The PROBA2 Mission

Part I PROBA2 satellite and instrument papers.- Title TBA, on PROBA.- The SWAP EUV Imaging Telescope.- Part I Instrument Overview and Pre-Flight Testing.- The SWAP EUV Imaging Telescope.- Part II In-flight Performance and Calibration.- Title TBA, on LYRA.- Part II The PROBA2 Science Center.- The Projects for Onboard Autonomy (PROBA2) Science Centre: Sun Watcher Using APS Detectors and Image Processing (SWAP) and Large-Yield Radiometer (LYRA) Science Operations and Data Products.- Part III Scientific results from SWAP and LYRA observations.- Formation of a White-Light Jet Within a Quadrupolar Magnetic Configuration.- Study of a Prominence Eruption using PROBA2/SWAP and STEREO/EUVI Data.- Solar TErrestrial Relations Observatory-A (STEREO-A) and PRoject for On-Board Autonomy 2 (PROBA2) Quadrature Observations of Reflections of Three EUV Waves from a Coronal Hole.- Detection of Solar Rotational Variability in the Large Yield RAdiometer (LYRA) 190 - 222 nm Spectral Band.- Eclipses Observed by Large Yield RAdiometer (LYRA) - A Sensitive Tool to Test Models for the Solar Irradiance.- Dynamics of Coronal Bright Points as Seen by Sun Watcher Using Active Pixel System Detector and Image Processing (SWAP), Atmospheric Imaging Assembly (AIA), and Helioseismic and Magnetic Imager (HMI).- Prominence-cavity regions observed using SWAP 17.4 nm filtergrams and simultaneous eclipse flash spectra.- SoFAST: Automated Flare Detection with the PROBA2/SWAP EUV Imager.- Sun-as-a-Star Observation of Flares in Lyman alpha by the PROBA2/LYRA radiometer.- Title TBA, on CLAIRE.

Dr. David Berghmans is Operational Director a.i. of the research group "Solar Physics and Space Weather" at the Royal Observatory of Belgium.  His research interests cover all aspects of coronal physics and related fields. He is co-author of 47 refereed publications (NASA ADS numbers). Dr. Berghmans is the principal investigator of the SWAP instrument on board PROBA2. Currently, he is leading the PROBA2 science center that coordinates the operations of the SWAP and LYRA space weather instruments on board PROBA2. D. Berghmans is co-PI in the EUI consortium that is preparing for the EUV imagers aboard the Solar Orbiter mission.

Dr. Anik de Groof is an ESA scientist for SWAP and LYRA, at the PROBA2 science center (located at the Royal Observatory of Belgium). She obtained her Ph.D. in Solar Physics in 2002 from the K.U. Leuven, Belgium, studying coronal heating mechanisms and coronal waves both in theory as in observational data, and is co-author of 20 refereed publications (NASA ADS number).  She has been involved in PROBA2 since the pre-flight calibration of the EUV imager SWAP in 2006. Since then, she has actively contributed to the many phases of the mission, from the design and development of the PROBA2 Science Centre and the launch activities, to the daily instrument commanding, data processing and scientific exploitation of the SWAP and LYRA data. Recently, Dr. de Groof moved to the European Space and Astronomy Centre (ESAC) in Madrid to design and implement the Scientific Operations Centre for the upcoming Solar Orbiter mission.

Ir. Marie Dominique is a scientist at the Royal Observatory of Belgium. Her main scientific interests are the evolution of UV solar irradiance and solar flares.  She joined the LYRA team at an early stage of its conception and took a significant part in the development of the instrument. Since mid-2010, Ir. Dominique has been the principal investigator of LYRA. She is co-author of 11 refereed publications (NASA ADS