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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Bulletin of volcanology 53 (1991), S. 579-596 
    ISSN: 1432-0819
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Notes: Abstract The Inyo Craters (North Inyo Crater and South Inyo Crater), and a third crater, Summit Crater, are the largest of more than a dozen 650- to 550-yr-B.p. phreatic craters that lie in a 1-km-square area at the south end of the Inyo Volcanic Chain, on the west side of the Long Valley Caldera in eastern California. The three craters are aligned within a 1-km-long northsouth system of fissures and normal faults, and coincide in age with aligned magmatic vents farther north in the Inyo Volcanic Chain, suggesting that they were all produced by intrusion of one or more dikes. To study the sequence and mechanisms of the eruptions, the deposits were mapped, sampled, and compared with subsurface stratigraphy obtained from the core of a slant hole drilled directly below the center of South Inyo Crater from the southwest. The deposits from the two Inyo Craters are fine-grained (median diameter less than 1 mm), are several meters thick at the crater walls, and cover at most a few km2 of ground surface. Stratigraphic relationships between the Inyo Craters and Summit Crater indicate that the eruptions proceeded from north to south, overlapped slightly in time, and produced indistinctly plane-parallel bedded, poorly sorted deposits, containing debris derived primarily from within 450 m of the surface. Debris from the deepest identifiable unit (whose top is at 450 m depth) is present at the very base of both Inyo Craters deposits, suggesting that the eruptive vents were open and tapping debris from at least that depth, probably along preexisting fractures, even at their inception. According to ballistic studies, the greatest velocity of ejected blocks was of the order of 100 m/s. All eruptions, particularly the least powerful, selectively removed debris from the finest-grained, most easily eroded subsurface units. Although juvenile fragments have been previously identified in these deposits, they are confined primarily to the grain-size fraction smaller than 0.25 mm dia. and probably did not constitute more than several percent of the deposit. It is therefore suggested that these juvenile fragments were not the main source of heat for the eruptions, and that the eruptions were caused either by: (1) heating of water by fragmented magma that was not ejected before the eruption shut off; (2) slow heating (over months to years) of groundwater under confined conditions without fragmentation of magma, followed by a second process (pressure buildup, seismic faulting, or intrusions) that breached the confinement; or (3) breach of a pre-existing confined geothermal aquifer.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Bulletin of volcanology 57 (1995), S. 85-98 
    ISSN: 1432-0819
    Keywords: Key words Thermodynamics ; Gas eruptions ; Steam-blast eruptions
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Notes: Abstract  Eruptions of gas or steam and non-juvenile debris are common in volcanic and hydrothermal areas. From reports of non-juvenile eruptions or eruptive sequences world-wide, at least three types (or end-members) can be identified: (1) those involving rock and liquid water initially at boiling-point temperatures ('boiling-point eruptions'); (2) those powered by gas (primarily water vapor) at initial temperatures approaching magmatic ('gas eruptions'); and (3) those caused by rapid mixing of hot rock and ground- or surface water ('mixing eruptions'). For these eruption types, the mechanical energy released, final temperatures, liquid water contents and maximum theoretical velocities are compared by assuming that the erupting mixtures of rock and fluid thermally equilibrate, then decompress isentropically from initial, near-surface pressure (?10 MPa) to atmospheric pressure. Maximum mechanical energy release is by far greatest for gas eruptions (?∼1.3 MJ/kg of fluid–rock mixture) – about one-half that of an equivalent mass of gunpowder and one-fourth that of TNT. It is somewhat less for mixing eruptions (?∼0.4 MJ/kg), and least for boiling-point eruptions (?∼0.25 MJ/kg). The final water contents of erupted boiling-point mixtures are usually high, producing wet, sloppy deposits. Final erupted mixtures from gas eruptions are nearly always dry, whereas those from mixing eruptions vary from wet to dry. If all the enthalpy released in the eruptions were converted to kinetic energy, the final velocity (νmax) of these mixtures could range up to 670 m/s for boiling-point eruptions and 1820 m/s for gas eruptions (highest for high initial pressure and mass fractions of rock (m r) near zero). For mixing eruptions, νmax ranges up to 1150 m/s. All observed eruption velocities are less than 400 m/s, largely because (1) most solid material is expelled when m r is high, hence νmax is low; (2) observations are made of large blocks the velocities of which may be less than the average for the mixture; (3) heat from solid particles is not efficiently transferred to the fluid during the eruptions; and (4) maximum velocities are reduced by choked flow or friction in the conduit.
    Type of Medium: Electronic Resource
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  • 3
    Publication Date: 2021-12-22
    Description: Eruptive columnmodels are powerful tools for investigating the transport of volcanic gas and ash, reconstructing past explosive eruptions, and simulating future hazards. However, the evaluation of these models is challenging as it requires independent estimates of themainmodel inputs (e.g.mass eruption rate) and outputs (e.g. column height). There exists no database of independently estimated eruption source parameters (ESPs) that is extensive, standardized, maintained, and consensus-based. This paper introduces the Independent Volcanic Eruption Source Parameter Archive (IVESPA, ivespa.co.uk), a community effort endorsed by the International Association of Volcanology and Chemistry of the Earth’s Interior (IAVCEI) Commission on Tephra HazardModelling.We compiled data for 134 explosive eruptive events, spanning the 1902-2016 period, with independent estimates of: i) total erupted mass of fall deposits; ii) duration; iii) eruption column height; and iv) atmospheric conditions. Crucially, we distinguish plume top versus umbrella spreading height, and the height of ash versus sulphur dioxide injection. All parameter values provided have been vetted independently by at least two experts. Uncertainties are quantified systematically, including flags to describe the degree of interpretation of the literature required for each estimate. IVESPA also includes a range of additional parameters such as total grain size distribution, eruption style, morphology of the plume (weak versus strong), and mass contribution from pyroclastic density currents, where available. We discuss the future developments and potential applications of IVESPA and make recommendations for reporting ESPs to maximize their usability across different applications. IVESPA covers an unprecedented range of ESPs and can therefore be used to evaluate and develop eruptive column models across a wide range of conditions using a standardized dataset.
    Description: Published
    Description: 107295
    Description: 5V. Processi eruttivi e post-eruttivi
    Description: JCR Journal
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 4
    Publication Date: 2024-02-09
    Description: Rapid and simple estimation of the mass eruption rate (MER) from column height is essential for real-time volcanic hazard management and reconstruction of past explosive eruptions. Using 134 eruptive events from the new Independent Volcanic Eruption Source Parameter Archive (IVESPA, v1.0), we explore empirical MER-height relationships for four measures of column height: spreading level, sulfur dioxide height, and top height from direct observations and as reconstructed from deposits. These relationships show significant differences and highlight limitations of empirical models currently used in operational and research applications. The roles of atmospheric stratification, wind, and humidity remain challenging to detect across the wide range of eruptive conditions spanned in IVESPA, ultimately resulting in empirical relationships outperforming analytical models that account for atmospheric conditions. This finding highlights challenges in constraining the MER-height relation using heterogeneous observations and empirical models, which reinforces the need for improved eruption source parameter data sets and physics-based models.
    Description: Published
    Description: e2022GL102633
    Description: OSV2: Complessità dei processi vulcanici: approcci multidisciplinari e multiparametrici
    Description: JCR Journal
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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