“Solar” oscillator strength scale and determination of the LTE silicon abundance in the solar atmosphere

We determine LTE abundance of silicon from 65 lines of Si I using one-dimensional semiempirical models of the solar atmosphere HOLMUL, MACKKL, and VAL,C. Our list of lines is considerably larger than lists used earlier. We confirm the reliability of the oscillator strength scale of E.A. Gurtovenko a...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Kinematics and physics of celestial bodies 2012-04, Vol.28 (2), p.49-61
Hauptverfasser: Shchukina, N. G., Sukhorukov, A. V.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 61
container_issue 2
container_start_page 49
container_title Kinematics and physics of celestial bodies
container_volume 28
creator Shchukina, N. G.
Sukhorukov, A. V.
description We determine LTE abundance of silicon from 65 lines of Si I using one-dimensional semiempirical models of the solar atmosphere HOLMUL, MACKKL, and VAL,C. Our list of lines is considerably larger than lists used earlier. We confirm the reliability of the oscillator strength scale of E.A. Gurtovenko and R.I. Kostik for Si I lines that was based on the fitting to the observed solar equivalent widths. It is shown that this scale is displaced by +0.073 dex and −0.026 dex from experimental scales derived by Becker et al. and Garz, respectively. The difference between “solar” and experimental oscillator strength scales hardly depends on their lower excitation potentials, wavelengths, and equivalent widths. This difference can be interpreted as a total error caused by the choice of the one-dimensional model of atmosphere, the neglect of NLTE effects, the ignoring of the granulation, errors of the van der Waals damping constant, the microturbulence velocity, and the observed equivalent width. We study the effect of changes in various input parameters on the obtained LTE abundance of silicon and show that both the experimental scale of Becker et al. and the displaced “solar” scale produce almost the same silicon abundance. A total root-mean-square error of the abundance, which is caused by errors in equivalent widths and the microturbulence velocity, is 0.02 dex. The use of the semiclassical theory of Anstee, Barklem, and O’Mara for the description of the van der Waals damping constant leads to the emergence of a correlation of the abundance obtained from Si I lines with the equivalent width. There is no such correlation when using the classical Unsöld approximation with an enhancement factor E = 1.5. On average, differences in abundances obtained using the mentioned approximations do not exceed 0.03 dex. At E = 1.5, the LTE silicon abundance calculated using the HOLMUL model with “solar” oscillator strengths referred to the experimental scale of Becker et al. is equal to 7.594 ± 0.015, whereas the LTE silicon abundance calculated using the VAL,C model is 7.623 ± 0.021.
doi_str_mv 10.3103/S0884591312020055
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1671425734</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1014108822</sourcerecordid><originalsourceid>FETCH-LOGICAL-c382t-dd54326b4cacc4bf25f41a57ebd2b8bbc3c40abe65c4866d4592274e203bd3463</originalsourceid><addsrcrecordid>eNqFkctKAzEUhoMoWC8P4C7gxs1ornNZSqkXKLhoXQ9J5kw7ZZrUJF2480H05XwSM9aFKOLqwPm__4f_HITOKLnklPCrGSlLISvKKSOMECn30IhWXGSlIHQfjQY5G_RDdBTCKhE5q8QI9e8vrzPXK__-8oZdMF3fq-g8DtGDXcQlDkb1gJVtcAMR_LqzKnbOYtfiuAQ8nU9w6PrOpJXSW9soawB39lMMQzBWce3CZgkeTtBBq_oAp1_zGD3eTObju2z6cHs_vp5mhpcsZk0jBWe5FkYZI3TLZCuokgXohulSa8ONIEpDLo0o87xJvRkrBDDCdcNFzo_RxS53493TFkKs110wkKpZcNtQ07yggsmCi_9RQgVNx2Msoec_0JXbepuKDBSpClZJmii6o4x3IXho643v1so_J6geXlX_elXysJ0nJNYuwH9P_sv0AYJKlxc</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1010972951</pqid></control><display><type>article</type><title>“Solar” oscillator strength scale and determination of the LTE silicon abundance in the solar atmosphere</title><source>SpringerLink Journals</source><creator>Shchukina, N. G. ; Sukhorukov, A. V.</creator><creatorcontrib>Shchukina, N. G. ; Sukhorukov, A. V.