Genetic Processes of Cave Minerals in Volcanic Environments: an Overview
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Geologic Map of the Long Valley Caldera, Mono-Inyo Craters
DEPARTMENT OF THE INTERIOR TO ACCOMPANY MAP 1-1933 US. GEOLOGICAL SURVEY GEOLOGIC MAP OF LONG VALLEY CALDERA, MONO-INYO CRATERS VOLCANIC CHAIN, AND VICINITY, EASTERN CALIFORNIA By Roy A. Bailey GEOLOGIC SETTING VOLCANISM Long Valley caldera and the Mono-Inyo Craters Long Valley caldera volcanic chain compose a late Tertiary to Quaternary Volcanism in the Long Valley area (Bailey and others, volcanic complex on the west edge of the Basin and 1976; Bailey, 1982b) began about 3.6 Ma with Range Province at the base of the Sierra Nevada frontal widespread eruption of trachybasaltic-trachyandesitic fault escarpment. The caldera, an east-west-elongate, lavas on a moderately well dissected upland surface oval depression 17 by 32 km, is located just northwest (Huber, 1981).Erosional remnants of these mafic lavas of the northern end of the Owens Valley rift and forms are scattered over a 4,000-km2 area extending from the a reentrant or offset in the Sierran escarpment, Adobe Hills (5-10 km notheast of the map area), commonly referred to as the "Mammoth embayment.'? around the periphery of Long Valley caldera, and The Mono-Inyo Craters volcanic chain forms a north- southwestward into the High Sierra. Although these trending zone of volcanic vents extending 45 km from lavas never formed a continuous cover over this region, the west moat of the caldera to Mono Lake. The their wide distribution suggests an extensive mantle prevolcanic basement in the area is mainly Mesozoic source for these initial mafic eruptions. Between 3.0 granitic rock of the Sierra Nevada batholith and and 2.5 Ma quartz-latite domes and flows erupted near Paleozoic metasedimentary and Mesozoic metavolcanic the north and northwest rims of the present caldera, at rocks of the Mount Morrisen, Gull Lake, and Ritter and near Bald Mountain and on San Joaquin Ridge Range roof pendants (map A). -
Satellite Observations of Fumarole Activity at Aluto Volcano, Ethiopia: Implications for Geothermal Monitoring and Volcanic Hazard
Accepted Manuscript Satellite observations of fumarole activity at Aluto volcano, Ethiopia: Implications for geothermal monitoring and volcanic hazard Mathilde Braddock, Juliet Biggs, Iain M. Watson, William Hutchison, David M. Pyle, Tamsin A. Mather PII: S0377-0273(17)30118-X DOI: doi: 10.1016/j.jvolgeores.2017.05.006 Reference: VOLGEO 6091 To appear in: Journal of Volcanology and Geothermal Research Received date: 24 February 2017 Revised date: 6 May 2017 Accepted date: 7 May 2017 Please cite this article as: Mathilde Braddock, Juliet Biggs, Iain M. Watson, William Hutchison, David M. Pyle, Tamsin A. Mather , Satellite observations of fumarole activity at Aluto volcano, Ethiopia: Implications for geothermal monitoring and volcanic hazard, Journal of Volcanology and Geothermal Research (2017), doi: 10.1016/ j.jvolgeores.2017.05.006 This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain. ACCEPTED MANUSCRIPT Satellite observations of fumarole activity at Aluto volcano, Ethiopia: implications for geothermal monitoring and volcanic hazard Mathilde Braddock1*, Juliet Biggs2, Iain M. Watson2, William Hutchison3, David M. Pyle4 and Tamsin A. Mather4 1 School of Earth Sciences, University of Bristol, Wills Memorial Building, Queens Road, Bristol BS8 1RJ, UK 2 COMET, School of Earth Sciences, University of Bristol, Wills Memorial Building, Queens Road, Bristol BS8 1RJ, UK 3 School of Earth and Environmental Sciences, University of St. -
Geothermal Springs, Geysers and Fumaroles
Sciences Secondary volcanic activities: Geothermal springs, Geysers and Fumaroles Geothermal Springs A geothermal (or hydrothermal) spring is produced by the emergence of geothermally heated groundwater from the Earth's crust. There are geothermal springs in many locations all over the crust of the earth. Geothermal Springs Surface water percolates downward through the rocks below the Earth's surface to high-temperature regions surrounding a magma chamber, either active or recently solidified but still hot. When the water is heated, becomes less dense, and rises Surface water back to the surface along fissures and cracks. Sometimes these features are called "dying volcanoes" because they seem to represent the last stage of volcanic activity as the magma, in depth, cools and