Picard SODISM, a Space Telescope to Study the Sun from the Middle Ultraviolet to the Near Infrared
The Solar Diameter Imager and Surface Mapper (SODISM) onboard the Picard space mission provides wide-field images of the photosphere and chromosphere of the Sun in five narrow bandpasses centered at 215.0, 393.37, 535.7, 607.1, and 782.2 nm. The Picard spacecraft was successfully launched on 15 June...
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| Veröffentlicht in: | Solar physics 2014-03, Vol.289 (3), p.1043-1076 |
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| creator | Meftah, M. Hochedez, J.-F. Irbah, A. Hauchecorne, A. Boumier, P. Corbard, T. Turck-Chièze, S. Abbaki, S. Assus, P. Bertran, E. Bourget, P. Buisson, F. Chaigneau, M. Damé, L. Djafer, D. Dufour, C. Etcheto, P. Ferrero, P. Hersé, M. Marcovici, J.-P. Meissonnier, M. Morand, F. Poiet, G. Prado, J.-Y. Renaud, C. Rouanet, N. Rouzé, M. Salabert, D. Vieau, A.-J. |
| description | The
Solar Diameter Imager and Surface Mapper
(SODISM) onboard the
Picard
space mission provides wide-field images of the photosphere and chromosphere of the Sun in five narrow bandpasses centered at 215.0, 393.37, 535.7, 607.1, and 782.2 nm. The
Picard
spacecraft was successfully launched on 15 June 2010 into a Sun-synchronous dawn–dusk orbit. The
Picard
space mission represents a European asset in collecting solar observations useful to improve Earth climatic models. The scientific payload consists of the SODISM imager and of two radiometers,
SOlar VAriability Picard
(SOVAP) and
PREcision MOnitor Sensor
(PREMOS), which measure the Total Solar Irradiance (TSI) and part of the Solar Spectral Irradiance (SSI).
The SODISM telescope continuously monitors solar activity from the middle ultraviolet to the near infrared spectral ranges and produces solar images that feed SSI reconstruction models. Further, SODISM probes the solar interior
via
a helioseismic analysis of the solar disc and limb images at 535.7 nm, and
via
astrometric investigations at the limb. The latter allows us to deduce the spectral dependence of the solar limb profile, and the asphericity of the Sun. Furthermore, SODISM data taken during the transit of Venus allow a determination of the absolute value of the solar diameter. This paper provides a detailed description of the SODISM instrument, including thermo-optical analysis, its different modes of observation, and its first performance in space. |
| doi_str_mv | 10.1007/s11207-013-0373-x |
| format | Article |
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Solar Diameter Imager and Surface Mapper
(SODISM) onboard the
Picard
space mission provides wide-field images of the photosphere and chromosphere of the Sun in five narrow bandpasses centered at 215.0, 393.37, 535.7, 607.1, and 782.2 nm. The
Picard
spacecraft was successfully launched on 15 June 2010 into a Sun-synchronous dawn–dusk orbit. The
Picard
space mission represents a European asset in collecting solar observations useful to improve Earth climatic models. The scientific payload consists of the SODISM imager and of two radiometers,
SOlar VAriability Picard
(SOVAP) and
PREcision MOnitor Sensor
(PREMOS), which measure the Total Solar Irradiance (TSI) and part of the Solar Spectral Irradiance (SSI).
