The Ultraviolet Spectrometer and Polarimeter on the Solar Maximum Mission
Abstract The Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission spacecraft is described, including the experiment objectives, system design, performance, and modes of operation. The instrument operates in the wavelength range 1150–3600 Å with better than 2 arc sec spatial r...
Ausführliche Beschreibung
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1980 |
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| Umfang: |
18 |
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| Reproduktion: |
Springer Online Journal Archives 1860-2002 |
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| Übergeordnetes Werk: |
in: Solar physics - 1967, 65(1980) vom: Jan., Seite 73-90 |
| Übergeordnetes Werk: |
volume:65 ; year:1980 ; month:01 ; pages:73-90 ; extent:18 |
| Links: |
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NLEJ195894405 |
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| 520 | |a Abstract The Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission spacecraft is described, including the experiment objectives, system design, performance, and modes of operation. The instrument operates in the wavelength range 1150–3600 Å with better than 2 arc sec spatial resolution, raster range 256 × 256 arc sec2, and 20 mÅ spectral resolution in second order. Observations can be made with specific sets of 4 lines simultaneously, or with both sides of 2 lines simultaneously for velocity and polarization. A rotatable retarder can be inserted into the spectrometer beam for measurement of Zeeman splitting and linear polarization in the transition region and chromosphere. | ||
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| 700 | 1 | |a Woodgate, B. E. |4 oth | |
| 700 | 1 | |a Tandberg-Hanssen, E. A. |4 oth | |
| 700 | 1 | |a Bruner, E. C. |4 oth | |
| 700 | 1 | |a Beckers, J. M. |4 oth | |
| 700 | 1 | |a Brandt, J. C. |4 oth | |
| 700 | 1 | |a Henze, W. |4 oth | |
| 700 | 1 | |a Hyder, C. L. |4 oth | |
| 700 | 1 | |a Kalet, M. W. |4 oth | |
| 700 | 1 | |a Kenny, P. J. |4 oth | |
| 700 | 1 | |a Knox, E. D. |4 oth | |
| 700 | 1 | |a Michalitsianos, A. G. |4 oth | |
| 700 | 1 | |a Rehse, R. |4 oth | |
| 700 | 1 | |a Shine, R. A. |4 oth | |
| 700 | 1 | |a Tinsley, H. D. |4 oth | |
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(DE-627)NLEJ195894405 DE-627 ger DE-627 rakwb eng The Ultraviolet Spectrometer and Polarimeter on the Solar Maximum Mission 1980 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission spacecraft is described, including the experiment objectives, system design, performance, and modes of operation. The instrument operates in the wavelength range 1150–3600 Å with better than 2 arc sec spatial resolution, raster range 256 × 256 arc sec2, and 20 mÅ spectral resolution in second order. Observations can be made with specific sets of 4 lines simultaneously, or with both sides of 2 lines simultaneously for velocity and polarization. A rotatable retarder can be inserted into the spectrometer beam for measurement of Zeeman splitting and linear polarization in the transition region and chromosphere. Springer Online Journal Archives 1860-2002 Woodgate, B. E. oth Tandberg-Hanssen, E. A. oth Bruner, E. C. oth Beckers, J. M. oth Brandt, J. C. oth Henze, W. oth Hyder, C. L. oth Kalet, M. W. oth Kenny, P. J. oth Knox, E. D. oth Michalitsianos, A. G. oth Rehse, R. oth Shine, R. A. oth Tinsley, H. D. oth in Solar physics 1967 65(1980) vom: Jan., Seite 73-90 (DE-627)NLEJ188983465 (DE-600)1473830-2 1573-093X nnns volume:65 year:1980 month:01 pages:73-90 extent:18 http://dx.doi.org/10.1007/BF00151385 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 65 1980 1 73-90 18 |
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(DE-627)NLEJ195894405 DE-627 ger DE-627 rakwb eng The Ultraviolet Spectrometer and Polarimeter on the Solar Maximum Mission 1980 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission spacecraft is described, including the experiment objectives, system design, performance, and modes of operation. The instrument operates in the wavelength range 1150–3600 Å with better than 2 arc sec spatial resolution, raster range 256 × 256 arc sec2, and 20 mÅ spectral resolution in second order. Observations can be made with specific sets of 4 lines simultaneously, or with both sides of 2 lines simultaneously for velocity and polarization. A rotatable retarder can be inserted into the spectrometer beam for measurement of Zeeman splitting and linear polarization in the transition region and chromosphere. Springer Online Journal Archives 1860-2002 Woodgate, B. E. oth Tandberg-Hanssen, E. A. oth Bruner, E. C. oth Beckers, J. M. oth Brandt, J. C. oth Henze, W. oth Hyder, C. L. oth Kalet, M. W. oth Kenny, P. J. oth Knox, E. D. oth Michalitsianos, A. G. oth Rehse, R. oth Shine, R. A. oth Tinsley, H. D. oth in Solar physics 1967 65(1980) vom: Jan., Seite 73-90 (DE-627)NLEJ188983465 (DE-600)1473830-2 1573-093X nnns volume:65 year:1980 month:01 pages:73-90 extent:18 http://dx.doi.org/10.1007/BF00151385 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 65 1980 1 73-90 18 |
