Author(s):  
Emanuele Marchetti ◽  
Maurizio Ripepe ◽  
Giacomo Ulivieri ◽  
Michael R. Burton ◽  
Tommaso Caltabiano ◽  
...  

Keyword(s):  

Lava samples, collected periodically during the 1971 eruption of Mt Etna, have been analysed. A certain evolution of their composition has been observed: the first lavas are phonolitic tephrites, while the last ones are mugearites. This evolution can be explained by assuming a pneumatolytic differentiation in the uppermost parts of the magma column and a subtraction of femic phenocrysts by gravitational differentiation in its deeper parts, where the last products originated. Furthermore, the analyses of the 1971 lavas are compared with all available data of ancient products of this complex volcano and, particularly, with those of its historical eruptions.


1988 ◽  
Vol 25 (7) ◽  
pp. 1000-1019 ◽  
Author(s):  
Stephen A. Shaver

Each of the two quartz monzonite porphyry intrusions that form the Hall stock contains four phases concentrically zoned from fine-grained, groundmass-rich, silicic (70–73 wt. % SiO2) phases at the top and margin toward deeper phases that are progressively coarser, more equigranular, and richer in plagioclase and biotite (68–72 wt. % SiO2). In each stock, the depthwise decrease in groundmass is not continuous but is interrupted by flow-foliated, gradational contacts (at 60–70, 50, and 10 vol. % groundmass) at or above which concentrations of quartz–molybdenite veins and (or) other SiO2-rich features are common. Magma supercooling is documented by quartz–K-feldspar dendrites and crenulate quartz layers at phase contacts. Rare sharp contacts and xenoliths document that all phases are temporally distinct, with earliest phases at the top and margin and progressively later phases inward and with depth. However, gradational contacts, concentricity of phases, and unidirectionality of textural–compositional zoning argue that each stock developed from a single magma column whose progressively inward crystallization was episodically interrupted by the release of molybdenum-bearing fluids to produce stacked orebodies. Conductive heat-loss modeling indicates that each stock took ≤ 1130 years to (i) cool to solidus temperature (740–750 °C) and (ii) form three distinct molybdenum shells. Not only is progressively deeper fluid release from concentrically zoned textural phases of a single magma column previously undocumented, but also the short cooling interval in each stock implies very rapid rates of volatile migration in these systems and thus very rapid development of vertical compositional gradients.


The summit cone of Mt Etna is cut by an approximately NNE-SSW trending, narrow fissure zone that controls much of the terminal activity of this volcano. Within the central crater, which lies at the top of the summit cone, there are two main vents alined on this fissure zone: the chasm, a deep pit; and the 1964 crater. Both of these vents were blocked before 1971. The NE crater first opened in 1911 on the lower slopes of the summit cone on the same fissure zone, and has had an open conduit from which lava has been erupted at a constant rate from 1966 to the beginning of the 1971 eruption. In 1968 a small gas bocca known as the Bocca Nuova opened near a fissure that had previously erupted lavas in 1956. The Bocca Nuova collapsed in early 1970 to give a 100 m wide crater. It is suggested that collapse resulted from movement of magma at depth into the 1956 fissure causing sudden lowering in the magma column below the Bocca, and that continued migration of magma into the fissure eventually lead to the eruption of April 1971, the site of this eruption being in line with the fissure. A rise in temperature of fumaroles at the edge of the central crater after the Bocca Nuova collapse is attributed to this incursion of magma across the crater.


The author believes the 1971 eruption has been triggered by an uprise of the magma column which had for several decades fed the persistent activity located in both the NE crater and in the central crater’s chasm. This uprise split open a set of en-echelon fissures first on the southern, then on the eastern upper slopes of Mt Etna. Degassing occurred at the uppermost part of the successive fissure systems, while the degassed lava flows poured out at the lowermost end. When the ENE tectonic fault-system came into operation and controlled the second half of the eruption, it led to the engulfment of the degassing vent and subsequently acted as an undergound channel through which the degassed lavas could flow freely until they poured out at the lower end of the fault zone. This fault zone follows one of the main tectonic trends which intersect below Mt Etna, the main other ones being oriented SW-NE and WSW—ENE.


2016 ◽  
Vol 80 (2) ◽  
pp. 213-225 ◽  
Author(s):  
R. G. Cawthorn ◽  
K. L. Lundgaard ◽  
C. Tegner ◽  
J. R. Wilson

AbstractMany layered intrusions are considered to have been repeatedly inflated by magma additions, but rates of magma mixing relative to rates of layer accumulation are difficult to model. The nature of magma recharge through the interval including the Pyroxenite Marker (PM), Main Zone, Bushveld Complex, South Africa, is examined with regard to such processes. The plagioclase compositions (An value) in five previously published and three new profiles (presented here and focusing on the core compositions) that are at least 600 m in vertical extent and spread along a strike length of 110 km are evaluated. The compilation of the eight profiles shows the following trends. Upward reversals in compositions show considerable lateral as well as vertical variations. Lateral variations show a range in: (1) the minimum An value reached in each profile prior to the onset of magma recharge (An51 to An59); (2) the depth below the PM at which the minimum value is observed (50 to 575 m); (3) the An value close to the PM (An54 to An75); (4) the maximum value recorded above the PM (An63 to An76); (5) the height above the PM at which this maximum value is reached (0 to 300 m) – in all cases, the highest values of An occur at the northern end of the studied sections; and (6) the vertical extents over which the reversals occur range from 150 to over 600 m indicating very protracted magma additions and/or slow mixing. The PM terminates toward the south, and close to this termination the immediate footwall rocks to the PM change from north to south from gabbronorite to magnetite gabbronorite. A cross-section through these profiles defines two basins, with an intervening structural upwarp. The magma pulses that were added to produce very gradual and protracted reversals in mineral compositions through the PM interval ponded initially at the base of the northern basin, and did not homogenize the entire magma column. These added magmas did not overflow and have an effect on mineral compositions in the southern basin until after considerable replenishment and crystallization (including the PM) had taken place in the northern basin. We emphasize the prolonged period(s) of magma input and slow rate of vertical homogenization of the magma column during the formation of this sequence of as much as 400 m of the Main Zone.


2021 ◽  
Vol 11 (1) ◽  
Author(s):  
M. Ripepe ◽  
D. Delle Donne ◽  
D. Legrand ◽  
S. Valade ◽  
G. Lacanna

AbstractVolcano seismicity is one of the key parameters to understand magma dynamics of erupting volcanoes. However, the physical process at the origin of the resulting complex and broadband seismic signals remains unclear. Syn-eruptive very long period (VLP) seismic signals have been explained in terms of the sudden expansion of gas pockets rising in the liquid melt. Their origin is linked to a magma dynamics which triggers the explosive process occurring before the explosive onset. We provide evidence based on acoustic, thermal, and ground deformation data to demonstrate that VLP signals at Stromboli are generated at the top of the magma column mainly after the explosion onset. We show that VLP amplitude and duration scale with the eruptive flux which induces a decompression of 103–104 Pa involving the uppermost ~ 250 m of the feeding conduit. The seismic VLP source represents the final stage of a ~ 200 s long charge and discharge mechanism the magma column has to release excess gas accumulated at the base of a denser and degassed magma mush. The position of the VLP seismic source coincides with the centroid of the shallow mush plug and tracks elevation changes of the magma free surface.


Geology ◽  
1995 ◽  
Vol 23 (12) ◽  
pp. 1091 ◽  
Author(s):  
Hiroshi Shinohara ◽  
Kohei Kazahaya ◽  
Jacob B. Lowenstern

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