The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description
- Autores
- Feller, Alex; Gandorfer, Achim; Grauf, Bianca; Hoelken, Johannes; Iglesias, Francisco Andres; Korpi-Lagg, Andreas; Riethmüller, Tino L.; Staub, Jan; Fernandez Rico, German; Castellanos Durán, Juan Sebastián; Solanki, Sami K.; Smitha, H. N.; Sant, Kamal; Barthol, Peter; Montserrat Bayon Laguna; Bergmann, Melani; Bischoff, Jörg; Bochmann, Jan; Bruns, Stefan; Deutsch, Werner; Berkefeld, Thomas; Bernasconi, Pietro; Katsukawa, Yukio; del Toro Iniesta, Jose Carlos; Bell, Alexander; Carpenter, Michael; Álvarez Herrero, Alberto; Kubo, Masahito; Martínez Pillet, Valentín; Orozco Suárez, David
- Año de publicación
- 2025
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The third science flight of the balloon-borne solar observatory Sunrise carries three entirely new post-focus science instruments with spectropolarimetric capabilities, concurrently covering an extended spectral range from the near ultraviolet to the near infrared. Sampling a larger height range, from the low photosphere to the chromosphere, with the sub-arcsecond resolution provided by the 1-m Sunrise telescope, is key in understanding critical small-scale phenomena which energetically couple different layers of the solar atmosphere. The SUSI operates between 309nm and 417nm. A key feature of SUSI is its capability to record up to several hundred spectral lines simultaneously without the harmful effects of the Earth´s atmosphere. The rich SUSI spectra can be exploited in terms of many-line inversions. Another important innovation of the instrument is the synchronized 2D context imaging which allows to numerically correct the spectrograph scans for residual optical aberrations. In this work we describe the main design aspects of SUSI, the instrument characterization and testing, and finally its operation, expected performance and data products.
Fil: Feller, Alex. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Gandorfer, Achim. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Grauf, Bianca. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Hoelken, Johannes. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Iglesias, Francisco Andres. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza; Argentina. Universidad de Mendoza. Facultad de Ingenieria; Argentina. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Korpi-Lagg, Andreas. Max Planck Institut Fur Sonnensystemforschung; Alemania. Aalto University; Finlandia
Fil: Riethmüller, Tino L.. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Staub, Jan. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Fernandez Rico, German. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Castellanos Durán, Juan Sebastián. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Solanki, Sami K.. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Smitha, H. N.. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Sant, Kamal. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Barthol, Peter. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Montserrat Bayon Laguna. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Bergmann, Melani. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Bischoff, Jörg. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Bochmann, Jan. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Bruns, Stefan. Fraunhofer-Institut für Schicht- und Oberflächentechnik; Alemania
Fil: Deutsch, Werner. Max Planck Institut Fur Sonnensystemforschung; Alemania
Fil: Berkefeld, Thomas. Institut für Sonnenphysik; Alemania
Fil: Bernasconi, Pietro. Johns Hopkins Applied Physics Laboratory; Estados Unidos
Fil: Katsukawa, Yukio. National Astronomical Observatory of Japan; Japón
Fil: del Toro Iniesta, Jose Carlos. Instituto de Astrofísica de Andalucía; España
Fil: Bell, Alexander. Institut für Sonnenphysik; Alemania
Fil: Carpenter, Michael. Johns Hopkins Applied Physics Laboratory; Estados Unidos
Fil: Álvarez Herrero, Alberto. Consejo Superior de Investigaciones Cientificas. Instituto Nacional de Tecnica Aeroespacial.; España
Fil: Kubo, Masahito. National Astronomical Observatory of Japan; Japón
Fil: Martínez Pillet, Valentín. Instituto de Astrofísica de Canarias; España
Fil: Orozco Suárez, David. Instituto de Astrofísica de Andalucía; España - Materia
-
Instrumentation and Data Management
Polarization
Optical Spectrum
Ultraviolet - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/273260
Ver los metadatos del registro completo
