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  • 2005-2009  (14)
  • 2007  (14)
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  • 2005-2009  (14)
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  • 1
    Publication Date: 2007-02-01
    Print ISSN: 0016-7061
    Electronic ISSN: 1872-6259
    Topics: Geosciences , Agriculture, Forestry, Horticulture, Fishery, Domestic Science, Nutrition
    Published by Elsevier
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  • 2
    Publication Date: 2007-03-01
    Print ISSN: 0304-8853
    Electronic ISSN: 1873-4766
    Topics: Physics
    Published by Elsevier
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  • 3
    Publication Date: 2021-06-07
    Description: In this work, the effects of magnetic inclusions in a Mars-like soil are considered with reference to the electromagnetic propagation features of ground-penetrating radars (GPRs). Low-frequency and time-domain techniques, using L-C-R meters and TDR instruments, respectively, are implemented in laboratory experimental set-ups in order to evaluate complex permittivity and permeability and wave velocity for different scenarios of a dielectric background medium (silica) with magnetic inclusions (magnetite). Attenuation and maximum detection ranges have also been evaluated by taking into account a realistic GPR environment, which includes the transmitting/receiving antenna performance and the complex structure of the subsurface. The analysis and the interpretation of these results shed new light on the significant influence of magnetic inclusions on the performance of Martian orbiting and rover-driven GPRs.
    Description: Published
    Description: 5-11
    Description: reserved
    Keywords: ground-penetrating radars ; Martian subsurface ; 04. Solid Earth::04.02. Exploration geophysics::04.02.99. General or miscellaneous
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 4
    Publication Date: 2017-04-04
    Description: IN THE FILE
    Description: Published
    Description: 377-392
    Description: open
    Keywords: NONE ; 04. Solid Earth::04.05. Geomagnetism::04.05.03. Global and regional models
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: book chapter
    Format: 879061 bytes
    Format: application/pdf
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  • 5
    Publication Date: 2017-04-04
    Description: GEOSTAR, an European-funded project, is based on a submarine multidisciplinary observatory, that gathered geophysical and geochemical data during a period of six months, from September 2000 to March 2001, in its first deep seafloor mission (about 2000 m depth), off the coast of Ustica Island (Sicily, Italy). GEOSTAR was equipped with several scientific instrumentations, among them two magnetometers. Total intensity of the Earth’s magnetic field and its vectorial components were recorded by means of a scalar magnetometer (Overhauser type) and a suspended three axial fluxgate magnetometer, the latter being designed and built at the Istituto Nazionale di Geofisica e Vulcanologia laboratories. The adverse conditions of an environment located at 2000 m under the sea surface, obliged the making of a special design for the whole frame, including the use of non-magnetic materials for the structure, and the installation of two opposite expanding arms that contained the magnetometers. The geomagnetic experiment was completed by carrying out two fundamental procedures: the instrumental calibration and the computation of the vectorial magnetometer orientation with respect to the geographical reference, both are described in this paper. We also illustrate some properties of the complete magnetic data set, together with a spectral analysis performed in a particular condition of planetary magnetic activity, as well as applications aimed at extracting information about the crustal electric conductivity from the magnetic data in the area around Ustica Island.
    Description: Published
    Description: 105-114
    Description: open
    Keywords: geomagnetic ; GEOSTAR, ; 01. Atmosphere::01.01. Atmosphere::01.01.08. Instruments and techniques
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 6
    Publication Date: 2017-04-04
    Description: Istituto Nazionale di Geofisica e Vulcanologia (INGV) is responsible for systematic magnetic observations in Italy made in observatories and repeat stations. At present, two regularly working geomagnetic observatories cover central and northern Italy: L’Aquila (the main Italian observatory since 1958) and Castello Tesino (since 1964). A new observatory is, at the moment, being installed in the southern Mediterranean (near Sicily) at Lampedusa Island. Once this installation is successfully completed, the three observatories will be able to provide a full coverage of the whole Italian latitudinal extension. A network of magnetic repeat stations is regularly distributed across Italy and measurements in some locations have been made for more than a century. Since the end of the 1970’s, INGV has been developing a modern repeat station network used for the compilation of the Italian magnetic maps. The most recent survey was made between 2004 and 2005 using L’Aquila Observatory as reference.
