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  • 11
    Publication Date: 2017-04-04
    Description: Volcanomagnetic monitoring is critically dependent on the ability to detect and isolate local magnetic variations related to volcanic activity. Accurate detection of volcanomagnetic anomalies attributable to the dynamics of volcanoes requires removal from measurements of the Earth’s magnetic field, fluctuations of external origin which may be up to hundreds of nanotesla during geomagnetic storms. The commonly used method of taking simple differences of the total intensity with respect to the simultaneous value at a remote reference is only partially successful. Variations in the difference fields are thought to arise principally from contrasting electromagnetics of rock properties at magnetometer sites. With the aim of improving the noise reduction of geomagnetic time series from the magnetic network of Mt Etna, we developed an adaptive filtering. Magnetic vector data are included as input to the filter, to account for the orientation of the magnetic field. The filter is able to estimate and adapt the model parameters continuously by means of the new observations, so that the estimated signal closely matches the observed data. Therefore, the filtering accuracy is improved in order to reduce the residual components. Experimental data collected on Mt Etna during 2010 are analysed to relate the field variation at a given station to the field at other sites, filtering out undesired noise and enhancing signal-to-noise ratio.
    Description: Published
    Description: 291-304
    Description: 1.6. Osservazioni di geomagnetismo
    Description: N/A or not JCR
    Description: reserved
    Keywords: Volcanomagnetic monitoring ; Mt Etna ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 12
    Publication Date: 2017-04-04
    Description: Significant changes in the local magnetic field marked the resumption of eruptive activity at Stromboli volcano on February 27, 2007. After differential magnetic fields were obtained by filtering out external noise using adaptive filters and seasonal thermal noise using temperature data, we identified step-like changes of 1–4 nT coincident with the opening of eruptive fissures in the upper part of the Sciara del Fuoco. The magnetic variations detected at two stations are closely related to the propagation of a shallow NE–SW magmatic intrusion extending beyond the summit craters area. These observations are consistent with those calculated using piezomagnetic models in which stress-induced changes in rock magnetization are produced by the magmatic intrusion. No significant magnetic changes were observed when the first fractures opened along the NE crater rim. Indeed, the stressinduced magnetization caused by this magmatic activity is expected to be too low because of the structural weakness and/or thermal state of the summit area. The continuous long-term decay characterizing the post-eruptive magnetic pattern can be related to a time-dependent relaxation process. A Maxwell rheology was assumed and the temporal evolution of the piezomagnetic field was evaluated. This allowed us to estimate the rheological properties of the medium; in particular, an average viscosity ranging between 1016 and 1017 Pa⋅s was a relaxation time τ of about 38 days.
    Description: Published
    Description: 1311–1322
    Description: 1.6. Osservazioni di geomagnetismo
    Description: JCR Journal
    Description: reserved
    Keywords: Stromboli Island ; Magnetic monitoring ; Piezomagnetic field ; Stress field ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 13
    Publication Date: 2017-04-04
    Description: Long-term and high temporal resolution gravity and deformation data move us toward a better understanding of the behavior of Mt Etna during the June 1995 – December 2011 period in which the volcano exhibited magma charging phases, flank eruptions and summit crater activity. Monthly repeated gravity measurements were coupled with deformation time series using the Differential Synthetic Aperture Radar Interferometry (DInSAR) technique on two sequences of interferograms from ERS/ENVISAT and COSMO-SkyMed satellites. Combining spatiotemporal gravity and DInSAR observations provides the signature of three underlying processes at Etna: (i) magma accumulation in intermediate storage zones, (ii) magmatic intrusions at shallow depth in the South Rift area, and (iii) the seaward sliding of the volcano’s eastern flank. Here we demonstrate the strength of the complementary gravity and DInSAR analysis in discerning among different processes and, thus, in detecting deep magma uprising in months to years before the onset of a new Etna eruption.