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(DE-627)NLEJ195894405 DE-627 ger DE-627 rakwb eng The Ultraviolet Spectrometer and Polarimeter on the Solar Maximum Mission 1980 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission spacecraft is described, including the experiment objectives, system design, performance, and modes of operation. The instrument operates in the wavelength range 1150–3600 Å with better than 2 arc sec spatial resolution, raster range 256 × 256 arc sec2, and 20 mÅ spectral resolution in second order. Observations can be made with specific sets of 4 lines simultaneously, or with both sides of 2 lines simultaneously for velocity and polarization. A rotatable retarder can be inserted into the spectrometer beam for measurement of Zeeman splitting and linear polarization in the transition region and chromosphere. Springer Online Journal Archives 1860-2002 Woodgate, B. E. oth Tandberg-Hanssen, E. A. oth Bruner, E. C. oth Beckers, J. M. oth Brandt, J. C. oth Henze, W. oth Hyder, C. L. oth Kalet, M. W. oth Kenny, P. J. oth Knox, E. D. oth Michalitsianos, A. G. oth Rehse, R. oth Shine, R. A. oth Tinsley, H. D. oth in Solar physics 1967 65(1980) vom: Jan., Seite 73-90 (DE-627)NLEJ188983465 (DE-600)1473830-2 1573-093X nnns volume:65 year:1980 month:01 pages:73-90 extent:18 http://dx.doi.org/10.1007/BF00151385 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 65 1980 1 73-90 18 |
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(DE-627)NLEJ195894405 DE-627 ger DE-627 rakwb eng The Ultraviolet Spectrometer and Polarimeter on the Solar Maximum Mission 1980 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission spacecraft is described, including the experiment objectives, system design, performance, and modes of operation. The instrument operates in the wavelength range 1150–3600 Å with better than 2 arc sec spatial resolution, raster range 256 × 256 arc sec2, and 20 mÅ spectral resolution in second order. Observations can be made with specific sets of 4 lines simultaneously, or with both sides of 2 lines simultaneously for velocity and polarization. A rotatable retarder can be inserted into the spectrometer beam for measurement of Zeeman splitting and linear polarization in the transition region and chromosphere. Springer Online Journal Archives 1860-2002 Woodgate, B. E. oth Tandberg-Hanssen, E. A. oth Bruner, E. C. oth Beckers, J. M. oth Brandt, J. C. oth Henze, W. oth Hyder, C. L. oth Kalet, M. W. oth Kenny, P. J. oth Knox, E. D. oth Michalitsianos, A. G. oth Rehse, R. oth Shine, R. A. oth Tinsley, H. D. oth in Solar physics 1967 65(1980) vom: Jan., Seite 73-90 (DE-627)NLEJ188983465 (DE-600)1473830-2 1573-093X nnns volume:65 year:1980 month:01 pages:73-90 extent:18 http://dx.doi.org/10.1007/BF00151385 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 65 1980 1 73-90 18 |
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(DE-627)NLEJ195894405 DE-627 ger DE-627 rakwb eng The Ultraviolet Spectrometer and Polarimeter on the Solar Maximum Mission 1980 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission spacecraft is described, including the experiment objectives, system design, performance, and modes of operation. The instrument operates in the wavelength range 1150–3600 Å with better than 2 arc sec spatial resolution, raster range 256 × 256 arc sec2, and 20 mÅ spectral resolution in second order. Observations can be made with specific sets of 4 lines simultaneously, or with both sides of 2 lines simultaneously for velocity and polarization. A rotatable retarder can be inserted into the spectrometer beam for measurement of Zeeman splitting and linear polarization in the transition region and chromosphere. Springer Online Journal Archives 1860-2002 Woodgate, B. E. oth Tandberg-Hanssen, E. A. oth Bruner, E. C. oth Beckers, J. M. oth Brandt, J. C. oth Henze, W. oth Hyder, C. L. oth Kalet, M. W. oth Kenny, P. J. oth Knox, E. D. oth Michalitsianos, A. G. oth Rehse, R. oth Shine, R. A. oth Tinsley, H. D. oth in Solar physics 1967 65(1980) vom: Jan., Seite 73-90 (DE-627)NLEJ188983465 (DE-600)1473830-2 1573-093X nnns volume:65 year:1980 month:01 pages:73-90 extent:18 http://dx.doi.org/10.1007/BF00151385 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 65 1980 1 73-90 18 |
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in Solar physics 65(1980) vom: Jan., Seite 73-90 volume:65 year:1980 month:01 pages:73-90 extent:18 |