</creatorcontrib><description>We determine LTE abundance of silicon from 65 lines of Si I using one-dimensional semiempirical models of the solar atmosphere HOLMUL, MACKKL, and VAL,C. Our list of lines is considerably larger than lists used earlier. We confirm the reliability of the oscillator strength scale of E.A. Gurtovenko and R.I. Kostik for Si I lines that was based on the fitting to the observed solar equivalent widths. It is shown that this scale is displaced by +0.073 dex and −0.026 dex from experimental scales derived by Becker et al. and Garz, respectively. The difference between “solar” and experimental oscillator strength scales hardly depends on their lower excitation potentials, wavelengths, and equivalent widths. This difference can be interpreted as a total error caused by the choice of the one-dimensional model of atmosphere, the neglect of NLTE effects, the ignoring of the granulation, errors of the van der Waals damping constant, the microturbulence velocity, and the observed equivalent width. We study the effect of changes in various input parameters on the obtained LTE abundance of silicon and show that both the experimental scale of Becker et al. and the displaced “solar” scale produce almost the same silicon abundance. A total root-mean-square error of the abundance, which is caused by errors in equivalent widths and the microturbulence velocity, is 0.02 dex. The use of the semiclassical theory of Anstee, Barklem, and O’Mara for the description of the van der Waals damping constant leads to the emergence of a correlation of the abundance obtained from Si I lines with the equivalent width. There is no such correlation when using the classical Unsöld approximation with an enhancement factor E = 1.5. On average, differences in abundances obtained using the mentioned approximations do not exceed 0.03 dex. At E = 1.5, the LTE silicon abundance calculated using the HOLMUL model with “solar” oscillator strengths referred to the experimental scale of Becker et al. is equal to 7.594 ± 0.015, whereas the LTE silicon abundance calculated using the VAL,C model is 7.623 ± 0.021.</description><identifier>ISSN: 0884-5913</identifier><identifier>EISSN: 1934-8401</identifier><identifier>DOI: 10.3103/S0884591312020055</identifier><language>eng</language><publisher>Heidelberg: Allerton Press, Inc</publisher><subject>Abundance ; Astronomy ; Atmosphere ; Equivalence ; Errors ; Kinematics ; Lists ; Mathematical models ; Observations and Techniques ; Oscillator strengths ; Physics ; Physics and Astronomy ; Silicon ; Solar atmosphere ; Solar Physics ; Wavelengths</subject><ispartof>Kinematics and physics of celestial bodies, 2012-04, Vol.28 (2), p.49-61</ispartof><rights>Allerton Press, Inc. 2012</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c382t-dd54326b4cacc4bf25f41a57ebd2b8bbc3c40abe65c4866d4592274e203bd3463</citedby><cites>FETCH-LOGICAL-c382t-dd54326b4cacc4bf25f41a57ebd2b8bbc3c40abe65c4866d4592274e203bd3463</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.3103/S0884591312020055$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.3103/S0884591312020055$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Shchukina, N. G.</creatorcontrib><creatorcontrib>Sukhorukov, A. V.</creatorcontrib><title>“Solar” oscillator strength scale and determination of the LTE silicon abundance in the solar atmosphere</title><title>Kinematics and physics of celestial bodies</title><addtitle>Kinemat. Phys. Celest. Bodies</addtitle><description>We determine LTE abundance of silicon from 65 lines of Si I using one-dimensional semiempirical models of the solar atmosphere HOLMUL, MACKKL, and VAL,C. Our list of lines is considerably larger than lists used earlier. We confirm the reliability of the oscillator strength scale of E.A. Gurtovenko and R.I. Kostik for Si I lines that was based on the fitting to the observed solar equivalent widths. It is shown that this scale is displaced by +0.073 dex and −0.026 dex from experimental scales derived by Becker et al. and Garz, respectively. The difference between “solar” and experimental