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  • 1
    Publication Date: 2023-08-22
    Description: We present here paleomagnetic and magnetic anisotropy data from discrete samples collected in the middle Eocene to early Miocene sediment recovered in International Ocean Discovery Program (IODP) Sites U1507 and U1511 (Expedition 371, Tasman Sea, 27 July to 26 September 2017). Data consists of three tables (Table S2, S3, S4). Table S2 contains the paleomagnetic directions from discrete specimens collected in both Hole U1507B and Hole U1511B. The samples were measured for their paleomagnetic signal at the University of Bremen (Germany) between 2019 and 2021. Paleomagnetic inclinations are listed before and after correction for inclination shallowing. Table S3 contains the anisotropy of magnetic susceptibility (AMS) of representative specimens from Hole U1507B. Table S4 contains the anisotropy of anhysteretic remanent magnetization (AARM) of representative specimens from Hole U1507B. Both the AMS and AARM data of tables S3 and S4 were acquired at the University of Turin (Italy) between 2020 and 2021. These data were used for determining the absolute paleolatitude of northern Zealandia between the middle Eocene and the early Miocene (Dallanave et al., 2022; doi:10.1029/2022JB024736).
    Keywords: IODP Exp. 371; Site U1507; Site U151; Tasman Sea
    Type: Dataset
    Format: application/zip, 3 datasets
    Location Call Number Limitation Availability
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  • 2
    Publication Date: 2023-08-22
    Keywords: 371-U1507B; Anisotropy of anhysteretic remanent magnetization, K int declination; Anisotropy of anhysteretic remanent magnetization, K int inclination; Anisotropy of anhysteretic remanent magnetization, K int normalized; Anisotropy of anhysteretic remanent magnetization, K max declination; Anisotropy of anhysteretic remanent magnetization, K max inclination; Anisotropy of anhysteretic remanent magnetization, K max normalized; Anisotropy of anhysteretic remanent magnetization, K min declination; Anisotropy of anhysteretic remanent magnetization, K min inclination; Anisotropy of anhysteretic remanent magnetization, K min normalized; DEPTH, sediment/rock; DRILL; Drilling/drill rig; DSDP/ODP/IODP sample designation; Exp371; IODP Depth Scale Terminology; IODP Exp. 371; Joides Resolution; Sample code/label; Site U1507; Site U151; Tasman Frontier Subduction Initiation and Paleogene Climate; Tasman Sea
    Type: Dataset
    Format: text/tab-separated-values, 350 data points
    Location Call Number Limitation Availability
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  • 3
    Publication Date: 2023-08-22
    Keywords: 371-U1507B; 371-U1511B; ChRM, Declination; ChRM, Inclination; Date/Time of event; DEPTH, sediment/rock; DRILL; Drilling/drill rig; DSDP/ODP/IODP sample designation; Event label; Exp371; Inclination; IODP Depth Scale Terminology; IODP Exp. 371; Joides Resolution; Latitude of event; Longitude of event; Maximum angular deviation; Number of points; Sample code/label; Site U1507; Site U151; Tasman Frontier Subduction Initiation and Paleogene Climate; Tasman Sea
    Type: Dataset
    Format: text/tab-separated-values, 1404 data points
    Location Call Number Limitation Availability
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  • 4
    Publication Date: 2023-08-22
