Pubblicazioni su Riviste Scientifiche
This study aims to present an overview of how climate change brought about by events such as earthquakes, volcanic eruptions, flares and variations in solar activity, etc. have characterized the area of central Italy, analyzing and comparing astronomical, geological, meteorological, seismological, historical and climatic data, taking as reference some specific locations in the period between 1250 and 1350.
We report our proposal for the establishment of a biocontainment and astrobiology laboratory in a strategic area of Pieve a Nievole (PT) – to face the lack of biological and astrobiological research centers and all the social, economic and cultural consequences that this project implicate.
This paper contains the result of the elaboration of informations about Solar Irradiation, Geological, Meteorological and Climatic from the point of view of the quantitative data and social interaction recorded in Taviano (LE).
We report briefly on the status of the new research facility in Andrate (TO).
All available CCD observation of RV UMa have been analyzed to obtain an accurate mathematical description of the ligh variation. We discuss in this paper a new study of variable star RV UMa, a short period RRab star, in orther to determine through the light curve and the physical parameters, the presence of “Blazhko effect”.
In this paper we present an analysis of the geological, meteorological and climatic data recorded in Acquapendente (VT).
In this paper we present an analysis of the geological, meteorological and climatic data recorded in Pieve a Nievole (PT)
In this work that continues the “NGICS – New Italian City Geological Study” a project of the Department of Climatology and Geology of TS Corporation, we present the study relating to the Municipality of Montefiascone (VT).
We present in this paper the new study of variable star AM Cnc, a short period RRab star, in orther to determine, through the light curve and the physical parameters.
A new CCD photometry survey of the open cluster NGC7788 in U, B, V, R and I colors to magnitude V=20 is present.