The Space Weather and Ultraviolet Solar Variability (SWUSV) Microsatellite Mission
We present the ambitions of the SWUSV (Space Weather and Ultraviolet Solar Variability) Microsatellite Mission that encompasses three major scientific objectives: (1) Space Weather including the prediction and detection of major eruptions and coronal mass ejections (Lyman-Alpha and Herzberg continu...
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doaj-48da8f43380e4facb46aa583409817b52020-11-25T00:01:28ZengElsevierJournal of Advanced Research2090-12322090-12242013-05-014323525110.1016/j.jare.2013.03.002The Space Weather and Ultraviolet Solar Variability (SWUSV) Microsatellite MissionLuc DaméMustapha MeftahAlain HauchecornePhilippe KeckhutAlain SarkissianMarion MarchandAbdenour IrbahÉric QuémeraisSlimane BekkiThomas FoujolsMatthieu KretzschmarGaël CessateurAlexander ShapiroWerner SchmutzSergey KuzinVladimir SlemzinAlexander UrnovSergey BogachevJosé MerayoPeter BrauerKanaris TsinganosAntonis PaschalisAyman MahrousSafinaz KhaledAhmed GhitasBesheir MarzoukAmal ZakiAhmed A. HadyRangaiah Kariyappa We present the ambitions of the SWUSV (Space Weather and Ultraviolet Solar Variability) Microsatellite Mission that encompasses three major scientific objectives: (1) Space Weather including the prediction and detection of major eruptions and coronal mass ejections (Lyman-Alpha and Herzberg continuum imaging); (2) solar forcing on the climate through radiation and their interactions with the local stratosphere (UV spectral irradiance from 180 to 400 nm by bands of 20 nm, plus Lyman-Alpha and the CN bandhead); (3) simultaneous radiative budget of the Earth, UV to IR, with an accuracy better than 1% in differential. The paper briefly outlines the mission and describes the five proposed instruments of the model payload: SUAVE (Solar Ultraviolet Advanced Variability Experiment), an optimized telescope for FUV (Lyman-Alpha) and MUV (200–220 nm Herzberg continuum) imaging (sources of variability); UPR (Ultraviolet Passband Radiometers), with 64 UV filter radiometers; a vector magnetometer; thermal plasma measurements and Langmuir probes; and a total and spectral solar irradiance and Earth radiative budget ensemble (SERB, Solar irradiance & Earth Radiative Budget). SWUSV is proposed as a small mission to CNES and to ESA for a possible flight as early as 2017–2018. http://www.sciencedirect.com/science/article/pii/S2090123213000337Solar eruptionsCoronal mass ejectionsSpace weatherUltraviolet variabilityUltraviolet instrumentationSolar irradiance |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Luc Damé Mustapha Meftah Alain Hauchecorne Philippe Keckhut Alain Sarkissian Marion Marchand Abdenour Irbah Éric Quémerais Slimane Bekki Thomas Foujols Matthieu Kretzschmar Gaël Cessateur Alexander Shapiro Werner Schmutz Sergey Kuzin Vladimir Slemzin Alexander Urnov Sergey Bogachev José Merayo Peter Brauer Kanaris Tsinganos Antonis Paschalis Ayman Mahrous Safinaz Khaled Ahmed Ghitas Besheir Marzouk Amal Zaki Ahmed A. Hady Rangaiah Kariyappa |
spellingShingle |
Luc Damé Mustapha Meftah Alain Hauchecorne Philippe Keckhut Alain Sarkissian Marion Marchand Abdenour Irbah Éric Quémerais Slimane Bekki Thomas Foujols Matthieu Kretzschmar Gaël Cessateur Alexander Shapiro Werner Schmutz Sergey Kuzin Vladimir Slemzin Alexander Urnov Sergey Bogachev José Merayo Peter Brauer Kanaris Tsinganos Antonis Paschalis Ayman Mahrous Safinaz Khaled Ahmed Ghitas Besheir Marzouk Amal Zaki Ahmed A. Hady Rangaiah Kariyappa The Space Weather and Ultraviolet Solar Variability (SWUSV) Microsatellite Mission Journal of Advanced Research Solar eruptions Coronal mass ejections Space weather Ultraviolet variability Ultraviolet instrumentation Solar irradiance |
author_facet |
Luc Damé Mustapha Meftah Alain Hauchecorne Philippe Keckhut Alain Sarkissian Marion Marchand Abdenour Irbah Éric Quémerais Slimane Bekki Thomas Foujols Matthieu Kretzschmar Gaël Cessateur Alexander Shapiro Werner Schmutz Sergey Kuzin Vladimir Slemzin Alexander Urnov Sergey Bogachev José Merayo Peter Brauer Kanaris Tsinganos Antonis Paschalis Ayman Mahrous Safinaz Khaled Ahmed Ghitas Besheir Marzouk Amal Zaki Ahmed A. Hady Rangaiah Kariyappa |
author_sort |
Luc Damé |
title |
The Space Weather and Ultraviolet Solar Variability (SWUSV) Microsatellite Mission |
title_short |
The Space Weather and Ultraviolet Solar Variability (SWUSV) Microsatellite Mission |
title_full |
The Space Weather and Ultraviolet Solar Variability (SWUSV) Microsatellite Mission |
title_fullStr |
The Space Weather and Ultraviolet Solar Variability (SWUSV) Microsatellite Mission |
title_full_unstemmed |
The Space Weather and Ultraviolet Solar Variability (SWUSV) Microsatellite Mission |
title_sort |
space weather and ultraviolet solar variability (swusv) microsatellite mission |
publisher |
Elsevier |
series |
Journal of Advanced Research |
issn |
2090-1232 2090-1224 |
publishDate |
2013-05-01 |
description |
We present the ambitions of the SWUSV (Space Weather and Ultraviolet Solar Variability) Microsatellite Mission that encompasses three major scientific objectives: (1) Space Weather including the prediction and detection of major eruptions and coronal mass ejections (Lyman-Alpha and Herzberg continuum imaging); (2) solar forcing on the climate through radiation and their interactions with the local stratosphere (UV spectral irradiance from 180 to 400 nm by bands of 20 nm, plus Lyman-Alpha and the CN bandhead); (3) simultaneous radiative budget of the Earth, UV to IR, with an accuracy better than 1% in differential. The paper briefly outlines the mission and describes the five proposed instruments of the model payload: SUAVE (Solar Ultraviolet Advanced Variability Experiment), an optimized telescope for FUV (Lyman-Alpha) and MUV (200–220 nm Herzberg continuum) imaging (sources of variability); UPR (Ultraviolet Passband Radiometers), with 64 UV filter radiometers; a vector magnetometer; thermal plasma measurements and Langmuir probes; and a total and spectral solar irradiance and Earth radiative budget ensemble (SERB, Solar irradiance & Earth Radiative Budget). SWUSV is proposed as a small mission to CNES and to ESA for a possible flight as early as 2017–2018.
|
topic |
Solar eruptions Coronal mass ejections Space weather Ultraviolet variability Ultraviolet instrumentation Solar irradiance |
url |
http://www.sciencedirect.com/science/article/pii/S2090123213000337 |
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