    Description: Published
    Description: 3089
    Description: 2V. Dinamiche di unrest e scenari pre-eruttivi
    Description: JCR Journal
    Description: restricted
    Keywords: Microgravity ; Ground deformation ; SAR Interferometry ; Volcano monitoring ; Etna volcano ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 14
    Publication Date: 2020-02-24
    Description: Advances in volcano monitoring and forecasting need a multidisciplinary collaborative framework. In light of this, a Bayesian Event Tree (BET) approach was performed by the application of the BET for Eruption Forecasting (BET_EF) code to analyze the space-time distribution of the volcanic activity of Mount Etna from 2001-2005. First, a reliable monitoring dataset was set up after some sessions to elicit geophysical, volcanological and geochemical ‘precursor’ parameters. A constant unrest probability of 100%, with a magma involvement usually greater than 95%, was computed throughout the time period analyzed. Eruption probabilities higher than 90% were estimated a few days before the onsets of the 2001 and 2002-2003 flank eruptions. Values slightly higher than 75% were observed during the lava fountaining period in June-July 2001. However, the probabilities flattened to around 30% for the 2004-2005 flank eruption. With suitable data, a good depiction of the actual location of the eruptive scenario for the 2001 and 2002-2003 events was provided. Conversely, the size of the eruptions was not indicated.
    Description: Published
    Description: 642-661
    Description: 1.6. Osservazioni di geomagnetismo
    Description: JCR Journal
    Description: open
    Keywords: Volcano monitoring ; Statistical analysis ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 15
    Publication Date: 2020-05-29
    Description: Gravity time sequences collected at Etna volcano by continuously recording spring-based relative gravimeters showed significant variations in temporal correspondence with paroxysmal eruptions. Since the observed gravity variations can only be partially related to subsurface mass redistribution phenomena, we investigated on the instrumental effects due to the ground vibrations as those accompanying explosive activity. We simulated the performances of relative gravimeters through laboratory experiments to estimate their response to vertical and horizontal excitations. Laboratory tests were carried out using a vibrating platform capable of accelerating the instruments with intensities and frequencies, in both the vertical and horizontal directions, observed in the ground vibrations associated with paroxysmal events. The seismic signals recorded at Etna volcano during the 10 April 2011 lava fountain were analyzed to retrieve the parameters used to drive the vibration platform. We tested two gravimeters used for Etna volcano monitoring: the LaCoste & Romberg D#185 and the Scintrex CG-3M#9310234. The experimental results highlight that vibrations, resembling the seismic waves propagated during paroxysmal events, cause an amplitude response in the gravity readings of the order of several hundred of microGals. Generally the relationship between the vibrations and the gravimeter response is non-linear with a fairly complex dependence on the frequencies and amplitude of the signals acting on the gravimeters.
    Description: Published
    Description: 44
    Description: 2V. Dinamiche di unrest e scenari pre-eruttivi
    Description: JCR Journal
    Description: open
    Keywords: Spring-based relative gravimeter ; Vibrating platform ; Volcano monitoring ; Explosive eruptions ; Gravity changes ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 16
    Publication Date: 2017-04-04
    Description: Detection of local magnetic field perturbations has often been proposed for monitoring the modifications within the volcanic edifice of the stress field or of the thermodynamic state and providing a tool for prediction of eruptions. In order to evaluate the suitability of magnetic monitoring on Mt. Etna, we analysed two historic series of magnetic data recorded there: i) during the 1981 eruption and ii) immediately after 1989 eruption. Moreover, we examined time series associated with the intense explosive activity of Etna in 1995 summer provided by the present permanent magnetic network which was set up between 1994 and 1995.
    Description: Published
    Description: 725-730
    Description: 1.6. Osservazioni di geomagnetismo
    Description: JCR Journal
    Description: reserved
    Keywords: Volcanomagnetic effect ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 17
    Publication Date: 2017-04-04
    Description: Significant changes in the local magnetic field marked the resumption of the eruptive activity at Stromboli volcano on February 27, 2007. After differential magnetic fields were filtered from the external noise by adaptive filters and from the seasonal thermic noise using temperature data, we highlighted step-like changes of 1-4 nT coincident with the eruptive fissures opening in the upper part of the Sciara del Fuoco. The magnetic variations detected at 2 stations are closely related to the propagation of a shallow NE-SW magmatic intrusion outside the summit craters area . These observations are consistent with those calculated from piezomagnetic models, where stress-induced changes in rock magnetization are produced by the magmatic intrusion. No significant magnetic changes were observed when the first fractures opened along the NE crater rim. Indeed, the stress-induced magnetization caused by this magmatic activity is expected to be too low because of the structural weakness and/or thermal state of the summit area. The continuous long-term decay characterizing the post-eruptive magnetic pattern was related to a time-dependent relaxation process. A Maxwell rheology was assumed and the temporal evolution of the piezomagnetic field was evaluated. This allowed for the estimate of the rheological properties of the medium, in particular an average viscosity ranging between 1016 and 1017 Pas was achieved involving a relaxation time τ of about 38 days.
