Marco Iarlori
Papers
3
Total Citations
16
H-Index
2
About
Marco Iarlori is an experimental physicist whose research bridges solar astrophysics and atmospheric characterization for next-generation astronomical observatories. His primary contributions lie in the development of robotic solar instrumentation and the precise measurement of atmospheric conditions critical for high-energy gamma-ray astronomy. Iarlori led the design and assembly of the Tor Vergata Synoptic Solar Telescope (TSST), a compact robotic facility for continuous multi-line imaging of the full solar disk. This system enables real-time inference of the Sun’s magnetic and dynamical state, providing essential precursors for space weather events such as flares and coronal mass ejections—work that has garnered 12 citations. In parallel, he has played a key role in preparing for the Cherenkov Telescope Array (CTA), the world’s largest ground-based gamma-ray observatory. By operating a dedicated meteorological station at the CTA’s southern site, Iarlori characterized detailed atmospheric properties—temperature, humidity, aerosol content—vital for calibrating CTA’s scientific data. His dual focus on solar monitoring and site characterization demonstrates a commitment to building the observational infrastructure that underpins both solar-terrestrial physics and very-high-energy astrophysics.
Research Focus
Key Achievements
Top Papers
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