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191.
We report on the unusual occurrence of the products of lava fountaining in a Pliocene calc-alkaline rhyolitic monogenetic center from northern Chile. Corral de Coquena is a discontinuous ring of lava located in the moat of La Pacana caldera (23°27' S, 67°23.5' W), part of the Altiplano-Puna Volcanic Complex of the Central Andes. The volcanic structure is composed of a maar-like crater, with an associated pyroclastic (possibly phreatomagmatic) unit, that is overlain by rhyolitic glassy lava ramparts, in which evidence of spatter, agglutinate and clastogenic material is found. Typical explanations for the unusual textures in a rhyolitic lava, such as peralkaline composition, high volatile content, or superheated magma are untenable in this case. We propose that the most likely explanation for this extreme style of rhyolitic volcanism is a combination of moderately high eruption rate and efficient degassing prior to eruption. In the light of reports of several other bodies of fountain-fed silicic magma from the UK, US, and Japan, we propose that Corral de Coquena is a rhyolitic spatter ring superimposed upon a maar-like crater. We further propose that pyroclastic fountaining should be considered an end-member of the spectrum of eruptive styles of calc-alkaline silicic magmas, and that Corral de Coquena is a rare example, preserved because of the hyper-arid climate in the Altiplano-Puna Volcanic Complex.  相似文献   
192.
Explosive degassing at Erebus Volcano produces infrasound that can be used to locate, characterize, and quantify eruptive activity from multiple vents. We use a three element distributed microphone network to pinpoint eruption sources and track the activity at the prominent vents through time. Eruptive mechanisms for both source types are analyzed in conjunction with the telemetered time-synced video imagery. We identify two commonly active vents corresponding to the large (often > 10-m diameter) bubble bursts at the free surface of a persistent phonolitic lava lake (‘Ray Lake’), and the less frequent ash-rich eruptions from a constricted vent (‘Active Vent’) located ∼ 80 m from the lava lake. During a 3-month study interval from 6 January to 13 April 2006 we identified and mapped more than 350 eruptive sources from the lava lake and 20 sources from the ash vent. Lava lake events are characterized by high-amplitude infrasonic transients that reflect rapid (less than a few s) acceleration and rupture of magma bubble films followed by an explosion of pressurized gases. Precise infrasonic localization of the lava lake events to accuracies of a few m indicates variable bubble source locations across a 40 by 50-m region spanning the lava lake. Spatial variability is corroborated by the video data. In contrast, degassing from the ash vent produces longer-duration (tens of s), lower amplitude transients that reflect diminished impulsivity and an extended degassing duration, features that are corroborated by video. Because infrasound networks can operate continuously in all weather conditions and during both diurnal and seasonal polar darkness, and are easily incorporated into automatic processing, they significantly contribute to the completeness and quantification of eruption catalogues for Erebus.  相似文献   
193.
Mount Erebus, a large intraplate stratovolcano dominating Ross Island, Antarctica, hosts the world's only active phonolite lava lakes. The main manifestation of activity at Erebus volcano in December 2004 was as the presence of two convecting lava lakes within an inner crater. The long-lived Ray Lake, ~ 1400 m2 in area, was the site of up to 10 small Strombolian eruptions per day. A new but short-lived, ~ 1000–1200 m2 lake formed at Werner vent in December 2004 sourced by lava flowing from a crater formed in 1993 by a phreatic eruption. We measured the radiative heat flux from the two lakes in December 2004 using a compact infrared (IR) imaging camera. Daily thermal IR surveys from the Main Crater rim provide images of the lava lake surface temperatures and identify sites of upwelling and downwelling. The radiative heat outputs calculated for the Ray and Werner Lakes are 30–35 MW and 20 MW, respectively. We estimate that the magma flux needed to sustain the combined heat loss is ~ 250–710 kg s− 1, that the minimum volume of the magma reservoir is 2 km3, and that the radius of the conduit feeding the Ray lake is ~ 2 m.  相似文献   
194.