oscillator strength scales hardly depends on their lower excitation potentials, wavelengths, and equivalent widths. This difference can be interpreted as a total error caused by the choice of the one-dimensional model of atmosphere, the neglect of NLTE effects, the ignoring of the granulation, errors of the van der Waals damping constant, the microturbulence velocity, and the observed equivalent width. We study the effect of changes in various input parameters on the obtained LTE abundance of silicon and show that both the experimental scale of Becker et al. and the displaced “solar” scale produce almost the same silicon abundance. A total root-mean-square error of the abundance, which is caused by errors in equivalent widths and the microturbulence velocity, is 0.02 dex. The use of the semiclassical theory of Anstee, Barklem, and O’Mara for the description of the van der Waals damping constant leads to the emergence of a correlation of the abundance obtained from Si I lines with the equivalent width. There is no such correlation when using the classical Unsöld approximation with an enhancement factor E = 1.5. On average, differences in abundances obtained using the mentioned approximations do not exceed 0.03 dex. At E = 1.5, the LTE silicon abundance calculated using the HOLMUL model with “solar” oscillator strengths referred to the experimental scale of Becker et al. is equal to 7.594 ± 0.015, whereas the LTE silicon abundance calculated using the VAL,C model is 7.623 ± 0.021.</description><subject>Abundance</subject><subject>Astronomy</subject><subject>Atmosphere</subject><subject>Equivalence</subject><subject>Errors</subject><subject>Kinematics</subject><subject>Lists</subject><subject>Mathematical models</subject><subject>Observations and Techniques</subject><subject>Oscillator strengths</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Silicon</subject><subject>Solar atmosphere</subject><subject>Solar Physics</subject><subject>Wavelengths</subject><issn>0884-5913</issn><issn>1934-8401</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</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>eNqFkctKAzEUhoMoWC8P4C7gxs1ornNZSqkXKLhoXQ9J5kw7ZZrUJF2480H05XwSM9aFKOLqwPm__4f_HITOKLnklPCrGSlLISvKKSOMECn30IhWXGSlIHQfjQY5G_RDdBTCKhE5q8QI9e8vrzPXK__-8oZdMF3fq-g8DtGDXcQlDkb1gJVtcAMR_LqzKnbOYtfiuAQ8nU9w6PrOpJXSW9soawB39lMMQzBWce3CZgkeTtBBq_oAp1_zGD3eTObju2z6cHs_vp5mhpcsZk0jBWe5FkYZI3TLZCuokgXohulSa8ONIEpDLo0o87xJvRkrBDDCdcNFzo_RxS53493TFkKs110wkKpZcNtQ07yggsmCi_9RQgVNx2Msoec_0JXbepuKDBSpClZJmii6o4x3IXho643v1so_J6geXlX_elXysJ0nJNYuwH9P_sv0AYJKlxc</recordid><startdate>20120401</startdate><enddate>20120401</enddate><creator>Shchukina, N. G.</creator><creator>Sukhorukov, A. V.</creator><general>Allerton Press, Inc</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>20120401</creationdate><title>“Solar” oscillator strength scale and determination of the LTE silicon abundance in the solar atmosphere</title><author>Shchukina, N. G. ; Sukhorukov, A. V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c382t-dd54326b4cacc4bf25f41a57ebd2b8bbc3c40abe65c4866d4592274e203bd3463</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Abundance</topic><topic>Astronomy</topic><topic>Atmosphere</topic><topic>Equivalence</topic><topic>Errors</topic><topic>Kinematics</topic><topic>Lists</topic><topic>Mathematical models</topic><topic>Observations and Techniques</topic><topic>Oscillator strengths</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Silicon</topic><topic>Solar atmosphere</topic><topic>Solar Physics</topic><topic>Wavelengths</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Shchukina, N. G.</creatorcontrib><creatorcontrib>Sukhorukov, A. V.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological &amp; 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 &amp; 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 &amp; Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies &amp; Aerospace Database</collection><collection>ProQuest Advanced Technologies &amp; 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>Kinematics and physics of celestial bodies</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Shchukina, N. G.