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Abstract The Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission spacecraft is described, including the experiment objectives, system design, performance, and modes of operation. The instrument operates in the wavelength range 1150–3600 Å with better than 2 arc sec spatial resolution, raster range 256 × 256 arc sec2, and 20 mÅ spectral resolution in second order. Observations can be made with specific sets of 4 lines simultaneously, or with both sides of 2 lines simultaneously for velocity and polarization. A rotatable retarder can be inserted into the spectrometer beam for measurement of Zeeman splitting and linear polarization in the transition region and chromosphere. |
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Abstract The Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission spacecraft is described, including the experiment objectives, system design, performance, and modes of operation. The instrument operates in the wavelength range 1150–3600 Å with better than 2 arc sec spatial resolution, raster range 256 × 256 arc sec2, and 20 mÅ spectral resolution in second order. Observations can be made with specific sets of 4 lines simultaneously, or with both sides of 2 lines simultaneously for velocity and polarization. A rotatable retarder can be inserted into the spectrometer beam for measurement of Zeeman splitting and linear polarization in the transition region and chromosphere. |
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Abstract The Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission spacecraft is described, including the experiment objectives, system design, performance, and modes of operation. The instrument operates in the wavelength range 1150–3600 Å with better than 2 arc sec spatial resolution, raster range 256 × 256 arc sec2, and 20 mÅ spectral resolution in second order. Observations can be made with specific sets of 4 lines simultaneously, or with both sides of 2 lines simultaneously for velocity and polarization. A rotatable retarder can be inserted into the spectrometer beam for measurement of Zeeman splitting and linear polarization in the transition region and chromosphere. |
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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">NLEJ195894405</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20210708015232.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">070526s1980 xx |||||o 00| ||eng c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ195894405</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">The Ultraviolet Spectrometer and Polarimeter on the Solar Maximum Mission</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1980</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">18</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">Abstract The Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission spacecraft is described, including the experiment objectives, system design, performance, and modes of operation. The instrument operates in the wavelength range 1150–3600 Å with better than 2 arc sec spatial resolution, raster range 256 × 256 arc sec2, and 20 mÅ spectral resolution in second order. Observations can be made with specific sets of 4 lines simultaneously, or with both sides of 2 lines simultaneously for velocity and polarization. A rotatable retarder can be inserted into the spectrometer beam for measurement of Zeeman splitting and linear polarization in the transition region and chromosphere.</subfield></datafield><datafield tag="533" ind1=" " ind2=" "><subfield code="f">Springer Online Journal Archives 1860-2002</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">Tandberg-Hanssen, E. A.</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">Beckers, J. M.</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">Henze, W.</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">Kalet, M. W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kenny, P. J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Knox, E. D.</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">Rehse, R.</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">Tinsley, H. D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">in</subfield><subfield code="t">Solar physics</subfield><subfield code="d">1967</subfield><subfield code="g">65(1980) vom: Jan., Seite 73-90</subfield><subfield code="w">(DE-627)NLEJ188983465</subfield><subfield code="w">(DE-600)1473830-2</subfield><subfield code="x">1573-093X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:65</subfield><subfield code="g">year:1980</subfield><subfield code="g">month:01</subfield><subfield code="g">pages:73-90</subfield><subfield code="g">extent:18</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://dx.doi.org/10.1007/BF00151385</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-1-SOJ</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">65</subfield><subfield code="j">1980</subfield><subfield code="c">1</subfield><subfield code="h">73-90</subfield><subfield code="g">18</subfield></datafield></record></collection>
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