Solar maximum mission experiment: Ultraviolet spectroscopy and polarimetry on the solar maximum mission
We describe the Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission (SMM) spacecraft. The instrument, which operates in the wavelength range 1150 - 3600 Å, has a spatial resolution of 2-3 arc sec and a spectral resolution of 0.02 Å FWHM in second order. A Gregorian telescope...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1981 |
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| Reproduktion: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
|---|---|
| Übergeordnetes Werk: |
in: Advances in Space Research - Amsterdam : Elsevier, 1(1981), 13, Seite 275-283 |
| Übergeordnetes Werk: |
volume:1 ; year:1981 ; number:13 ; pages:275-283 |
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NLEJ18038886X |
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| 520 | |a We describe the Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission (SMM) spacecraft. The instrument, which operates in the wavelength range 1150 - 3600 Å, has a spatial resolution of 2-3 arc sec and a spectral resolution of 0.02 Å FWHM in second order. A Gregorian telescope, focal length 1.8 m, feeds a 1 m Ebert-Fastie spectrometer. A polarimeter comprising rotating Mg F"2 waveplates can be inserted behind the spectrometer entrance slit and allows all four Stokes parameters to be determined. The observing modes include rasters, spectral scans, velocity measurements, and polarimetry. Finally, we present examples of initial observations made since launch. | ||
| 533 | |f Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 | ||
| 700 | 1 | |a Tandberg-Hanssen, E. |4 oth | |
| 700 | 1 | |a Cheng, C.C. |4 oth | |
| 700 | 1 | |a Woodgate, B.E. |4 oth | |
| 700 | 1 | |a Brandt, J.C. |4 oth | |
| 700 | 1 | |a Chapman, R.D. |4 oth | |
| 700 | 1 | |a Kenney, P.J. |4 oth | |
| 700 | 1 | |a Michalitsianos, A.G. |4 oth | |
| 700 | 1 | |a Shine, R.A. |4 oth | |
| 700 | 1 | |a Athay, R.G. |4 oth | |
| 700 | 1 | |a Beckers, J.M. |4 oth | |
| 700 | 1 | |a Bruner, E.C. |4 oth | |
| 700 | 1 | |a Rehse, R.A. |4 oth | |
| 700 | 1 | |a Schoolman, S.A. |4 oth | |
| 700 | 1 | |a Gurman, J.B. |4 oth | |
| 700 | 1 | |a Hyder, C.L. |4 oth | |
| 700 | 1 | |a Henze, W. |4 oth | |
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(DE-627)NLEJ18038886X (DE-599)GBVNLZ18038886X DE-627 ger DE-627 rakwb eng Solar maximum mission experiment: Ultraviolet spectroscopy and polarimetry on the solar maximum mission 1981 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We describe the Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission (SMM) spacecraft. The instrument, which operates in the wavelength range 1150 - 3600 Å, has a spatial resolution of 2-3 arc sec and a spectral resolution of 0.02 Å FWHM in second order. A Gregorian telescope, focal length 1.8 m, feeds a 1 m Ebert-Fastie spectrometer. A polarimeter comprising rotating Mg F"2 waveplates can be inserted behind the spectrometer entrance slit and allows all four Stokes parameters to be determined. The observing modes include rasters, spectral scans, velocity measurements, and polarimetry. Finally, we present examples of initial observations made since launch. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Tandberg-Hanssen, E. oth Cheng, C.C. oth Woodgate, B.E. oth Brandt, J.C. oth Chapman, R.D. oth Kenney, P.J. oth Michalitsianos, A.G. oth Shine, R.A. oth Athay, R.G. oth Beckers, J.M. oth Bruner, E.C. oth Rehse, R.A. oth Schoolman, S.A. oth Gurman, J.B. oth Hyder, C.L. oth Henze, W. oth in Advances in Space Research Amsterdam : Elsevier 1(1981), 13, Seite 275-283 (DE-627)NLEJ180340476 (DE-600)2023311-5 0273-1177 nnns volume:1 year:1981 number:13 pages:275-283 http://linkinghub.elsevier.com/retrieve/pii/0273-1177(81)90208-8 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 1 1981 13 275-283 |
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(DE-627)NLEJ18038886X (DE-599)GBVNLZ18038886X DE-627 ger DE-627 rakwb eng Solar maximum mission experiment: Ultraviolet spectroscopy and polarimetry on the solar maximum mission 1981 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We describe the Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission (SMM) spacecraft. The instrument, which operates in the wavelength range 1150 - 3600 Å, has a spatial resolution of 2-3 arc sec and a spectral resolution of 0.02 Å FWHM in second order. A Gregorian telescope, focal length 1.8 m, feeds a 1 m Ebert-Fastie spectrometer. A polarimeter comprising rotating Mg F"2 waveplates can be inserted behind the spectrometer entrance slit and allows all four Stokes parameters to be determined. The observing modes include rasters, spectral scans, velocity measurements, and polarimetry. Finally, we present examples of initial observations made since launch. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Tandberg-Hanssen, E. oth Cheng, C.C. oth Woodgate, B.E. oth Brandt, J.C. oth Chapman, R.D. oth Kenney, P.J. oth Michalitsianos, A.G. oth Shine, R.A. oth Athay, R.G. oth Beckers, J.M. oth Bruner, E.C. oth Rehse, R.A. oth Schoolman, S.A. oth Gurman, J.B. oth Hyder, C.L. oth Henze, W. oth in Advances in Space Research Amsterdam : Elsevier 1(1981), 13, Seite 275-283 (DE-627)NLEJ180340476 (DE-600)2023311-5 0273-1177 nnns volume:1 year:1981 number:13 pages:275-283 http://linkinghub.elsevier.com/retrieve/pii/0273-1177(81)90208-8 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 1 1981 13 275-283 |