    Keywords: 371-U1507B; Anisotropy-magnetic susceptibility, factor Pj; Anisotropy-magnetic susceptibility, factor T; Anisotropy-magnetic susceptibility, K int declination; Anisotropy-magnetic susceptibility, K int inclination; Anisotropy-magnetic susceptibility, K int normalized; Anisotropy-magnetic susceptibility, K max declination; Anisotropy-magnetic susceptibility, K max inclination; Anisotropy-magnetic susceptibility, K max normalized; Anisotropy-magnetic susceptibility, K min declination; Anisotropy-magnetic susceptibility, K min inclination; Anisotropy-magnetic susceptibility, K min normalized; DEPTH, sediment/rock; DRILL; Drilling/drill rig; DSDP/ODP/IODP sample designation; Exp371; IODP Depth Scale Terminology; IODP Exp. 371; Joides Resolution; Sample code/label; Site U1507; Site U151; Tasman Frontier Subduction Initiation and Paleogene Climate; Tasman Sea
    Type: Dataset
    Format: text/tab-separated-values, 420 data points
    Location Call Number Limitation Availability
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  • 5
    Publication Date: 2021-11-29
    Description: L’eruzione pliniana delle Pomici di Avellino rappresenta uno dei principali eventi esplosivi nell’area Mediterranea dell’Olocene. Le eruzioni pliniane costituiscono uno fra gli eventi naturali potenzialmente più dannosi per le vite umane e l’ambiente. Esse sono generalmente caratterizzate da fasi esplosive sostenute molto energetiche, che possono durare diverse ore, con Intensità non inferiori a 107 -108 kg s-1 . Queste caratteristiche portano alla formazione di colonne convettive stratosferiche, la cui instabilità e collasso possono generare correnti piroclastiche di densità (PDC)1 , che si formano quando miscele di gas e particelle solide, emesse durante le eruzioni, collassano e scorrono al suolo sotto l’effetto della gravità2 . Le PDC possono devastare completamente le zone circostanti il vulcano fino a decine di chilometri di distanza. Distanze di centinaia di chilometri dal centro eruttivo, nella direzione del vento dominante caratterizzano, invece, i depositi da caduta associati alle fasi di colonna sostenuta. Nell’insieme, si tratta di eventi molto rari alla scala della vita umana, per cui la loro dinamica eruttiva viene ricostruita principalmente sulla base dello studio dei depositi delle eruzioni passate. Tali studi sono particolarmente importanti nel caso di vulcani quiescenti, la cui riattivazione e comportamento eruttivo sono difficili da definire in assenza di attività frequente3 .
    Description: Published
    Description: 41-55
    Description: 5V. Processi eruttivi e post-eruttivi
    Keywords: L’eruzione pliniana ; Nola - Croce del Papa
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: book chapter
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  • 6
    Publication Date: 2021-11-29
    Description: In the last decades, palaeomagnetic research has provided us with a picture of the temporal and spatial behaviour of the Earth’s magnetic field (EMF) from its origin up to the present day. Well-dated palaeomagnetic data offer important sources of information about the past variation of the geomagnetic field and have shown that it is characterized by temporal fluctuations such as reversals, excursions and spikes. Despite the advances in our understanding of EMF behaviour, the current dataset is biased towards high and northern latitudes and, therefore, several questions remain open to debate, such as the origin and evolution of the EMF and the frequency and spatial distribution of its variations. This Special Publication focuses on the study of the temporal and spatial evolution of the EMF in the past through new data from palaeomagnetic and rock magnetic studies of archaeological materials, sediments and lavas from Europe, Africa, Australia, New Zealand, India and Baltic Sea, and their applications in archaeology, stratigraphy and climate. This paper summarizes our current knowledge on geomagnetic field variations in the past, open questions and future challenges and gives an overview of the volume’s context, which aims to disclose fundamental properties of the Earth’s magnetic field evolution.
