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Earth-Prints is an open archive created and maintained by Istituto Nazionale di Geofisica e Vulcanologia. This digital collection allows users to browse, search and access manuscripts, journal articles, theses, conference materials, books, book-chapters, web products.

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  • PublicationOpen Access
    Radon activity concentrations in the soils of the Gioia Tauro Basin (Calabria, southern Italy), with insights on geo-structural control
    (Abingdon U.K.: Taylor & Francis Surrey U.K.: School of Earth Sciences and Geography Kingston University, 2005-, 2026-03-17)
    Muto, Marina
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    Lupiano, Valeria
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    Buttafuoco, Gabriele
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    Procopio, Salvatore
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    Russo, Luigi
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    Department of Biology, Ecology and Earth Sciences, UNICAL-DiBEST (University of Calabria), Rende, Italy; CNR-IRPI (National Research Council, Research Institute for Geo-Hydrological Protection), Cosenza, Italy
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    CNR-IRPI (National Research Council, Research Institute for Geo-Hydrological Protection), Cosenza, Italy
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    Department of Biology, Ecology and Earth Sciences, UNICAL-DiBEST (University of Calabria), Rende, Italy
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    CNR – ISAFOM (National Research Council, Institute for Agricultural and Forest Systems in the Mediterranean), Rende, Italy
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    ARPA-Calabria (Regional Agency for Environmental Protection of Calabria), Catanzaro, Italy
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    Department of Biology, Ecology and Earth Sciences, UNICAL-DiBEST (University of Calabria), Rende, Italy
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    Department of Biology, Ecology and Earth Sciences, UNICAL-DiBEST (University of Calabria), Rende, Italy
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    CNR-IRPI (National Research Council, Research Institute for Geo-Hydrological Protection), Cosenza, Italy
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    Department of Biology, Ecology and Earth Sciences, UNICAL-DiBEST (University of Calabria), Rende, It
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    The main aim of this work is to map Radon activity concentrations in the soil of a tectonicallyactive Mediterranean sector (Gioia Tauro Basin, Calabria, southern Italy). A total of 276 measurements have been taken at a depth of ca. 60 cm from the soil surface, using a portable ionisation chamber, according to a pre-established protocol. Measurements have been performed at the centroids of a 2.5 km square grid, and along transverse sections across the main faults. Spatial variation of 222Rn concentrations in soil gas has been modelled through a geostatistical approach, generating 200 realisations by sequential Gaussian simulation. Maps of 222Rn, of 220Rn and of ratio 222Rn / (220Rn + 222Rn) are presented. The distribution of Rn concentrations is highly asymmetrical (median: 14.5 kBq/ m3; standard dev. 22.7 kBq/m3; min: 0.06 kBq/m3; max: 137 kBq/m3). The results provide insights into the relationships with the geo-structural characteristics of the territory.
  • PublicationOpen Access
    The INGV data registry as a curated metadata infrastructure for Earth Science data stewardship
    The Istituto Nazionale di Geofisica e Vulcanologia (INGV), Italy’s primary institution for geophysics and volcanology, produces vast, heterogeneous geophysical and volcanological datasets. To enhance these assets under Open Science mandates, we implemented the INGV Data Registry: a centralized, curated metadata infrastructure. This metadata-only system is designed to decouple data description from physical storage, providing a scalable solution for distributed data environments. The Registry operates as a dynamic ecosystem that manages hundreds of records, each assigned to a Digital Object Identifier (DOI) and mapped to international standards. This article examines the implementation and impact of the Registry as a critical infrastructure that supports the FAIR data principles. We demonstrate how a three-tiered validation workflow, combined with the integration of Persistent Identifiers (ORCIDs, RORs), ensures high-quality, interoperable metadata. By providing a single discovery point for INGV’s distributed data assets, the Registry offers a model for data stewardship in large research organizations, accelerating scientific discovery and decoupling data availability from traditional publication cycles. The underlying metadata dataset is publicly available and formally citable.