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The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument DescriptionFeller, AlexGandorfer, AchimGrauf, BiancaHoelken, JohannesIglesias, Francisco AndresKorpi-Lagg, AndreasRiethmüller, Tino L.Staub, JanFernandez Rico, GermanCastellanos Durán, Juan SebastiánSolanki, Sami K.Smitha, H. N.Sant, KamalBarthol, PeterMontserrat Bayon LagunaBergmann, MelaniBischoff, JörgBochmann, JanBruns, StefanDeutsch, WernerBerkefeld, ThomasBernasconi, PietroKatsukawa, Yukiodel Toro Iniesta, Jose CarlosBell, AlexanderCarpenter, MichaelÁlvarez Herrero, AlbertoKubo, MasahitoMartínez Pillet, ValentínOrozco Suárez, DavidInstrumentation and Data ManagementPolarizationOptical SpectrumUltraviolethttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The third science flight of the balloon-borne solar observatory Sunrise carries three entirely new post-focus science instruments with spectropolarimetric capabilities, concurrently covering an extended spectral range from the near ultraviolet to the near infrared. Sampling a larger height range, from the low photosphere to the chromosphere, with the sub-arcsecond resolution provided by the 1-m Sunrise telescope, is key in understanding critical small-scale phenomena which energetically couple different layers of the solar atmosphere. The SUSI operates between 309nm and 417nm. A key feature of SUSI is its capability to record up to several hundred spectral lines simultaneously without the harmful effects of the Earth´s atmosphere. The rich SUSI spectra can be exploited in terms of many-line inversions. Another important innovation of the instrument is the synchronized 2D context imaging which allows to numerically correct the spectrograph scans for residual optical aberrations. In this work we describe the main design aspects of SUSI, the instrument characterization and testing, and finally its operation, expected performance and data products.Fil: Feller, Alex. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Gandorfer, Achim. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Grauf, Bianca. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Hoelken, Johannes. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Iglesias, Francisco Andres. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza; Argentina. Universidad de Mendoza. Facultad de Ingenieria; Argentina. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Korpi-Lagg, Andreas. Max Planck Institut Fur Sonnensystemforschung; Alemania. Aalto University; FinlandiaFil: Riethmüller, Tino L.. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Staub, Jan. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Fernandez Rico, German. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Castellanos Durán, Juan Sebastián. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Solanki, Sami K.. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Smitha, H. N.. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Sant, Kamal. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Barthol, Peter. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Montserrat Bayon Laguna. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Bergmann, Melani. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Bischoff, Jörg. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Bochmann, Jan. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Bruns, Stefan. Fraunhofer-Institut für Schicht- und Oberflächentechnik; AlemaniaFil: Deutsch, Werner. Max Planck Institut Fur Sonnensystemforschung; AlemaniaFil: Berkefeld, Thomas. Institut für Sonnenphysik; AlemaniaFil: Bernasconi, Pietro. Johns Hopkins Applied Physics Laboratory; Estados UnidosFil: Katsukawa, Yukio. National Astronomical Observatory of Japan; JapónFil: del Toro Iniesta, Jose Carlos. Instituto de Astrofísica de Andalucía; EspañaFil: Bell, Alexander. Institut für Sonnenphysik; AlemaniaFil: Carpenter, Michael. Johns Hopkins Applied Physics Laboratory; Estados UnidosFil: Álvarez Herrero, Alberto. Consejo Superior de Investigaciones Cientificas. Instituto Nacional de Tecnica Aeroespacial.; EspañaFil: Kubo, Masahito. National Astronomical Observatory of Japan; JapónFil: Martínez Pillet, Valentín. Instituto de Astrofísica de Canarias; EspañaFil: Orozco Suárez, David. Instituto de Astrofísica de Andalucía; EspañaSpringer2025-05-15info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/273260Feller, Alex; Gandorfer, Achim; Grauf, Bianca; Hoelken, Johannes; Iglesias, Francisco Andres; et al.; The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description; Springer; Solar Physics; 300; 65; 15-5-20250038-0938CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/s11207-025-02471-7info:eu-repo/semantics/altIdentifier/doi/10.1007/s11207-025-02471-7info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T15:05:08Zoai:ri.conicet.gov.ar:11336/273260instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-15 15:05:08.939CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description |