Estimating depths of buried lava tubes is important for determining the thermal budgets and effusion rates of basaltic volcanic systems. This research used a laboratory experiment scaled to a lava tube system to measure the 3D temperature field surrounding a hot viscous fluid flowing through a buried glass tube while varying conditions such as flow rate and temperature. The depth of the glass tube was changed for different experimental runs. Numerical techniques were applied to model the laboratory experiment. The surface thermal distributions from 166 thermal traverses, constrained to a depth to width ratio of 0.6 to 1.6, were analyzed to empirically derive a depth estimation function using regression techniques. This “Linear Anomaly Surface Transect (LAST)” depth function is a scaleable depth estimation technique which can be solved with thermal imaging data alone. The minimum temperature, maximum temperature and width of a Lorentzian distribution fit to a surface thermal transect, are the only inputs required for the LAST function to estimate the depths of the hot source. The input parameters were then applied to non-laboratory situations including the Kuhio lava tube system in Hawai’i. The LAST function produced depth estimates of ∼ 0.3 m for the Kuhio lava tube in Hawai’i, which did not agree with observations on the ground. This is the result of the complex composition and geometry of an actual lava tube where heat transfer is controlled by more than a simple fluid filling a tube, but also by convection of gasses and fluids in a partially filled passage. Though not effective for lava tubes at this time, the model provides promising results for simple cases applied to engineering and underground coal fires.  相似文献   
195.
Anisotropy of magnetic susceptibility (AMS) data analysis is a convenient method used to investigate strain and flow during lava flow emplacement. In order to make a sound interpretation, the origin of the AMS signal must be verified. Two questions must be answered: 1) what phase, or phases carry the AMS signal and 2) when was the AMS fabric acquired? The verification steps themselves can provide extra data for interpreting lava flow conditions. Here, we present a methodology to answer the two questions in a 6 km-long Chaîne des Puys trachybasaltic lava flow that descended into the future site of Clermont Ferrand (France) 45,000 years ago. Knowledge of lava flow emplacement will be useful specifically to this site, if a reactivation of the volcanic chain occurs. The results are also of more general interest to understand lava flow emplacement dynamics.  相似文献   
196.
辽西义县许家屯巨型枕状熔岩产在义县旋回第二亚旋回火山岩沉积夹层中.以其岩枕巨大(5~8m)、形态多样构成独特的火山岩景观.岩枕大体由冷凝边、过渡带和核部3部分组成,三者间在颜色、气孔和杏仁的数量与大小上彼此有别.它们的岩石学、地球化学特征完全可以和下伏火山岩对比,岩性属玄武安山岩.其是在第二亚旋回火山活动间歇期,岩浆再次溢出,涌流进水体(如湖泊)里冷凝而成为陆相环境产物,与海相玄武质枕状熔岩明显不同.  相似文献   
197.
Measurements of the anisotropy of magnetic susceptibility (AMS) of natural lavas have shown that AMS varies with depth within a lava flow. We have investigated the reasons for such variation by studying the effects of temperature and strain rate on the AMS of recent lava in the laboratory. Samples of lava from Kilauea were melted and subjected to a range of strain rate and cooling histories. The results show that the degree of anisotropy is a function of both the thermal and shearing history of a sample. High degrees of anisotropy were found only in samples that were deformed at temperatures close to those encountered during eruption and then rapidly quenched. Lavas subjected to similar shear stresses at high temperatures had low degrees of anisotropy if allowed to cool down slowly without further deformation. Additionally, lava subjected to complex shearing yield a lower degree of anisotropy even when high strain rates were imposed on it. These results lead to the conclusion that only the last phase of deformation is detectable using AMS and that high strain rates will not result in high degrees of anisotropy if either deformation ends while lava is still fluid or if the orientation of the maximum shear stress varies with time. The relation between the orientation of the principal susceptibilities and that of shear is less sensitive to variation on shear with time. Consequently, flow directions can be inferred confidently with this type of measurements.  相似文献   
198.