    Description: Published
    Description: 209-216
    Description: 1.6. Osservazioni di geomagnetismo
    Description: N/A or not JCR
    Description: open
    Keywords: Magnetic observatories ; magnetic network ; 04. Solid Earth::04.05. Geomagnetism::04.05.02. Geomagnetic field variations and reversals
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 7
    Publication Date: 2017-04-04
    Description: The analysis of the foF2 ionosonde data acquired at mid and high latitudes reveals a general decreasing of the F2 plasma frequency over more than two solar cycles, showing steeper trends over the high latitude stations and, in particular, over Antarctica. A careful analysis of the foF2 hourly data, opportunely catalogued in different levels of magneto-ionospheric conditions, highlights the role of the geomagnetic activity in the secular change of the ionosphere and confirms the latitudinal dependence of the trends. These results suggest interesting relations with some recent findings on the rapid decrease of some important physical and statistical quantities related to the geomagnetic field over the whole globe and mainly in Antarctica. In this paper we discuss the possibility of a connection between the ionospheric trends and a possible imminent geomagnetic reversal or excursion.
    Description: In press
    Description: 3.9. Fisica della magnetosfera, ionosfera e meteorologia spaziale
    Description: JCR Journal
    Description: open
    Keywords: Long term trends ; polar ionosphere ; monlinear phenomena ; 01. Atmosphere::01.02. Ionosphere::01.02.99. General or miscellaneous ; 05. General::05.07. Space and Planetary sciences::05.07.01. Solar-terrestrial interaction
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: manuscript
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  • 8
    Publication Date: 2017-04-04
    Description: We assess the first mission of the GEOSTAR (GEophysical and Oceanographic STation for Abyssal Research) deep-sea multidisciplinary observatory for its technical capacity, performance and quality of recorded data. The functioning of the system was verified by analyzing oceanographic, seismological and geomagnetic measurements. Despite the mission’s short duration (21 days), its data demonstrated the observatory’s technological reliability and scientific value. After analyzing the oceanographic data, we found two different regimes of seawater circulation and a sharp and deepening pycnocline, linked to a down-welling phenomenon. The reliability of the magnetic and seismological measurements was evaluated by comparison with those made using on-land sensors. Such comparison of magnetic signals recorded by permanent land geomagnetic stations and GEOSTAR during a “quiet” day and one with a magnetic storm confirmed the correct functioning of the sensor and allowed us to estimate the seafloor observatory’s orientation. The magnitudes of regional seismic events recorded by our GEOSTAR seismometer agreed with those computed from land stations. GEOSTAR has thus proven itself reliable for integrating other deep-sea observation systems, such as modular observatories, arrays, and instrumented submarine cables
    Description: Published
    Description: 361-373
    Description: open
    Keywords: oceanographic data ; magnetic data ; seismological data ; 05. General::05.02. Data dissemination::05.02.99. General or miscellaneous
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
    Format: 1856236 bytes
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  • 9
    Publication Date: 2017-04-04
    Description: From the three-component magnetic field observations taken from 1988 to 2005 during the measurement of Albanian and Italian magnetic repeat station network, as well as from a selected set of Ørsted satellite total field measurements, a geomagnetic reference model is determined for the region comprising the Albanian territory, the south-east part of the Italian Peninsula and the Ionian Sea. This model is designed to represent the components X,Y,Z and the total intensity F of the main geomagnetic field for epochs between 1990 and 2005 with prediction to 2008. The model is based on an expansion of the magnetic potential in terms of spherical cap harmonics applied to a cap of semi angle 8≅ . The model can be used as a reference model to reduce magnetic surveys undertaken in the area during the time of validity of the model, including also epochs up to 2008 for which the model is predictive.
    Description: Published
    Description: 1-5
    Description: open
    Keywords: GEOMAGNETIC ; 04. Solid Earth::04.05. Geomagnetism::04.05.03. Global and regional models
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 10
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    Osservatorio Ximeniano di Firenze,
    Publication Date: 2017-04-04
    Description: Il campo magnetico terrestre è una proprietà intrinseca del nostro pianeta e di altri oggetti del sistema solare. Il Sole stesso possiede un forte campo magnetico che si inverte quasi ciclicamente ogni 10-11 anni; tale comportamento è visibile attraverso la medesima ciclicità delle macchie solari che denotano sulla superficie l’intensa attività magnetica della nostra stella. Il campo magnetico terrestre è importantissimo per la vita sulla Terra. Esso protegge il pianeta dalle particelle cariche provenienti dal Sole: con la sua presenza si oppone alla forza di questo vento solare che altrimenti spazzerebbe via gran parte dell’atmosfera terrestre, così come probabilmente è già avvenuto in passato con l’atmosfera di Marte.
    Description: Published
    Description: 43-50
    Description: open
    Keywords: geomagnetic ; 04. Solid Earth::04.01. Earth Interior::04.01.02. Geological and geophysical evidences of deep processes ; 04. Solid Earth::04.05. Geomagnetism::04.05.01. Dynamo theory ; 04. Solid Earth::04.05. Geomagnetism::04.05.02. Geomagnetic field variations and reversals
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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