</au><au>Sukhorukov, A. V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>“Solar” oscillator strength scale and determination of the LTE silicon abundance in the solar atmosphere</atitle><jtitle>Kinematics and physics of celestial bodies</jtitle><stitle>Kinemat. Phys. Celest. Bodies</stitle><date>2012-04-01</date><risdate>2012</risdate><volume>28</volume><issue>2</issue><spage>49</spage><epage>61</epage><pages>49-61</pages><issn>0884-5913</issn><eissn>1934-8401</eissn><abstract>We determine LTE abundance of silicon from 65 lines of Si I using one-dimensional semiempirical models of the solar atmosphere HOLMUL, MACKKL, and VAL,C. Our list of lines is considerably larger than lists used earlier. We confirm the reliability of the oscillator strength scale of E.A. Gurtovenko and R.I. Kostik for Si I lines that was based on the fitting to the observed solar equivalent widths. It is shown that this scale is displaced by +0.073 dex and −0.026 dex from experimental scales derived by Becker et al. and Garz, respectively. The difference between “solar” and experimental oscillator strength scales hardly depends on their lower excitation potentials, wavelengths, and equivalent widths. This difference can be interpreted as a total error caused by the choice of the one-dimensional model of atmosphere, the neglect of NLTE effects, the ignoring of the granulation, errors of the van der Waals damping constant, the microturbulence velocity, and the observed equivalent width. We study the effect of changes in various input parameters on the obtained LTE abundance of silicon and show that both the experimental scale of Becker et al. and the displaced “solar” scale produce almost the same silicon abundance. A total root-mean-square error of the abundance, which is caused by errors in equivalent widths and the microturbulence velocity, is 0.02 dex. The use of the semiclassical theory of Anstee, Barklem, and O’Mara for the description of the van der Waals damping constant leads to the emergence of a correlation of the abundance obtained from Si I lines with the equivalent width. There is no such correlation when using the classical Unsöld approximation with an enhancement factor E = 1.5. On average, differences in abundances obtained using the mentioned approximations do not exceed 0.03 dex. At E = 1.5, the LTE silicon abundance calculated using the HOLMUL model with “solar” oscillator strengths referred to the experimental scale of Becker et al. is equal to 7.594 ± 0.015, whereas the LTE silicon abundance calculated using the VAL,C model is 7.623 ± 0.021.</abstract><cop>Heidelberg</cop><pub>Allerton Press, Inc</pub><doi>10.3103/S0884591312020055</doi><tpages>13</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0884-5913
ispartof Kinematics and physics of celestial bodies, 2012-04, Vol.28 (2), p.49-61
issn 0884-5913
1934-8401
language eng
recordid cdi_proquest_miscellaneous_1671425734
source SpringerLink Journals
subjects Abundance
Astronomy
Atmosphere
Equivalence
Errors
Kinematics
Lists
Mathematical models
Observations and Techniques
Oscillator strengths
Physics
Physics and Astronomy
Silicon
Solar atmosphere
Solar Physics
Wavelengths
title “Solar” oscillator strength scale and determination of the LTE silicon abundance in the solar atmosphere
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-26T10%3A32%3A00IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=%E2%80%9CSolar%E2%80%9D%20oscillator%20strength%20scale%20and%20determination%20of%20the%20LTE%20silicon%20abundance%20in%20the%20solar%20atmosphere&rft.jtitle=Kinematics%20and%20physics%20of%20celestial%20bodies&rft.au=Shchukina,%20N.%20G.&rft.date=2012-04-01&rft.volume=28&rft.issue=2&rft.spage=49&rft.epage=61&rft.pages=49-61&rft.issn=0884-5913&rft.eissn=1934-8401&rft_id=info:doi/10.3103/S0884591312020055&rft_dat=%3Cproquest_cross%3E1014108822%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1010972951&rft_id=info:pmid/&rfr_iscdi=true