The SODISM telescope continuously monitors solar activity from the middle ultraviolet to the near infrared spectral ranges and produces solar images that feed SSI reconstruction models. Further, SODISM probes the solar interior
via
a helioseismic analysis of the solar disc and limb images at 535.7 nm, and
via
astrometric investigations at the limb. The latter allows us to deduce the spectral dependence of the solar limb profile, and the asphericity of the Sun. Furthermore, SODISM data taken during the transit of Venus allow a determination of the absolute value of the solar diameter. This paper provides a detailed description of the SODISM instrument, including thermo-optical analysis, its different modes of observation, and its first performance in space.</description><identifier>ISSN: 0038-0938</identifier><identifier>EISSN: 1573-093X</identifier><identifier>DOI: 10.1007/s11207-013-0373-x</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Astrophysics ; Astrophysics and Astroparticles ; Atmospheric Sciences ; Infrared radiation ; Instrumentation and Methods for Astrophysic ; Irradiance ; Monitors ; Optical analysis ; Physics ; Physics and Astronomy ; Sciences of the Universe ; Solar activity ; Solar and Stellar Astrophysics ; Solar diameter ; Solar physics ; Space Exploration and Astronautics ; Space missions ; Space Sciences (including Extraterrestrial Physics ; Space telescopes ; Spacecraft ; Spectra ; Sun ; Ultraviolet ; Ultraviolet radiation</subject><ispartof>Solar physics, 2014-03, Vol.289 (3), p.1043-1076</ispartof><rights>Springer Science+Business Media Dordrecht 2013</rights><rights>Springer Science+Business Media Dordrecht 2014</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c416t-ce06dd9f43a9f51db1a54f5728d5337af1f27ac0f36504dd2bb5ea57e16ba7313</citedby><cites>FETCH-LOGICAL-c416t-ce06dd9f43a9f51db1a54f5728d5337af1f27ac0f36504dd2bb5ea57e16ba7313</cites><orcidid>0000-0001-8990-2526 ; 0000-0002-0168-987X ; 0000-0003-3265-3148 ; 0000-0002-9615-9619</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11207-013-0373-x$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11207-013-0373-x$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>230,314,776,780,881,27901,27902,41464,42533,51294</link.rule.ids><backlink>$$Uhttps://hal.science/hal-00796903$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Meftah, M.</creatorcontrib><creatorcontrib>Hochedez, J.-F.</creatorcontrib><creatorcontrib>Irbah, A.</creatorcontrib><creatorcontrib>Hauchecorne, A.</creatorcontrib><creatorcontrib>Boumier, P.</creatorcontrib><creatorcontrib>Corbard, T.</creatorcontrib><creatorcontrib>Turck-Chièze, S.</creatorcontrib><creatorcontrib>Abbaki, S.</creatorcontrib><creatorcontrib>Assus, P.</creatorcontrib><creatorcontrib>Bertran, E.</creatorcontrib><creatorcontrib>Bourget, P.</creatorcontrib><creatorcontrib>Buisson, F.</creatorcontrib><creatorcontrib>Chaigneau, M.</creatorcontrib><creatorcontrib>Damé, L.</creatorcontrib><creatorcontrib>Djafer, D.</creatorcontrib><creatorcontrib>Dufour, C.</creatorcontrib><creatorcontrib>Etcheto, P.</creatorcontrib><creatorcontrib>Ferrero, P.</creatorcontrib><creatorcontrib>Hersé, M.</creatorcontrib><creatorcontrib>Marcovici, J.-P.</creatorcontrib><creatorcontrib>Meissonnier, M.</creatorcontrib><creatorcontrib>Morand, F.</creatorcontrib><creatorcontrib>Poiet, G.</creatorcontrib><creatorcontrib>Prado, J.-Y.</creatorcontrib><creatorcontrib>Renaud, C.</creatorcontrib><creatorcontrib>Rouanet, N.</creatorcontrib><creatorcontrib>Rouzé, M.</creatorcontrib><creatorcontrib>Salabert, D.</creatorcontrib><creatorcontrib>Vieau, A.-J.</creatorcontrib><title>Picard SODISM, a Space Telescope to Study the Sun from the Middle Ultraviolet to the Near Infrared</title><title>Solar physics</title><addtitle>Sol Phys</addtitle><description>The
Solar Diameter Imager and Surface Mapper
(SODISM) onboard the
Picard
space mission provides wide-field images of the photosphere and chromosphere of the Sun in five narrow bandpasses centered at 215.0, 393.37, 535.7, 607.1, and 782.2 nm. The
Picard
spacecraft was successfully launched on 15 June 2010 into a Sun-synchronous dawn–dusk orbit. The
Picard
space mission represents a European asset in collecting solar observations useful to improve Earth climatic models. The scientific payload consists of the SODISM imager and of two radiometers,
SOlar VAriability Picard
(SOVAP) and
PREcision MOnitor Sensor
(PREMOS), which measure the Total Solar Irradiance (TSI) and part of the Solar Spectral Irradiance (SSI).