    Description: Published
    Description: 1-8
    Description: 1A. Geomagnetismo e Paleomagnetismo
    Description: N/A or not JCR
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: book chapter
    Location Call Number Limitation Availability
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  • 7
    Publication Date: 2021-11-29
    Description: Speleothems are potentially excellent archives of the Earth’s magnetic field, capable of recording its past variations. Their characteristics, such as the continuity of the record, the possibility to be easily dated, the almost instantaneous remanence acquisition and the high time-resolution make them potentially unique high-quality Paleosecular Variation (PSV) recorders. Nevertheless, speleothems are commonly characterized by low magnetic intensities, which often limits their resolution. Here we present a paleomagnetic study performed on two cores from a flowstone from the Rio Martino Cave (Western Alps, Italy). U/Th dating indicates that the flowstone’s deposition covers almost the entire Holocene, spanning the period ca. 0.5–9.0 ka, while an estimation of its mean growth rate is around 1 mm per 15 years. The flowstone is composed of columnar calcite, characterized by a highly magnetic detrital content from meta-ophiolites in the cave’s catchment. This favorablegeological context results in an intense magnetic signal that permits the preparation and measurement of thin (∼3 mm depth equivalent) samples, each representing around 45 yr. The Characteristic Remanent Magnetization (ChRM), isolated after systematic stepwise Alternating Field demagnetization, is well defined, with Maximum Angular Deviation (MAD) generally lower than 10◦. Paleomagnetic directional data allow the reconstruction of the PSV path during the Holocene for the area. Comparison of the new data with archeomagnetic data from Italian archeological and volcanic records and using the predictions of the SHA.DIF.14k and pfm9k.1a global geomagnetic field models shows that the Rio Martino flowstone represents an excellent recorder of the Earth’s magnetic field during the last 9,000 years. Our high resolution paleomagnetic record, anchored by a high-quality chronology, provides promising data both for the detection of short term geomagnetic field variations and for complementing existing regional PSV curves for the prehistoric period, for which well-dated data are still scarce
    Description: Published
    Description: 32-42
    Description: 1A. Geomagnetismo e Paleomagnetismo
    Description: JCR Journal
    Keywords: Paleosecular variation ; rock magnetism ; speleothem
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 8
    Publication Date: 2021-11-29
    Description: Disentangling the effects of climate and human impact on the long-term evolution of the Earth Critical Zone is crucial to understand the array of its potential responses to the ongoing Global Change. This task requires natural archives from which local information about soil and vegetation can be linked directly to climate parameters. Here we present a high-resolution, well-dated, speleothem multiproxy record from the SW Italian Alps, spanning the last ~10,000 years of the present interglacial (Holocene). We correlate magnetic properties and the carbon stable isotope ratio to soil stability and pedogenesis, whereas the oxygen isotope composition is interpreted as primarily related to precipitation amount, modulated at different timescales by changes in precipitation source and seasonality. During the 9.7-2.8 ka period, when anthropic pressure over the catchment was scarce, intervals of enhanced soil erosion are related to climate-driven vegetation contractions and occurred during drier periods. Immediately following the onset of the Iron Age (ca. 2.8 ka), by contrast, periods of enhanced soil erosion coincided with a wetter climate. We propose that the observed changes in the soil response to climate forcing were related to early anthropogenic manipulations of Earth's surface, which made the ECZ more sensitive to climate oscillations.
    Description: University of Pisa (Fondi di Ateneo assigned to ER and GZ)Australian Research Council Discovery Project scheme (grant number DP160102969, assigned to RND, JH, GZ and ER)the National Geographic Society (CP-073ER-17)
    Description: Published
    Description: id 17829
    Description: 5A. Ricerche polari e paleoclima
    Description: JCR Journal
    Keywords: speleothem ; magnetism ; stable isotope geochemistry ; Earth Critical Zone ; Anthropocene ; Alps ; the effects of climate and human impact
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 9
    Publication Date: 2021-11-29
    Description: L’eruzione pliniana delle Pomici di Avellino rappresenta uno dei principali eventi esplosivi nell'area Mediterranea dell’Olocene. Le eruzioni pliniane costituiscono uno fra gli eventi naturali potenzialmente più dannosi per le vite umane e l’ambiente. Esse sono generalmente caratterizzate da fasi esplosive sostenute molto energetiche, che possono durare diverse ore, con Intensità non inferiori a 107 -108 kg s-1. Queste caratteristiche portano alla formazione di colonne convettive stratosferiche, la cui instabilità e collasso possono generare correnti piroclastiche di densità (PDC)1 , che si formano quando miscele di gas e particelle solide, emesse durante le eruzioni, collassano e scorrono al suolo sotto l’effetto della gravità2 . Le PDC possono devastare completamente le zone circostanti il vulcano fino a decine di chilometri di distanza. Distanze di centinaia di chilometri dal centro eruttivo, nella direzione del vento dominante caratterizzano,invece,i depositi da caduta associati alle fasi di colonna sostenuta. Nell’insieme, si tratta di eventi molto rari...
    Description: Published
    Description: 41-56
    Description: 1V. Storia eruttiva
    Description: 6V. Pericolosità vulcanica e contributi alla stima del rischio
    Keywords: eruzione Pomici di Avellino ; Nola - Croce del Papa
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: book chapter
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