Abstract : The Large Yield Radiometer (LYRA) is an XUV-EUV-MUV (soft X-ray to mid-ultraviolet) solar radiometer onboard the European Space Agency Project for On-Board Autonomy 2 (PROBA2) mission, which was launched in November 2009. LYRA acquires solar-irradiance measurements at a high cadence (nominally 20 Hz) in four broad spectral channels, from soft X-ray to MUV, which have been chosen for their relevance to solar physics, space weather, and aeronomy. We briefly review the design of the instrument, give an overview of the data products distributed through the instrument website, and describe how the data are calibrated. We also briefly present a summary of the main fields of research currently under investigation by the LYRA consortium.
https://hal.archives-ouvertes.fr/hal-00794273
Contributor : Catherine Cardon
<>
Submitted on : Monday, January 18, 2016 - 3:31:29 PM
Last modification on : Tuesday, April 9, 2019 - 11:16:01 AM
Document(s) archivé(s) le : Friday, November 11, 2016 - 9:51:19 AM
Marie Dominique, Jean-François Hochedez, W. Schmutz, I. E. Dammasch, A. I. Shapiro, et al.. The LYRA Instrument Onboard PROBA2: Description and In-Flight Performance. Solar Physics, Springer Verlag, 2013, 286 (1), pp.21-42. ⟨10.1007/s11207-013-0252-5⟩. ⟨hal-00794273⟩