Following the eruption of January 1992, episodes of lava dome growth accompanied by generation of dome-collapse nuées ardentes occurred in 1994–1998. In addition, nuées ardentes were generated by fountain-collapse in January 1997, and the 1998 events also suggest an explosive component. Significant tilt and seismic precursors on varying time scales preceded these events. Deformation about the summit has been detected by electronic tiltmeters since November 1992, with inflation corresponding generally to lava dome growth, and deflation (or decreased inflation) corresponding to loss of dome mass. Strong short-term (days to weeks) accelerations in tilt rate and seismicity occurred prior to the major nuées ardentes episodes, apart from those of 22 November 1994 which were preceded by steadily increasing tilt for over 200 days but lacked short-term precursors. Because of the combination of populated hazardous areas and the lack of an issued warning, about 100 casualties occurred in 1994. In contrast, the strong precursors in 1997 and 1998 provided advance warning to observatory scientists, enabled the stepped raising of alert levels, and aided hazard management. As a result of these factors, but also the fortunate fact that the large nuées ardentes did not quite descend into populated areas, no casualties occurred. The nuée ardente episode of 1994 is interpreted as purely due to gravitational collapse, whereas those of 1997 and 1998 were influenced by gas-pressurization of the lava dome.  相似文献   
199.
火山熔岩油气藏是准噶尔盆地油气勘探和开发的重要目标之一。通过对准噶尔盆地西泉地区16口石炭系火山熔岩井的岩心观察、普通薄片和铸体薄片镜下鉴定和定量统计、扫描电镜和X-射线衍射等实验,研究玄武岩、安山岩、英安岩的岩石学特征、孔隙类型及储集特征及异同点,建立火山熔岩成岩演化序列,探讨成岩作用对火山熔岩孔隙演化的影响。研究表明,安山岩的储集空间最发育,孔隙类型及组合多样,多为气孔+斑晶溶孔+基质溶孔+溶蚀缝组合和气孔+斑晶溶孔+基质溶孔+溶蚀缝+构造裂缝组合。英安岩的孔隙组合为气孔+斑晶溶孔+基质溶孔和气孔+斑晶溶孔+基质溶孔+溶蚀缝。玄武岩孔隙类型及组合单一,为构造裂缝+溶蚀缝,构造裂缝+基质溶孔,气孔+溶蚀缝。挥发分逸出作用控制火山熔岩原生气孔的发育,岩浆期后热液作用和充填作用破坏了火山熔岩的储集空间,溶蚀作用、风化淋滤作用和构造破裂作用极大地改善了火山熔岩的储集性能。认为西泉地区石炭系顶部风化剥蚀淋滤带(距石炭系顶面0~20 m)的安山岩是油气聚集的最有利层段。  相似文献   
200.
During the past 500 thousand years, Unzen volcano, an active composite volcano in the Southwest Japan Arc, has erupted lavas and pyroclastic materials of andesite to dacite composition and has developed a volcanotectonic graben. The volcano can be divided into the Older and the Younger Unzen volcanoes. The exposed rocks of the Older Unzen volcano are composed of thick lava flows and pyroclastic deposits dated around 200–300 ka. Drill cores recovered from the basal part of the Older Unzen volcano are dated at 400–500 ka. The volcanic rocks of the Older Unzen exceed 120 km3 in volume. The Younger Unzen volcano is composed of lava domes and pyroclastic deposits, mostly younger than 100 ka. This younger volcanic edifice comprises Nodake, Myokendake, Fugendake, and Mayuyama volcanoes. Nodake, Myokendake and Fugendake volcanoes are 100–70 ka, 30–20 ka, and <20 ka, respectively. Mayuyama volcano formed huge lava domes on the eastern flank of the Unzen composite volcano about 4000 years ago. Total eruptive volume of the Younger Unzen volcano is about 8 km3, and the eruptive production rate is one order of magnitude smaller than that of the Older Unzen volcano.  相似文献   
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