E. Pietropaolo
Papers
2
Total Citations
14
H-Index
2
About
E. Pietropaolo is a solar and atmospheric physicist whose work bridges ground-based solar monitoring and high-energy astrophysics. A key contribution is the development of the **Tor Vergata Synoptic Solar Telescope (TSST)**, a robotic facility designed for continuous, multi-line imaging of the solar atmosphere. This instrument enables real-time inference of the Sun’s magnetic and dynamic state—critical for identifying precursors to space weather events like flares and coronal mass ejections. The TSST’s design and assembly, detailed in a 2020 paper (12 citations), represents a significant step toward automated, compact solar observatories. Pietropaolo also contributes to the **Cherenkov Telescope Array (CTA)** project, where they lead atmospheric characterization efforts at future CTA sites. Their 2019 study (2 citations) analyzes meteorological variables using dedicated instrumentation at the southern site, ensuring optimal conditions for gamma-ray observations. This work highlights a rare expertise in both solar physics and atmospheric science, directly supporting two major international facilities. By linking solar activity to space weather prediction and enabling next-generation gamma-ray astronomy, Pietropaolo’s research has tangible impacts on both fundamental astrophysics and practical space-weather forecasting.
Research Focus
Key Achievements
Top Papers
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