    Description: In press
    Description: 1.6. Osservazioni di geomagnetismo
    Description: JCR Journal
    Description: open
    Keywords: Stromboli Island ; magnetic monitoring ; piezomagnetic field ; stress field ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 18
    Publication Date: 2017-04-04
    Description: Nonlinear dynamic systems can be described by means of statistical learning theory: neural networks and kernel machines. In this work the recurrent least-squares support vector machines are chosen as learning system. The unknown dynamic system is a mapping of past states into the future. The recurrent system is implemented by special data preparation in the learning phase. The next iterations can be calculated but the convergence is usually not guaranteed. Due to the fact that the predicted trajectory can diverge from the real trajectory the semi-directed mode can be applied, i.e. after several prediction steps the system is updated by using the current values of the considered process as new initial conditions. The idea was tested on the data generated by the chaotic dynamic system – the Chua’s circuit. The methodology was then applied to real magnetic data acquired at Etna volcano.
    Description: Published
    Description: 213-218
    Description: 1.6. Osservazioni di geomagnetismo
    Description: reserved
    Keywords: recurrent ls-svm, ; volcanomagnetic dynamics ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: book chapter
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  • 19
    Publication Date: 2017-04-04
    Description: Over the past few decades we have been intensively monitoring the magnetic field on Mt. Etna. The largest anomaly, about 10 nT, was observed in the geo-magnetic time series recorded in 1981 and associated with the March 17-23 eruption. It was interpreted as the joint effect of piezomagnetism and thermal demagnetization engendered by an intrusive dike. A convincing case of thermo-magnetic effects was observed during the 1989 fissure eruption, when repeated measurements at intervals of 3 months for two years revealed the slow buildup of a 130 nT anomaly. The anomaly vanished laterally within 0.2 km from the sur-face expression of the fissure system. The nature and structure of the anomaly is consistent with the location and time of cooling of a shallow dike. Between Sep-tember and December 1995 geomagnetic changes, greater than 8 nT, associated with the renewal of the NE crater's activity were detected. The center of the magnetic anomaly source, which was thought to be the region heated by hightemperature fluids and gases originating from fresh magma, was estimated, by the spatial distribution of the variation rate, to be at a depth of 500 m near the 1991-93 eruptive vents. Finally, significant changes, ranging from 2 to 7 nT, in the local magnetic field closely related to the main phases of the 2001 eruption were observed. Piezomagnetic models were used to calculate the expected geo-magnetic changes for each volcanic process. Model parameters were based on estimated fault geometry using seismic and ground deformation data from each event.
    Description: Published
    Description: 241-262
    Description: 1.6. Osservazioni di geomagnetismo
    Description: reserved
    Keywords: magnetic field monitoring ; Etna ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: book chapter
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  • 20
    Publication Date: 2017-04-04
    Description: The volcanomagnetic monitoring is critically dependent on the ability to detect and isolate magnetic variations related to volcanic activity. Accurate detection of volcanomagnetic anomalies attributable to the volcano’s dynamics requires removing from measurements of the earth’s magnetic field, fluctuations of external origin which may be up to hundreds of nanotesla during geomagnetic storms. The commonly used method of taking simple differences of the total intensity with respect to the simultaneous value at a remote reference is partially successful. Variations in the difference fields arise principally from contrasting electromagnetic properties at magnetometer sites. To improve the noise reduction of geomagnetic data from magnetic network of Mt Etna we developed an adaptive filtering. Magnetic vector data are included as input to the filter, to account for the orientation of the disturbance field. The filter is able to estimate and rectify the model parameters continuously by means of new observations, so that predictions match the observed data. The error of state estimation has been decreased and the filtering accuracy improved. Experimental data collected on Mt Etna during 2010 are analyzed to relate the field variation at a given station to the field at other sites filtering out undesired noise and enhancing signal-to-noise ratio.
    Description: Submitted
    Description: 1.6. Osservazioni di geomagnetismo
    Description: N/A or not JCR
    Description: open
    Keywords: vectorial magnetometer ; volcanomagnetic monitoring ; 04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: manuscript
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