The comparison of the magnetographic magnetic field measured in different spectral lines

Measurements of the Sun's circulation, as derived from the Doppler displacements of Fraunhofer lines, are subject to error if the solar components are contaminated by weak, perhaps undetected, atmospheric blends (Livingston and Milkey, 1972). This note presents the telluric content of two spect...

Full description

Saved in:
Bibliographic Details
Published in:Solar physics 1973-08, Vol.31 (2), p.307-316
Main Authors: Gopasyuk, S. I., Kotov, V. A., Severny, A. B., Tsap, T. T.
Format: Article
Language:English
Subjects:
ASTRONOMY AND ASTROPHYSICS
PHOTOSPHERE- MAGNETIC FIELDS
SPECTRA
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c256t-45680ef65b419a7557263585ac233656bf72f4d6f6ede3c268a062509644dcdf3
cites cdi_FETCH-LOGICAL-c256t-45680ef65b419a7557263585ac233656bf72f4d6f6ede3c268a062509644dcdf3
container_end_page 316
container_issue 2
container_start_page 307
container_title Solar physics
container_volume 31
creator Gopasyuk, S. I.
Kotov, V. A.
Severny, A. B.
Tsap, T. T.
description Measurements of the Sun's circulation, as derived from the Doppler displacements of Fraunhofer lines, are subject to error if the solar components are contaminated by weak, perhaps undetected, atmospheric blends (Livingston and Milkey, 1972). This note presents the telluric content of two spectral regions of interest: the vicinity of Fe I 5233.0-- Pe I 5250.2, and Hk 6562. The threshhold of detection is considerably better than previously achieved (see, for example, Moore et al., 1966).
doi_str_mv 10.1007/BF00152808
format article
fullrecord <record><control><sourceid>crossref_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_4355940</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>10_1007_BF00152808</sourcerecordid><originalsourceid>FETCH-LOGICAL-c256t-45680ef65b419a7557263585ac233656bf72f4d6f6ede3c268a062509644dcdf3</originalsourceid><addsrcrecordid>eNpFkE9LAzEUxIMoWKsXP0HwKKxm82-zRy22CgUvFXpb0uSljewmSxIPfnu3tODpzRt-DMMgdF-Tp5qQ5vl1SUgtqCLqAs1q0bCKtGx7iWaEMHXU6hrd5Pw9URMuZmi7OQA2cRh18jkGHB0ukzPofYAS90mPB2_O7ySch97iAXT-SWCxD9h65yBBKDiPYErSPe59gHyLrpzuM9yd7xx9Ld82i_dq_bn6WLysK0OFLBUXUhFwUux43epGiIZKJpTQhjImhdy5hjpupZNggRkqlSaSCtJKzq2xjs3Rwyk35uK7bHwBczAxhKlMx5kQLScT9HiCTIo5J3DdmPyg029Xk-64RPc_HPsDztlf1w</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>The comparison of the magnetographic magnetic field measured in different spectral lines</title><source>Springer Online Journal Archives (Through 1996)</source><creator>Gopasyuk, S. I. ; Kotov, V. A. ; Severny, A. B. ; Tsap, T. T.</creator><creatorcontrib>Gopasyuk, S. I. ; Kotov, V. A. ; Severny, A. B. ; Tsap, T. T. ; Crimean Astrophysical Observatory, USSR</creatorcontrib><description>Measurements of the Sun's circulation, as derived from the Doppler displacements of Fraunhofer lines, are subject to error if the solar components are contaminated by weak, perhaps undetected, atmospheric blends (Livingston and Milkey, 1972). This note presents the telluric content of two spectral regions of interest: the vicinity of Fe I 5233.0-- Pe I 5250.2, and Hk 6562. The threshhold of detection is considerably better than previously achieved (see, for example, Moore et al., 1966).</description><identifier>ISSN: 0038-0938</identifier><identifier>EISSN: 1573-093X</identifier><identifier>DOI: 10.1007/BF00152808</identifier><language>eng</language><publisher>Springer</publisher><subject>ASTRONOMY AND ASTROPHYSICS ; PHOTOSPHERE- MAGNETIC FIELDS ; SPECTRA</subject><ispartof>Solar physics, 1973-08, Vol.31 (2), p.307-316</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c256t-45680ef65b419a7557263585ac233656bf72f4d6f6ede3c268a062509644dcdf3</citedby><cites>FETCH-LOGICAL-c256t-45680ef65b419a7557263585ac233656bf72f4d6f6ede3c268a062509644dcdf3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><backlink>$$Uhttps://www.osti.gov/biblio/4355940$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Gopasyuk, S. I.</creatorcontrib><creatorcontrib>Kotov, V. A.</creatorcontrib><creatorcontrib>Severny, A. B.</creatorcontrib><creatorcontrib>Tsap, T. T.