The SODISM telescope continuously monitors solar activity from the middle ultraviolet to the near infrared spectral ranges and produces solar images that feed SSI reconstruction models. Further, SODISM probes the solar interior
via
a helioseismic analysis of the solar disc and limb images at 535.7 nm, and
via
astrometric investigations at the limb. The latter allows us to deduce the spectral dependence of the solar limb profile, and the asphericity of the Sun. Furthermore, SODISM data taken during the transit of Venus allow a determination of the absolute value of the solar diameter. This paper provides a detailed description of the SODISM instrument, including thermo-optical analysis, its different modes of observation, and its first performance in space.</description><subject>Astrophysics</subject><subject>Astrophysics and Astroparticles</subject><subject>Atmospheric Sciences</subject><subject>Infrared radiation</subject><subject>Instrumentation and Methods for Astrophysic</subject><subject>Irradiance</subject><subject>Monitors</subject><subject>Optical analysis</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Sciences of the Universe</subject><subject>Solar activity</subject><subject>Solar and Stellar Astrophysics</subject><subject>Solar diameter</subject><subject>Solar physics</subject><subject>Space Exploration and Astronautics</subject><subject>Space missions</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Space telescopes</subject><subject>Spacecraft</subject><subject>Spectra</subject><subject>Sun</subject><subject>Ultraviolet</subject><subject>Ultraviolet radiation</subject><issn>0038-0938</issn><issn>1573-093X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNqFkV1r1UAQhoMoeKz-AO8WvFEwOpPN7iaXpdX2wKkV0oJ3yyY7a1NyssfdpLT_3k0jIoJ4NV_PO8zwZtlrhA8IoD5GxAJUDshz4Irn90-yDYqUQM2_Pc02ALxa8up59iLGW4BFJTZZ-7XvTLCsuTzdNhfvmWHNwXTErmig2PkDscmzZprtA5tuiDXzyFzw-8fiord2IHY9TMHc9X6gaYGXyRcygW1HF0wg-zJ75swQ6dWveJRdf_50dXKe7y7PtifHu7wrUU55RyCtrV3JTe0E2haNKJ1QRWUF58o4dIUyHTguBZTWFm0ryAhFKFujOPKj7N2698YM-hD6vQkP2ptenx_v9NJLH9eyBn63sG9X9hD8j5nipPd97GgYzEh-jhqlQlFJBer_aFkXEkEUVULf_IXe-jmM6elESYmyqEEmCleqCz7GQO73sQh6sUWvZupkpl7M1PdJU6yamNjxO4U_Nv9T9BNNRZ8u</recordid><startdate>20140301</startdate><enddate>20140301</enddate><creator>Meftah, M.</creator><creator>Hochedez, J.-F.</creator><creator>Irbah, 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Infrared</title><author>Meftah, M. ; Hochedez, J.-F. ; Irbah, A. ; Hauchecorne, A. ; Boumier, P. ; Corbard, T. ; Turck-Chièze, S. ; Abbaki, S. ; Assus, P. ; Bertran, E. ; Bourget, P. ; Buisson, F. ; Chaigneau, M. ; Damé, L. ; Djafer, D. ; Dufour, C. ; Etcheto, P. ; Ferrero, P. ; Hersé, M. ; Marcovici, J.-P. ; Meissonnier, M. ; Morand, F. ; Poiet, G. ; Prado, J.-Y. ; Renaud, C. ; Rouanet, N. ; Rouzé, M. ; Salabert, D. ; Vieau, A.-J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c416t-ce06dd9f43a9f51db1a54f5728d5337af1f27ac0f36504dd2bb5ea57e16ba7313</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>Astrophysics</topic><topic>Astrophysics and Astroparticles</topic><topic>Atmospheric Sciences</topic><topic>Infrared radiation</topic><topic>Instrumentation and Methods for Astrophysic</topic><topic>Irradiance</topic><topic>Monitors</topic><topic>Optical analysis</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Sciences of the Universe</topic><topic>Solar activity</topic><topic>Solar and Stellar Astrophysics</topic><topic>Solar diameter</topic><topic>Solar physics</topic><topic>Space Exploration and Astronautics</topic><topic>Space missions</topic><topic>Space Sciences (including Extraterrestrial Physics</topic><topic>Space telescopes</topic><topic>Spacecraft</topic><topic>Spectra</topic><topic>Sun</topic><topic>Ultraviolet</topic><topic>Ultraviolet radiation</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Meftah, M.</creatorcontrib><creatorcontrib>Hochedez, J.-F.