DocumentCode
2075180
Title
SWAP and LYRA: space weather from a small spacecraft
Author
Defise, J.M. ; Lecat, J.H. ; Stockman, Y. ; Rochus, P. ; Mazy, E. ; Denis, F. ; Halain, J.P. ; Rossi, L. ; Thibert, T. ; Berghmans, D. ; Hochedez, J.F. ; Bogdan, N. ; Ben Moussa, A. ; Lawrence, G. ; Katsiyannis, T. ; Schmutz, W. ; Koller, S. ; Schuhle, U.
Author_Institution
Centre Spatial de Liege, Univ. of Liege, Angleur, Belgium
fYear
2005
fDate
9-11 June 2005
Firstpage
793
Lastpage
798
Abstract
Two scientific instruments for Sun observations are being developed to be part of the payload of the ESA´s second microsatellite, Proba-II (Project for On-board Autonomy). PROBA-2 is scheduled for launch in early 2007, on a low Earth orbit. Like Proba-1, in orbit since October 2001, Proba-2 is a 100-kilogram class spacecraft. PROBA-II will demonstrate new advanced technologies on its scientific payload but also on new platform subsystems such as star tracker, digital Sun sensor, cool gas generator, solar array concentrator, Li-Ion Battery, new central processor. This paper is dedicated to the solar payload, comprising the Sun Watcher using Active Pixel System detector and image Processing (SWAP) and the Lyman alpha Radiometer (LYRA), both aiming at Sun observations. SWAP, the Belgian-led main instrument, will continuously provide detailed images of the solar atmosphere, by the light of extreme ultraviolet rays, at 17.4 nm, completely absorbed by the terrestrial atmosphere. SWAP will perform as an operational solar monitoring tool for space weather forecasting while it will also demonstrate new technological solutions: CMOS/APS detector, new off-axis telescope design, a thermal structure. LYRA (LYman-alpha RAdiometer) is a small compact solar VUV radiometer. This instrument is designed, manufactured and calibrated by a Belgian-Swiss-German consortium. It will monitor the solar flux in four UV passbands. The spectral channels have been carefully selected for their relevance to space weather, solar physics and aeronomy, ranging from 1 nm to 220 nm. On the technological side, LYRA will benefit from the pioneering UV detectors program using diamond technology. The LYRA data will produce valuable solar monitoring information, for operational space weather nowcasting and research. This paper will detail the instrument concepts and their preparation for delivery to the platform.
Keywords
astronomical instruments; radiometers; solar atmosphere; ultraviolet astronomy; Active Pixel System detector; LYRA; Lyman alpha Radiometer; Proba-1; Proba-2; Proba-II; Project for On-board Autonomy; SWAP; Sun Watcher; Sun Watcher using Active Pixel System detector and image Processing; Sun observations; VUV radiometer; extreme ultraviolet; microsatellite; scientific payload; solar atmosphere; space weather; CMOS technology; Detectors; Instruments; Monitoring; Payloads; Radiometry; Sensor arrays; Space technology; Space vehicles; Sun;
fLanguage
English
Publisher
ieee
Conference_Titel
Recent Advances in Space Technologies, 2005. RAST 2005. Proceedings of 2nd International Conference on
Print_ISBN
0-7803-8977-8
Type
conf
DOI
10.1109/RAST.2005.1512688
Filename
1512688
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