts in waves emerging from the ensemble. This may have implications for the interpretation of seismic data for solar plage regions, and in particular their small measured phase shifts. |
| doi_str_mv | 10.1007/s11207-015-0732-x |
| format | Article |
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f
- and
p
-mode multiple scattering from ensembles of thin flux tubes (Hanson and Cally,
Astrophys. J.
781
, 125,
2014a
;
791
, 129,
2014b
) is extended by allowing both sausage and kink waves to freely escape at the top of the model using a radiative boundary condition there. As expected, this additional avenue of escape, supplementing downward loss into the deep solar interior, results in substantially greater absorption of incident
f
- and
p
-modes. However, less intuitively, it also yields mildly to substantially smaller phase shifts in waves emerging from the ensemble. This may have implications for the interpretation of seismic data for solar plage regions, and in particular their small measured phase shifts.</description><identifier>ISSN: 0038-0938</identifier><identifier>EISSN: 1573-093X</identifier><identifier>DOI: 10.1007/s11207-015-0732-x</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Astrophysics and Astroparticles ; Atmospheric Sciences ; Boundary conditions ; Flux ; Phase shift ; Physics ; Physics and Astronomy ; Scattering ; Seismic waves ; Solar interior ; Solar physics ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Texts ; Theory ; Tubes</subject><ispartof>Solar physics, 2015-07, Vol.290 (7), p.1889-1896</ispartof><rights>Springer Science+Business Media Dordrecht 2015</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c452t-edd16a3ea1cd48d62eca3267656c8bb1444d8f95add19fcecd818ed16345a6133</citedby><cites>FETCH-LOGICAL-c452t-edd16a3ea1cd48d62eca3267656c8bb1444d8f95add19fcecd818ed16345a6133</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11207-015-0732-x$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11207-015-0732-x$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>315,781,785,27929,27930,41493,42562,51324</link.rule.ids></links><search><creatorcontrib>Hanson, Chris S.</creatorcontrib><creatorcontrib>Cally, Paul S.</creatorcontrib><title>Multiple Scattering of Seismic Waves from Ensembles of Upwardly Lossy Thin Flux Tubes</title><title>Solar physics</title><addtitle>Sol Phys</addtitle><description>Our previous semi-analytic treatment of
f
- and
p
-mode multiple scattering from ensembles of thin flux tubes (Hanson and Cally,
Astrophys. J.
781
, 125,
2014a
;
791
, 129,
2014b
) is extended by allowing both sausage and kink waves to freely escape at the top of the model using a radiative boundary condition there. As expected, this additional avenue of escape, supplementing downward loss into the deep solar interior, results in substantially greater absorption of incident
f
- and
p
-modes. However, less intuitively, it also yields mildly to substantially smaller phase shifts in waves emerging from the ensemble. This may have implications for the interpretation of seismic data for solar plage regions, and in particular their small measured phase shifts.</description><subject>Astrophysics and Astroparticles</subject><subject>Atmospheric Sciences</subject><subject>Boundary conditions</subject><subject>Flux</subject><subject>Phase shift</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Scattering</subject><subject>Seismic waves</subject><subject>Solar interior</subject><subject>Solar physics</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Texts</subject><subject>Theory</subject><subject>Tubes</subject><issn>0038-0938</issn><issn>1573-093X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNqNkU9LwzAYh4MoOKcfwFvAi5dq3qZt0qOMTYWJh23oLWTpW-3oP5NWt29v6jyIIHhKQp7nhff3I-Qc2BUwJq4dQMhEwCAOmOBhsD0gI4gFD1jKnw_JiDEuh7s8JifObRgbrHhEVg992RVtiXRhdNehLeoX2uR0gYWrCkOf9Ds6mtumotPaYbUu_dP_r9oPbbNyR-eNczu6fC1qOiv7LV32a3Sn5CjXpcOz73NMVrPpcnIXzB9v7yc388BEcdgFmGWQaI4aTBbJLAnRaB4mIokTI9driKIok3kaa8-luUGTSZDoHR7FOgHOx-RyP7e1zVuPrlNV4QyWpa6x6Z0CEUVJmkoQ_0AhFCKEL_TiF7ppelv7RTzlc0w5yIGCPWWsj8BirlpbVNruFDA1pKv2nSjfiRo6UVvvhHvHtUPQaH9M_lP6BHa7jsE</recordid><startdate>20150701</startdate><enddate>20150701</enddate><creator>Hanson, Chris S.</creator><creator>Cally, Paul S.</creator><general>Springer Netherlands</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>20150701</creationdate><title>Multiple Scattering of Seismic Waves from Ensembles of Upwardly Lossy Thin Flux Tubes</title><author>Hanson, Chris S. ; Cally, Paul S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c452t-edd16a3ea1cd48d62eca3267656c8bb1444d8f95add19fcecd818ed16345a6133</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Astrophysics and Astroparticles</topic><topic>Atmospheric Sciences</topic><topic>Boundary conditions</topic><topic>Flux</topic><topic>Phase shift</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Scattering</topic><topic>Seismic waves</topic><topic>Solar interior</topic><topic>Solar physics</topic><topic>Space Exploration and Astronautics</topic><topic>Space Sciences (including Extraterrestrial Physics</topic><topic>Texts</topic><topic>Theory</topic><topic>Tubes</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hanson, Chris S.</creatorcontrib><creatorcontrib>Cally, Paul S.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><jtitle>Solar physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hanson, Chris S.</au><au>Cally, Paul S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Multiple Scattering of Seismic Waves from Ensembles of Upwardly Lossy Thin Flux Tubes</atitle><jtitle>Solar physics</jtitle><stitle>Sol Phys</stitle><date>2015-07-01</date><risdate>2015</risdate><volume>290</volume><issue>7</issue><spage>1889</spage><epage>1896</epage><pages>1889-1896</pages><issn>0038-0938</issn><eissn>1573-093X</eissn><abstract>Our previous semi-analytic treatment of
f
- and
p
-mode multiple scattering from ensembles of thin flux tubes (Hanson and Cally,
Astrophys. J.
781
, 125,
2014a
;
791
, 129,
2014b
) is extended by allowing both sausage and kink waves to freely escape at the top of the model using a radiative boundary condition there. As expected, this additional avenue of escape, supplementing downward loss into the deep solar interior, results in substantially greater absorption of incident
f
- and
p
-modes. However, less intuitively, it also yields mildly to substantially smaller phase shifts in waves emerging from the ensemble. This may have implications for the interpretation of seismic data for solar plage regions, and in particular their small measured phase shifts.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s11207-015-0732-x</doi><tpages>8</tpages></addata></record> |
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| issn | 0038-0938 1573-093X |
| language | eng |
| recordid | cdi_proquest_miscellaneous_1744699817 |
| source | SpringerNature Journals |
| subjects | Astrophysics and Astroparticles Atmospheric Sciences Boundary conditions Flux Phase shift Physics Physics and Astronomy Scattering Seismic waves Solar interior Solar physics Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Texts Theory Tubes |
| title | Multiple Scattering of Seismic Waves from Ensembles of Upwardly Lossy Thin Flux Tubes |
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