hardens. Water percolation Heated water rises up The temperature of hot springs depends on factors such as: •the rate at which water circulates through the underground channels Hot rocks •the amount of heat at depth •the dilution of the heated water by cool ground water near the surface. Geothermal Springs The water issuing from a hot spring is heated by geothermal heat from the Earth's astenosphere. In general, the temperature of rocks increases with depth. The rate of temperature increase is known as the geothermal gradient (it is about 25°C per km). If water percolates deeply enough into the crust, it will be heated as it comes into contact with hot rocks. Warm springs are sometimes the result of hot and cold springs mixing but may also occur outside of volcanic areas. Geysers Geyser are located near active volcanic areas, and the geyser effect is due to the proximity of magma. -
Insights from Fumarole Gas Geochemistry on the Recent Volcanic Unrest of Pico Do Fogo, Cape Verde
ORIGINAL RESEARCH published: 15 July 2021 doi: 10.3389/feart.2021.631190 Insights from Fumarole Gas Geochemistry on the Recent Volcanic Unrest of Pico do Fogo, Cape Verde Gladys V. Melián 1,2,3*, Pedro A. Hernández 1,2,3, Nemesio M. Pérez 1,2,3, María Asensio-Ramos 1, Eleazar Padrón 1,2,3, Mar Alonso 1,2, Germán D. Padilla 1,2, José Barrancos 1,2, Francesco Sortino 4, Hirochicka Sumino 5, Fátima Rodríguez 1, Cecilia Amonte 1, Sonia Silva 6, Nadir Cardoso 6 and José M. Pereira 7 1Instituto Volcanológico de Canarias (INVOLCAN), La Laguna, Spain, 2Instituto Tecnológico y de Energías Renovables (ITER), Granadilla de Abona, Spain, 3Agencia Insular de la Energía de Tenerife (AIET), Granadilla de Abona, Spain, 4Istituto Nazionale di Geofisica e Vulcanologia - Sezione Roma 2, Roma, Italy, 5Department of General Systems Studies, Graduate School of Arts and Sciences, The University of Tokyo, Komaba, Meguro-ku, Japan, 6Universidade de Cabo Verde (UNICV), Praia, Cape Verde, 7Laboratório de Engenharia Civil of Cape Verde (LEC) Tira - Chapéu, Praia, Cape Verde Edited by: We report the results of the geochemical monitoring of the fumarolic discharges at the Pico Francesco Italiano, do Fogo volcano in Cape Verde from 2007 to 2016. During this period Pico do Fogo National Institute of Geophysics and Volcanology, Italy experienced a volcanic eruption (November 23, 2014) that lasted 77 days, from a new vent Reviewed by: ∼2.5 km from the fumaroles. Two fumaroles were sampled, a low (F1∼100°C) and a Pierpaolo Zuddas, medium (F2∼300°C) temperature. The variations observed in the δ18O and δ2H in F1 and Sorbonne Universités, France F2 suggest different fluid source contributions and/or fractionation processes. -
Deep Electrical Resistivity Tomography for a 3D Picture of the Most Active Sector of Campi Flegrei Caldera A
www.nature.com/scientificreports Corrected: Publisher Correction OPEN Deep Electrical Resistivity Tomography for a 3D picture of the most active sector of Campi Flegrei caldera A. Troiano 1*, R. Isaia1, M. G. Di Giuseppe1, F. D. A. Tramparulo1 & S. Vitale1,2 The central sector of the Campi Flegrei volcano, including the Solfatara maar and Pisciarelli fumarole feld, is currently the most active area of the caldera as regards seismicity and gaseous emissions and it plays a signifcant role in the ongoing unrest. However, a general volcano-tectonic reconstruction of the entire sector is still missing. This work aims to depict, for the frst time, the architecture of the area through the application of deep Electrical Resistivity Tomography. We reconstructed a three- dimensional resistivity model for the entire sector. Results provide useful elements to understand the present state of the system and the possible evolution of the volcanic activity and shed solid bases for any attempt to develop physical-mathematical models investigating the ongoing phenomena. Te present research shows the results of an original application of the deep electrical resistivity tomography (ERT) aimed to investigate the central sector of the Campi Flegrei (CF) caldera (Italy). Te CF caldera (Fig. 1) is one of the most dangerous volcanoes in Europe1,2. Te most active zone, as for seis- micity and gas emission, is currently located in the central sector of the caldera including the volcanic structure of Solfatara, Pisciarelli and Agnano Plain3–5. Intense and recurrent volcanism, culminated in two main caldera forming events, namely the eruption of the Campanian Ignimbrite (39.8 ka)6 and that of the Neapolitan Yellow Tuf (15 ka)7, marks the CF eruptive history. -