</creatorcontrib><creatorcontrib>Crimean Astrophysical Observatory, USSR</creatorcontrib><title>The comparison of the magnetographic magnetic field measured in different spectral lines</title><title>Solar physics</title><description>Measurements of the Sun's circulation, as derived from the Doppler displacements of Fraunhofer lines, are subject to error if the solar components are contaminated by weak, perhaps undetected, atmospheric blends (Livingston and Milkey, 1972). This note presents the telluric content of two spectral regions of interest: the vicinity of Fe I 5233.0-- Pe I 5250.2, and Hk 6562. The threshhold of detection is considerably better than previously achieved (see, for example, Moore et al., 1966).</description><subject>ASTRONOMY AND ASTROPHYSICS</subject><subject>PHOTOSPHERE- MAGNETIC FIELDS</subject><subject>SPECTRA</subject><issn>0038-0938</issn><issn>1573-093X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1973</creationdate><recordtype>article</recordtype><recordid>eNpFkE9LAzEUxIMoWKsXP0HwKKxm82-zRy22CgUvFXpb0uSljewmSxIPfnu3tODpzRt-DMMgdF-Tp5qQ5vl1SUgtqCLqAs1q0bCKtGx7iWaEMHXU6hrd5Pw9URMuZmi7OQA2cRh18jkGHB0ukzPofYAS90mPB2_O7ySch97iAXT-SWCxD9h65yBBKDiPYErSPe59gHyLrpzuM9yd7xx9Ld82i_dq_bn6WLysK0OFLBUXUhFwUux43epGiIZKJpTQhjImhdy5hjpupZNggRkqlSaSCtJKzq2xjs3Rwyk35uK7bHwBczAxhKlMx5kQLScT9HiCTIo5J3DdmPyg029Xk-64RPc_HPsDztlf1w</recordid><startdate>19730801</startdate><enddate>19730801</enddate><creator>Gopasyuk, S. I.</creator><creator>Kotov, V. A.</creator><creator>Severny, A. B.</creator><creator>Tsap, T. T.</creator><general>Springer</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>19730801</creationdate><title>The comparison of the magnetographic magnetic field measured in different spectral lines</title><author>Gopasyuk, S. I. ; Kotov, V. A. ; Severny, A. B. ; Tsap, T. T.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c256t-45680ef65b419a7557263585ac233656bf72f4d6f6ede3c268a062509644dcdf3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1973</creationdate><topic>ASTRONOMY AND ASTROPHYSICS</topic><topic>PHOTOSPHERE- MAGNETIC FIELDS</topic><topic>SPECTRA</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gopasyuk, S. I.</creatorcontrib><creatorcontrib>Kotov, V. A.</creatorcontrib><creatorcontrib>Severny, A. B.</creatorcontrib><creatorcontrib>Tsap, T. T.</creatorcontrib><creatorcontrib>Crimean Astrophysical Observatory, USSR</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Solar physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gopasyuk, S. I.</au><au>Kotov, V. A.</au><au>Severny, A. B.</au><au>Tsap, T. T.</au><aucorp>Crimean Astrophysical Observatory, USSR</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The comparison of the magnetographic magnetic field measured in different spectral lines</atitle><jtitle>Solar physics</jtitle><date>1973-08-01</date><risdate>1973</risdate><volume>31</volume><issue>2</issue><spage>307</spage><epage>316</epage><pages>307-316</pages><issn>0038-0938</issn><eissn>1573-093X</eissn><abstract>Measurements of the Sun's circulation, as derived from the Doppler displacements of Fraunhofer lines, are subject to error if the solar components are contaminated by weak, perhaps undetected, atmospheric blends (Livingston and Milkey, 1972). This note presents the telluric content of two spectral regions of interest: the vicinity of Fe I 5233.0-- Pe I 5250.2, and Hk 6562. The threshhold of detection is considerably better than previously achieved (see, for example, Moore et al., 1966).</abstract><pub>Springer</pub><doi>10.1007/BF00152808</doi><tpages>10</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0038-0938
ispartof Solar physics, 1973-08, Vol.31 (2), p.307-316
issn 0038-0938
1573-093X
language eng
recordid cdi_osti_scitechconnect_4355940
source Springer Online Journal Archives (Through 1996)
subjects ASTRONOMY AND ASTROPHYSICS
PHOTOSPHERE- MAGNETIC FIELDS
SPECTRA
title The comparison of the magnetographic magnetic field measured in different spectral lines
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-03-05T19%3A07%3A58IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-crossref_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20comparison%20of%20the%20magnetographic%20magnetic%20field%20measured%20in%20different%20spectral%20lines&rft.jtitle=Solar%20physics&rft.au=Gopasyuk,%20S.%20I.&rft.aucorp=Crimean%20Astrophysical%20Observatory,%20USSR&rft.date=1973-08-01&rft.volume=31&rft.issue=2&rft.spage=307&rft.epage=316&rft.pages=307-316&rft.issn=0038-0938&rft.eissn=1573-093X&rft_id=info:doi/10.1007/BF00152808&rft_dat=%3Ccrossref_osti_%3E10_1007_BF00152808%3C/crossref_osti_%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c256t-45680ef65b419a7557263585ac233656bf72f4d6f6ede3c268a062509644dcdf3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true