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(DE-627)NLEJ18038886X (DE-599)GBVNLZ18038886X DE-627 ger DE-627 rakwb eng Solar maximum mission experiment: Ultraviolet spectroscopy and polarimetry on the solar maximum mission 1981 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We describe the Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission (SMM) spacecraft. The instrument, which operates in the wavelength range 1150 - 3600 Å, has a spatial resolution of 2-3 arc sec and a spectral resolution of 0.02 Å FWHM in second order. A Gregorian telescope, focal length 1.8 m, feeds a 1 m Ebert-Fastie spectrometer. A polarimeter comprising rotating Mg F"2 waveplates can be inserted behind the spectrometer entrance slit and allows all four Stokes parameters to be determined. The observing modes include rasters, spectral scans, velocity measurements, and polarimetry. Finally, we present examples of initial observations made since launch. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Tandberg-Hanssen, E. oth Cheng, C.C. oth Woodgate, B.E. oth Brandt, J.C. oth Chapman, R.D. oth Kenney, P.J. oth Michalitsianos, A.G. oth Shine, R.A. oth Athay, R.G. oth Beckers, J.M. oth Bruner, E.C. oth Rehse, R.A. oth Schoolman, S.A. oth Gurman, J.B. oth Hyder, C.L. oth Henze, W. oth in Advances in Space Research Amsterdam : Elsevier 1(1981), 13, Seite 275-283 (DE-627)NLEJ180340476 (DE-600)2023311-5 0273-1177 nnns volume:1 year:1981 number:13 pages:275-283 http://linkinghub.elsevier.com/retrieve/pii/0273-1177(81)90208-8 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 1 1981 13 275-283 |
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(DE-627)NLEJ18038886X (DE-599)GBVNLZ18038886X DE-627 ger DE-627 rakwb eng Solar maximum mission experiment: Ultraviolet spectroscopy and polarimetry on the solar maximum mission 1981 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We describe the Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission (SMM) spacecraft. The instrument, which operates in the wavelength range 1150 - 3600 Å, has a spatial resolution of 2-3 arc sec and a spectral resolution of 0.02 Å FWHM in second order. A Gregorian telescope, focal length 1.8 m, feeds a 1 m Ebert-Fastie spectrometer. A polarimeter comprising rotating Mg F"2 waveplates can be inserted behind the spectrometer entrance slit and allows all four Stokes parameters to be determined. The observing modes include rasters, spectral scans, velocity measurements, and polarimetry. Finally, we present examples of initial observations made since launch. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Tandberg-Hanssen, E. oth Cheng, C.C. oth Woodgate, B.E. oth Brandt, J.C. oth Chapman, R.D. oth Kenney, P.J. oth Michalitsianos, A.G. oth Shine, R.A. oth Athay, R.G. oth Beckers, J.M. oth Bruner, E.C. oth Rehse, R.A. oth Schoolman, S.A. oth Gurman, J.B. oth Hyder, C.L. oth Henze, W. oth in Advances in Space Research Amsterdam : Elsevier 1(1981), 13, Seite 275-283 (DE-627)NLEJ180340476 (DE-600)2023311-5 0273-1177 nnns volume:1 year:1981 number:13 pages:275-283 http://linkinghub.elsevier.com/retrieve/pii/0273-1177(81)90208-8 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 1 1981 13 275-283 |
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(DE-627)NLEJ18038886X (DE-599)GBVNLZ18038886X DE-627 ger DE-627 rakwb eng Solar maximum mission experiment: Ultraviolet spectroscopy and polarimetry on the solar maximum mission 1981 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We describe the Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission (SMM) spacecraft. The instrument, which operates in the wavelength range 1150 - 3600 Å, has a spatial resolution of 2-3 arc sec and a spectral resolution of 0.02 Å FWHM in second order. A Gregorian telescope, focal length 1.8 m, feeds a 1 m Ebert-Fastie spectrometer. A polarimeter comprising rotating Mg F"2 waveplates can be inserted behind the spectrometer entrance slit and allows all four Stokes parameters to be determined. The observing modes include rasters, spectral scans, velocity measurements, and polarimetry. Finally, we present examples of initial observations made since launch. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Tandberg-Hanssen, E. oth Cheng, C.C. oth Woodgate, B.E. oth Brandt, J.C. oth Chapman, R.D. oth Kenney, P.J. oth Michalitsianos, A.G. oth Shine, R.A. oth Athay, R.G. oth Beckers, J.M. oth Bruner, E.C. oth Rehse, R.A. oth Schoolman, S.A. oth Gurman, J.B. oth Hyder, C.L. oth Henze, W. oth in Advances in Space Research Amsterdam : Elsevier 1(1981), 13, Seite 275-283 (DE-627)NLEJ180340476 (DE-600)2023311-5 0273-1177 nnns volume:1 year:1981 number:13 pages:275-283 http://linkinghub.elsevier.com/retrieve/pii/0273-1177(81)90208-8 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 1 1981 13 275-283 |
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Solar maximum mission experiment: Ultraviolet spectroscopy and polarimetry on the solar maximum mission |