</creatorcontrib><creatorcontrib>Irbah, A.</creatorcontrib><creatorcontrib>Hauchecorne, A.</creatorcontrib><creatorcontrib>Boumier, P.</creatorcontrib><creatorcontrib>Corbard, T.</creatorcontrib><creatorcontrib>Turck-Chièze, S.</creatorcontrib><creatorcontrib>Abbaki, S.</creatorcontrib><creatorcontrib>Assus, 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S.</au><au>Abbaki, S.</au><au>Assus, P.</au><au>Bertran, E.</au><au>Bourget, P.</au><au>Buisson, F.</au><au>Chaigneau, M.</au><au>Damé, L.</au><au>Djafer, D.</au><au>Dufour, C.</au><au>Etcheto, P.</au><au>Ferrero, P.</au><au>Hersé, M.</au><au>Marcovici, J.-P.</au><au>Meissonnier, M.</au><au>Morand, F.</au><au>Poiet, G.</au><au>Prado, J.-Y.</au><au>Renaud, C.</au><au>Rouanet, N.</au><au>Rouzé, M.</au><au>Salabert, D.</au><au>Vieau, A.-J.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Picard SODISM, a Space Telescope to Study the Sun from the Middle Ultraviolet to the Near Infrared</atitle><jtitle>Solar physics</jtitle><stitle>Sol Phys</stitle><date>2014-03-01</date><risdate>2014</risdate><volume>289</volume><issue>3</issue><spage>1043</spage><epage>1076</epage><pages>1043-1076</pages><issn>0038-0938</issn><eissn>1573-093X</eissn><abstract>The
Solar Diameter Imager and Surface Mapper
(SODISM) onboard the
Picard
space mission provides wide-field images of the photosphere and chromosphere of the Sun in five narrow bandpasses centered at 215.0, 393.37, 535.7, 607.1, and 782.2 nm. The
Picard
spacecraft was successfully launched on 15 June 2010 into a Sun-synchronous dawn–dusk orbit. The
Picard
space mission represents a European asset in collecting solar observations useful to improve Earth climatic models. The scientific payload consists of the SODISM imager and of two radiometers,
SOlar VAriability Picard
(SOVAP) and
PREcision MOnitor Sensor
(PREMOS), which measure the Total Solar Irradiance (TSI) and part of the Solar Spectral Irradiance (SSI).
The SODISM telescope continuously monitors solar activity from the middle ultraviolet to the near infrared spectral ranges and produces solar images that feed SSI reconstruction models. Further, SODISM probes the solar interior
via
a helioseismic analysis of the solar disc and limb images at 535.7 nm, and
via
astrometric investigations at the limb. The latter allows us to deduce the spectral dependence of the solar limb profile, and the asphericity of the Sun. Furthermore, SODISM data taken during the transit of Venus allow a determination of the absolute value of the solar diameter. This paper provides a detailed description of the SODISM instrument, including thermo-optical analysis, its different modes of observation, and its first performance in space.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s11207-013-0373-x</doi><tpages>34</tpages><orcidid>https://orcid.org/0000-0001-8990-2526</orcidid><orcidid>https://orcid.org/0000-0002-0168-987X</orcidid><orcidid>https://orcid.org/0000-0003-3265-3148</orcidid><orcidid>https://orcid.org/0000-0002-9615-9619</orcidid></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0038-0938 |
| ispartof | Solar physics, 2014-03, Vol.289 (3), p.1043-1076 |
| issn | 0038-0938 1573-093X |
| language | eng |
| recordid | cdi_hal_primary_oai_HAL_hal_00796903v1 |
| source | SpringerLink |
| subjects | Astrophysics Astrophysics and Astroparticles Atmospheric Sciences Infrared radiation Instrumentation and Methods for Astrophysic Irradiance Monitors Optical analysis Physics Physics and Astronomy Sciences of the Universe Solar activity Solar and Stellar Astrophysics Solar diameter Solar physics Space Exploration and Astronautics Space missions Space Sciences (including Extraterrestrial Physics Space telescopes Spacecraft Spectra Sun Ultraviolet Ultraviolet radiation |
| title | Picard SODISM, a Space Telescope to Study the Sun from the Middle Ultraviolet to the Near Infrared |
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