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LYRA team

Royal Observatory of Belgium (ROB) Jean-François Hochedez LYRA Principal Investigator Marie Dominique Boris Giordanengo Ingolf Dammasch Ali BenMoussa Observatory and World Radiation Center (PMOD) Werner Schmutz LYRA Lead co-Investigator Silvio Koller Tatiana Egorova Eugene Rozanov Centre (...)

LYRA Science Goals

Flares Detection and Analysis Solar flares are one of the most energetic phenomena in the solar system. During these events, particles can be heated to millions of degrees and ejected in the solar atmosphere. These events appear in radiometer time series as an increase of the solar irradiance, (...)

LYRA instrument

Instrument overview LYRA is composed of three units, each of them constituted of the same four channels: the 120-123 nm Lyman-α channel, the 200-220 nm Herzberg continuum channel, the 17-80 nm Aluminium filter channel, including He II at 30.4 nm, the 6-20 nm Zirconium filter channel. The (...)

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Last update: 17th of March 2010

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LYRA
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- ADS papers: LYRA
- ADS papers: PROBA2
LYRA Analysis Manual
- LYRA analysis manual

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