LYRA
This articleneeds additional citations forverification.(March 2009) |
Alternative names | LYRA |
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Part of | PROBA-2![]() |
Organization | European Space Agency![]() |
Telescope style | radiometer space instrument ![]() |
LYRA(Lyman Alpha Radiometer) is the solar UV radiometer on boardProba-2,aEuropean Space Agencytechnology demonstration satellite that was launched on November 2, 2009.[1]
LYRA[2][3]has been designed and manufactured by a Belgian-Swiss-German consortium (ROB-SIDC,PMOD/WRC,IMOMEC, CSL, MPS and BISA) with additional international collaborations (Japan, USA, Russia, and France). Jean-François Hochedez (ROB) is Principal Investigator, Yves Stockman (CSL) is Project Manager, and Werner Schmutz (PMOD) is Lead co-Investigator.
LYRA will monitor theSolar irradiancein four UV passbands. They have been chosen for their relevance to solar physics, aeronomy and Space Weather:
- the 115-125 nmLyman-αchannel,
- the 200-220 nmHerzbergcontinuum channel,
- theAluminium filter channel(17-50 nm) including He II at 30.4 nm, and
- theZirconium filter channel(1-20 nm).
TheRadiometric calibrationof the instrument is traceable toSynchrotronsource standards,Physikalisch-Technische Bundesanstalt(PTB) andNational Institute of Standards and Technology(NIST).[4]Its stability will be monitored by onboard calibration light sources (light-emitting diodes), which allow distinguishing between potential degradations of the detectors and filters. Additionally, a redundancy strategy contributes to the accuracy and the stability of the measurements. LYRA will benefit from wide bandgap detectors based on diamond: it will be the first space assessment ofa pioneering UV detectors program.Diamond sensors make the instruments radiation-hard andsolar-blind:their high bandgap energy makes them quasi-insensitive to visible light (see also references inMarchywka Effect). TheSWAPextreme ultraviolet (EUV) imaging telescope will operate next to LYRA on Proba-2. Together, they will establish a high performance solar monitor for operational space weather nowcasting and research. LYRA demonstrates technologies important for future missions such as the ESASolar Orbitermission.
References[edit]
- ^Successful launch qualification test for Proba-2Archived2011-07-25 at theWayback Machine
- ^Hochedez, J; Schmutz, W; Stockman, Y; Schuhle, U; Benmoussa, A; Koller, S; Haenen, K; Berghmans, D; Defise, J; Halain, J.-P.; Theissen, A.; Delouille, V.; Slemzin, V.; Gillotay, D.; Fussen, D.; Dominique, M.; Vanhellemont, F.; McMullin, D.; Kretzschmar, M.; Mitrofanov, A.; Nicula, B.; Wauters, L.; Roth, H.; Rozanov, E.; Rüedi, I.; Wehrli, C.; Soltani, A.; Amano, H.; Van Der Linden, R.; et al. (2006), "LYRA, a solar UV radiometer on Proba2",Advances in Space Research,37(2): 303,Bibcode:2006AdSpR..37..303H,doi:10.1016/j.asr.2005.10.041,hdl:1942/933
- ^LYRA websiteProba-2 Science Center
- ^LYRA, A SOLAR UV RADIOMETER ON PROBA2