Removing instrumental polarization from infrared solar polarimetric observations
Identifieur interne : 000773 ( Main/Exploration ); précédent : 000772; suivant : 000774Removing instrumental polarization from infrared solar polarimetric observations
Auteurs : R. Kuhn [États-Unis] ; S. Balasubramaniam [États-Unis] ; G. Kopp [États-Unis] ; J. Penn [États-Unis] ; J. Dombard [États-Unis] ; H. Lin [États-Unis]Source :
- Solar Physics [ 0038-0938 ] ; 1994-08-01.
Abstract
Abstract: Full Stokes polarimetry is obtained using the National Solar Observatory Vacuum Tower Telescope at Sacramento Peak while observing the magnetically sensitive infrared Fei line at wavelength of 1.56μ. A technique is described which makes use of the high magnetic resolution in this spectral range to remove instrumental polarization from observed StokesQ, U, andV line profiles.
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DOI: 10.1007/BF00712497
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Lin</name><affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Big Bear Solar Observatory, CalTech, Pasadena, CA</wicri:regionArea><wicri:noRegion>CA</wicri:noRegion></affiliation></author></analytic><monogr></monogr><series><title level="j">Solar Physics</title><title level="j" type="abbrev">Sol Phys</title><idno type="ISSN">0038-0938</idno><idno type="eISSN">1573-093X</idno><imprint><publisher>Springer Netherlands</publisher><pubPlace>Dordrecht</pubPlace><date type="published" when="1994-08-01">1994-08-01</date><biblScope unit="volume">153</biblScope><biblScope unit="issue">1-2</biblScope><biblScope unit="page" from="143">143</biblScope><biblScope unit="page" to="155">155</biblScope></imprint><idno type="ISSN">0038-0938</idno></series><idno type="istex">2D313A397C7D2FCD2FCAAD61F3ABAE7BDBDB5940</idno><idno type="DOI">10.1007/BF00712497</idno><idno type="ArticleID">BF00712497</idno><idno type="ArticleID">Art10</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0038-0938</idno></seriesStmt></fileDesc><profileDesc><textClass></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">Abstract: Full Stokes polarimetry is obtained using the National Solar Observatory Vacuum Tower Telescope at Sacramento Peak while observing the magnetically sensitive infrared Fei line at wavelength of 1.56μ. A technique is described which makes use of the high magnetic resolution in this spectral range to remove instrumental polarization from observed StokesQ, U, andV line profiles.</div></front></TEI><affiliations><list><country><li>États-Unis</li></country></list><tree><country name="États-Unis"><noRegion><name sortKey="Kuhn, R" sort="Kuhn, R" uniqKey="Kuhn R" first="R." last="Kuhn">R. Kuhn</name></noRegion><name sortKey="Balasubramaniam, S" sort="Balasubramaniam, S" uniqKey="Balasubramaniam S" first="S." last="Balasubramaniam">S. Balasubramaniam</name><name sortKey="Dombard, J" sort="Dombard, J" uniqKey="Dombard J" first="J." last="Dombard">J. Dombard</name><name sortKey="Kopp, G" sort="Kopp, G" uniqKey="Kopp G" first="G." last="Kopp">G. Kopp</name><name sortKey="Lin, H" sort="Lin, H" uniqKey="Lin H" first="H." last="Lin">H. Lin</name><name sortKey="Penn, J" sort="Penn, J" uniqKey="Penn J" first="J." last="Penn">J. Penn</name></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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