| title |
The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description |
| spellingShingle |
The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description Feller, Alex Instrumentation and Data Management Polarization Optical Spectrum Ultraviolet |
| title_short |
The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description |
| title_full |
The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description |
| title_fullStr |
The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description |
| title_full_unstemmed |
The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description |
| title_sort |
The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description |
| dc.creator.none.fl_str_mv |
Feller, Alex Gandorfer, Achim Grauf, Bianca Hoelken, Johannes Iglesias, Francisco Andres Korpi-Lagg, Andreas Riethmüller, Tino L. Staub, Jan Fernandez Rico, German Castellanos Durán, Juan Sebastián Solanki, Sami K. Smitha, H. N. Sant, Kamal Barthol, Peter Montserrat Bayon Laguna Bergmann, Melani Bischoff, Jörg Bochmann, Jan Bruns, Stefan Deutsch, Werner Berkefeld, Thomas Bernasconi, Pietro Katsukawa, Yukio del Toro Iniesta, Jose Carlos Bell, Alexander Carpenter, Michael Álvarez Herrero, Alberto Kubo, Masahito Martínez Pillet, Valentín Orozco Suárez, David |
| author |
Feller, Alex |
| author_facet |
Feller, Alex Gandorfer, Achim Grauf, Bianca Hoelken, Johannes Iglesias, Francisco Andres Korpi-Lagg, Andreas Riethmüller, Tino L. Staub, Jan Fernandez Rico, German Castellanos Durán, Juan Sebastián Solanki, Sami K. Smitha, H. N. Sant, Kamal Barthol, Peter Montserrat Bayon Laguna Bergmann, Melani Bischoff, Jörg Bochmann, Jan Bruns, Stefan Deutsch, Werner Berkefeld, Thomas Bernasconi, Pietro Katsukawa, Yukio del Toro Iniesta, Jose Carlos Bell, Alexander Carpenter, Michael Álvarez Herrero, Alberto Kubo, Masahito Martínez Pillet, Valentín Orozco Suárez, David |
| author_role |
author |
| author2 |
Gandorfer, Achim Grauf, Bianca Hoelken, Johannes Iglesias, Francisco Andres Korpi-Lagg, Andreas Riethmüller, Tino L. Staub, Jan Fernandez Rico, German Castellanos Durán, Juan Sebastián Solanki, Sami K. Smitha, H. N. Sant, Kamal Barthol, Peter Montserrat Bayon Laguna Bergmann, Melani Bischoff, Jörg Bochmann, Jan Bruns, Stefan Deutsch, Werner Berkefeld, Thomas Bernasconi, Pietro Katsukawa, Yukio del Toro Iniesta, Jose Carlos Bell, Alexander Carpenter, Michael Álvarez Herrero, Alberto Kubo, Masahito Martínez Pillet, Valentín Orozco Suárez, David |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
Instrumentation and Data Management Polarization Optical Spectrum Ultraviolet |
| topic |
Instrumentation and Data Management Polarization Optical Spectrum Ultraviolet |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
The third science flight of the balloon-borne solar observatory Sunrise carries three entirely new post-focus science instruments with spectropolarimetric capabilities, concurrently covering an extended spectral range from the near ultraviolet to the near infrared. Sampling a larger height range, from the low photosphere to the chromosphere, with the sub-arcsecond resolution provided by the 1-m Sunrise telescope, is key in understanding critical small-scale phenomena which energetically couple different layers of the solar atmosphere. The SUSI operates between 309nm and 417nm. A key feature of SUSI is its capability to record up to several hundred spectral lines simultaneously without the harmful effects of the Earth´s atmosphere. The rich SUSI spectra can be exploited in terms of many-line inversions. Another important innovation of the instrument is the synchronized 2D context imaging which allows to numerically correct the spectrograph scans for residual optical aberrations. In this work we describe the main design aspects of SUSI, the instrument characterization and testing, and finally its operation, expected performance and data products. Fil: Feller, Alex. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Gandorfer, Achim. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Grauf, Bianca. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Hoelken, Johannes. