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Scientific Report 2007-2009<br />

Organization<br />

A- Astronomy & Astrophysics:<br />

A1. Structure and Evolution of Galaxies<br />

A2. Evolution of stellar systems and galactic nuclei formation and activity<br />

A3. Advanced evolutionary phases of high mass stars<br />

A4. Equilibrium and stability of relativistic stellar clusters and study of properties of systems with<br />

anisotropic distribution of stars velocities<br />

A5. Search for periodicities in the solar energetic proton fluxes<br />

A6. Measurement of the Galactic dust emission in the infrared and microwave bands<br />

A7. Gravitational lensing and its cosmological applications<br />

A8. Galactic and extragalactic sources of X and Gamma rays<br />

A9. Spectral evolution and variability of Active Galactic Nuclei<br />

A10. Search and analysis of galaxy clusters in the optical and X-ray bands<br />

A11. Astronomical Databases: the Digitized First Byurakan Survey (DFBS) and the Roma Blazar<br />

Catalogue (BZCat)<br />

A12. Ground-based observations of the Secondary Anisotropy of the Cosmic Microwave Background<br />

A13. Balloon-borne and satellite measurements of the Cosmic Microwave Background and its interaction<br />

with Clusters of Galaxies<br />

A14. Cosmic Microwave Background Polarization Measurements<br />

A15. Kinetic Inductance Detectors for Measurements of the Cosmic Microwave Background<br />

A16. Testing fundamental physics with cosmology<br />

G- Geophysics:<br />

G1. Theory and observations of climate and its changes<br />

G2. Solar spectrophotometry to measure O 3 , NO 2 , UV irradiance and polysulphone dosimetry to quantify<br />

human UV exposure<br />

G3. Atmospheric acoustical and optical remote sensing at middle latitudes<br />

G4. Atmospheric optical remote sensing in Polar regions<br />

H- History of physics and physics education:<br />

H1. The early history of experimental physics at la <strong>Sapienza</strong> (1746-1930) and the development<br />

of physics in Italy after WWII<br />

H2. Italy in Space<br />

H3. Physics education: new perspectives on the problem of the transition from classical to quantum physics<br />

<strong>Sapienza</strong> Università di Roma 18 Dipartimento di Fisica

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