  • PublicationOpen Access
    The state of mid-latitude thermosphere retrieved from ionosonde and Swarm satellite observations during geomagnetic storms in February 2022
    This analysis of the impact of geomagnetic storms on the Thermosphere-Ionosphere system provides critical insights into the complex interplay between geomagnetic activity and the upper atmosphere dynamics. On February 3, 2022, SpaceX launched 49 Starlink satellites into orbits at altitudes ranging between 210 and 320 km. Unfortunately, 38 of these satellites were lost due to the effects of two moderate geomagnetic storms, which caused a significant increase in neutral density in the thermosphere, resulting in higher atmospheric drag. To study the impact of these geomagnetic storms on the Thermosphere-Ionosphere system, F-layer Ne(h) profiles from ground-based ionosondes, located in different longitudinal sectors of both hemispheres, along with Swarm-C neutral density observations, were analyzed using an original method called THERION (THERmospheric parameters from IONosonde observations). The analysis revealed that during the daytime in mid-latitude regions, the thermosphere exhibited relatively small neutral density perturbations of less than 50% at an altitude of 250 km. However, significant disturbances in thermospheric and ionospheric parameters were identified in the longitudinal sectors over America and Australia. In the Northern Hemisphere's winter, the largest increase in atomic oxygen [O] was revealed, ranging between 30% and 50%, which significantly contributed to the rise in neutral density at 250 km (q 250). This seasonal increase in [O] was a key factor driving the observed neutral density changes. Conversely, in the summer hemisphere, atomic oxygen [O] decreased by 20-40%, reducing its contribution to neutral density. Instead, the rise in q 250 was primarily attributed to an increase in molecular nitrogen [N 2 ], which was driven by elevated neutral temperatures (Tex) caused by the geomagnetic storms. In the Northern Hemisphere's winter, the combined effects of atomic oxygen [O] downwelling and an increase in molecular nitrogen [N 2 ], driven by higher neutral temperatures (Tex), acted in phase. This synergy resulted in a 35-45% rise in neutral density at 250 km. In contrast, during the Southern Hemisphere's summer, the opposing effects of [O] (which decreased) and [N 2 ] (which increased) largely cancelled each other out. As a result, the overall impact on q 250 was minimized, showing limited changes in neutral density. This contrast illustrates the seasonal dependence of thermospheric composition and temperature responses to geomagnetic disturbances. The European longitudinal sector exhibited behavior similar to the American longitudinal sector but with less intensity. Here, a 16-35% storm-time increase in neutral density at 250 km was primarily driven by a rise in atomic oxygen [O]. In the winter Japanese sector, neutral density perturbations were modest, with increases of less than 21%, primarily attributed to elevated neutral temperatures (Tex). These findings indicate that while the overall impact of the two February 2022 geomagnetic storms on the Thermosphere-Ionosphere system was moderate, it was significant enough to cause the loss of 38 satellites. This underscores the critical need for continuous monitoring of the thermosphere to better predict and mitigate the effects of geomagnetic activity on satellite operations.
  • PublicationOpen Access
    The factors affecting noontime ionospheric NmF2 equinoctial asymmetry over mid-latitude regions
    Mid-latitude semiannual noontime NmF 2 peaks were analyzed at four North Hemisphere (Boulder, Rome, Wakkanai, Juliusruh) and two South Hemisphere (Hobart, Port Stanley) stations. Aeronomic parameters responsible for the observed NmF 2 variations were obtained solving an inverse problem of aeronomy with the original THERION method. The NmF 2 autumnal peak on average is larger than the vernal one in both Hemispheres under solar minimum. The observed NmF 2 difference in the two peaks is attributed to the difference in thermospheric parameters not related to solar and geomagnetic activity. The vernal peak may occur in the course of three months in both Hemispheres while the occurrence of the autumnal peak is confined by two months. The abundance of atomic oxygen [O] plays the leading role in the difference between NmF 2 in the two peaks. A two-hump NmF 2 variation with a trough in December-January (Northern Hemisphere) is a manifestation of low [O] concentration in December/January relative to October/November values rather than the solar zenith angle effect. The empirical (based on observations) MSISE00 model indicates the global increase of the total atomic oxygen abundance during equinoxes which cannot be attributed to any redistribution of [O] in the thermosphere as we have the absolute global scale [O] increase. The downward transfer of [O] by eddy diffusion is the process which can globally control the amount of [O] in the thermosphere. Anyway it is not seen any other way to explain the global increase of the total amount of atomic oxygen during equinoxes.