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We describe the Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission (SMM) spacecraft. The instrument, which operates in the wavelength range 1150 - 3600 Å, has a spatial resolution of 2-3 arc sec and a spectral resolution of 0.02 Å FWHM in second order. A Gregorian telescope, focal length 1.8 m, feeds a 1 m Ebert-Fastie spectrometer. A polarimeter comprising rotating Mg F"2 waveplates can be inserted behind the spectrometer entrance slit and allows all four Stokes parameters to be determined. The observing modes include rasters, spectral scans, velocity measurements, and polarimetry. Finally, we present examples of initial observations made since launch. |
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We describe the Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission (SMM) spacecraft. The instrument, which operates in the wavelength range 1150 - 3600 Å, has a spatial resolution of 2-3 arc sec and a spectral resolution of 0.02 Å FWHM in second order. A Gregorian telescope, focal length 1.8 m, feeds a 1 m Ebert-Fastie spectrometer. A polarimeter comprising rotating Mg F"2 waveplates can be inserted behind the spectrometer entrance slit and allows all four Stokes parameters to be determined. The observing modes include rasters, spectral scans, velocity measurements, and polarimetry. Finally, we present examples of initial observations made since launch. |
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We describe the Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission (SMM) spacecraft. The instrument, which operates in the wavelength range 1150 - 3600 Å, has a spatial resolution of 2-3 arc sec and a spectral resolution of 0.02 Å FWHM in second order. A Gregorian telescope, focal length 1.8 m, feeds a 1 m Ebert-Fastie spectrometer. A polarimeter comprising rotating Mg F"2 waveplates can be inserted behind the spectrometer entrance slit and allows all four Stokes parameters to be determined. The observing modes include rasters, spectral scans, velocity measurements, and polarimetry. Finally, we present examples of initial observations made since launch. |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">NLEJ18038886X</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20210706124859.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">070505s1981 xx |||||o 00| ||eng c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ18038886X</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVNLZ18038886X</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Solar maximum mission experiment: Ultraviolet spectroscopy and polarimetry on the solar maximum mission</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1981</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We describe the Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission (SMM) spacecraft. The instrument, which operates in the wavelength range 1150 - 3600 Å, has a spatial resolution of 2-3 arc sec and a spectral resolution of 0.02 Å FWHM in second order. A Gregorian telescope, focal length 1.8 m, feeds a 1 m Ebert-Fastie spectrometer. A polarimeter comprising rotating Mg F"2 waveplates can be inserted behind the spectrometer entrance slit and allows all four Stokes parameters to be determined. The observing modes include rasters, spectral scans, velocity measurements, and polarimetry. Finally, we present examples of initial observations made since launch.</subfield></datafield><datafield tag="533" ind1=" " ind2=" "><subfield code="f">Elsevier Journal Backfiles on ScienceDirect 1907 - 2002</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tandberg-Hanssen, E.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cheng, C.C.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Woodgate, B.E.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Brandt, J.C.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chapman, R.D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kenney, P.J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Michalitsianos, A.G.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shine, R.A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Athay, R.G.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Beckers, J.M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bruner, E.C.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rehse, R.A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Schoolman, S.A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Gurman, J.B.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hyder, C.L.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Henze, W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">in</subfield><subfield code="t">Advances in Space Research</subfield><subfield code="d">Amsterdam : Elsevier</subfield><subfield code="g">1(1981), 13, Seite 275-283</subfield><subfield code="w">(DE-627)NLEJ180340476</subfield><subfield code="w">(DE-600)2023311-5</subfield><subfield code="x">0273-1177</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:1</subfield><subfield code="g">year:1981</subfield><subfield code="g">number:13</subfield><subfield code="g">pages:275-283</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://linkinghub.elsevier.com/retrieve/pii/0273-1177(81)90208-8</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_H</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-1-SDJ</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_NL_ARTICLE</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">1</subfield><subfield code="j">1981</subfield><subfield code="e">13</subfield><subfield code="h">275-283</subfield></datafield></record></collection>
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