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Iglesias, Francisco Andres. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza; Argentina. Universidad de Mendoza. Facultad de Ingenieria; Argentina. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Korpi-Lagg, Andreas. Max Planck Institut Fur Sonnensystemforschung; Alemania. Aalto University; Finlandia Fil: Riethmüller, Tino L.. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Staub, Jan. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Fernandez Rico, German. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Castellanos Durán, Juan Sebastián. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Solanki, Sami K.. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Smitha, H. N.. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Sant, Kamal. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Barthol, Peter. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Montserrat Bayon Laguna. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Bergmann, Melani. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Bischoff, Jörg. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Bochmann, Jan. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Bruns, Stefan. Fraunhofer-Institut für Schicht- und Oberflächentechnik; Alemania Fil: Deutsch, Werner. Max Planck Institut Fur Sonnensystemforschung; Alemania Fil: Berkefeld, Thomas. Institut für Sonnenphysik; Alemania Fil: Bernasconi, Pietro. Johns Hopkins Applied Physics Laboratory; Estados Unidos Fil: Katsukawa, Yukio. National Astronomical Observatory of Japan; Japón Fil: del Toro Iniesta, Jose Carlos. Instituto de Astrofísica de Andalucía; España Fil: Bell, Alexander. Institut für Sonnenphysik; Alemania Fil: Carpenter, Michael. Johns Hopkins Applied Physics Laboratory; Estados Unidos Fil: Álvarez Herrero, Alberto. Consejo Superior de Investigaciones Cientificas. Instituto Nacional de Tecnica Aeroespacial.; España Fil: Kubo, Masahito. National Astronomical Observatory of Japan; Japón Fil: Martínez Pillet, Valentín. Instituto de Astrofísica de Canarias; España Fil: Orozco Suárez, David. Instituto de Astrofísica de Andalucía; España |
| description |
The third science flight of the balloon-borne solar observatory Sunrise carries three entirely new post-focus science instruments with spectropolarimetric capabilities, concurrently covering an extended spectral range from the near ultraviolet to the near infrared. Sampling a larger height range, from the low photosphere to the chromosphere, with the sub-arcsecond resolution provided by the 1-m Sunrise telescope, is key in understanding critical small-scale phenomena which energetically couple different layers of the solar atmosphere. The SUSI operates between 309nm and 417nm. A key feature of SUSI is its capability to record up to several hundred spectral lines simultaneously without the harmful effects of the Earth´s atmosphere. The rich SUSI spectra can be exploited in terms of many-line inversions. Another important innovation of the instrument is the synchronized 2D context imaging which allows to numerically correct the spectrograph scans for residual optical aberrations. In this work we describe the main design aspects of SUSI, the instrument characterization and testing, and finally its operation, expected performance and data products. |
| publishDate |
2025 |
| dc.date.none.fl_str_mv |
2025-05-15 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/273260 Feller, Alex; Gandorfer, Achim; Grauf, Bianca; Hoelken, Johannes; Iglesias, Francisco Andres; et al.; The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description; Springer; Solar Physics; 300; 65; 15-5-2025 0038-0938 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/273260 |
| identifier_str_mv |
Feller, Alex; Gandorfer, Achim; Grauf, Bianca; Hoelken, Johannes; Iglesias, Francisco Andres; et al.; The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description; Springer; Solar Physics; 300; 65; 15-5-2025 0038-0938 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/s11207-025-02471-7 info:eu-repo/semantics/altIdentifier/doi/10.1007/s11207-025-02471-7 |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/2.5/ar/ |
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openAccess |
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Springer |
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Springer |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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