Processes Culminating in the 2015 Phreatic Explosion at Lascar Volcano, Chile, Evidenced by Multiparametric Data
Nat. Hazards Earth Syst. Sci., 20, 377–397, 2020 https://doi.org/10.5194/nhess-20-377-2020 © Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License. Processes culminating in the 2015 phreatic explosion at Lascar volcano, Chile, evidenced by multiparametric data Ayleen Gaete1, Thomas R. Walter1, Stefan Bredemeyer1,2, Martin Zimmer1, Christian Kujawa1, Luis Franco Marin3, Juan San Martin4, and Claudia Bucarey Parra3 1GFZ German Research Centre for Geosciences, Telegrafenberg, 14473 Potsdam, Germany 2GEOMAR Helmholtz Centre for Ocean Research Kiel, 24148 Kiel, Germany 3Observatorio Volcanológico de Los Andes del Sur (OVDAS), Servicio Nacional de Geología y Minería (SERNAGEOMIN), Temuco, Chile 4Physics Science Department, Universidad de la Frontera, Casilla 54-D, Temuco, Chile Correspondence: Ayleen Gaete ([email protected]) Received: 13 June 2019 – Discussion started: 25 June 2019 Accepted: 5 December 2019 – Published: 4 February 2020 Abstract. Small steam-driven volcanic explosions are com- marole on the southern rim of the Lascar crater revealed a mon at volcanoes worldwide but are rarely documented or pronounced change in the trend of the relationship between monitored; therefore, these events still put residents and the CO2 mixing ratio and the gas outlet temperature; we tourists at risk every year. Steam-driven explosions also oc- speculate that this change was associated with the prior pre- cur frequently (once every 2–5 years on average) at Lascar cipitation event. An increased thermal anomaly inside the ac- volcano, Chile, where they are often spontaneous and lack tive crater as observed in Sentinel-2 images and drone over- any identifiable precursor activity. -
Lofthellir Lava Tube Ice Cave, Iceland
50th Lunar and Planetary Science Conference 2019 (LPI Contrib. No. 2132) 3118.pdf LOFTHELLIR LAVA TUBE ICE CAVE, ICELAND: SUBSURFACE MICRO-GLACIERS, ROCKFALLS, DRONE LIDAR 3D-MAPPING, AND IMPLICATIONS FOR THE EXPLORATION OF POTENTIAL ICE- RICH LAVA TUBES ON THE MOON AND MARS. Pascal Lee1,2,3, Eirik Kommedal1,2, Andrew Horchler,4, Eric Amoroso4, Kerry Snyder4, and Anton F. Birgisson5. 1SETI Institute, 2Mars Institute, 3NASA Ames Research Center, e-mail: [email protected], 4Astrobotic, 5Geo Travel Iceland. Summary: The Lofthellir lava tube, Iceland, con- tains massive ice formations accumulated from mete- oric H2O. We report here on micro-glaciers and rock- falls, as well as the first 3D-mapping of a lava tube and ice-rich cave by drone-borne lidar. Implications for the exploration of potential ice-rich lava tubes on the Moon and Mars are examined. Figure 1. Location of Lofthellir Lava Tube, Iceland. Introduction: Caves and pits have been identified on the Moon and Mars, many of which are likely lava tubes and their associated skylights, respectively. Can- didate impact-melt lava tubes and skylights recently reported at high latitude on the Moon [1], and volcanic lava tubes and skylights identified at high altitude on Mars’ giant volcanoes [2], might offer access not only to unique sheltered subsurface environments, but also to potential repositories of subsurface volatiles, in par- ticular H2O ice. Given this prospect on the Moon and Mars, under- standing the occurrence (origin, distribution, evolution through time) of ice inside lava tubes on Earth is im- portant. While analogies between the Moon or Mars and the Earth regarding ice in lava tubes are not ex- pected to be straightforward, some processes and fea- tures associated with ice in such subsurface environ- ments might nevertheless be shared, e.g., the potential role of gravity in cave-ice dynamics (independent of the origin of the ice), or the role of freeze-thaw cycling on cave stability. -
Lava Tube Formation
Lava Tube Formation Lava Flows and their Caves The Shaft, 3H-8, Lava Flows and Caves is an open >Long lava flows are invariably fed by tubes volcanic vent which insulate the lava travelling within them. Scoria Welded >The leading edge of a flow is an advancing Cone Spatter wall of pahoehoe lobes or aa rubble. >Behind the edge, flow is concentrated into surface channels, or hidden tubes beneath the crust. Stagnant areas solidify. Volcanic 10 m Chamber >When the lava drains out an open cave is left. Lava Flows ? ? ? Liquid lava spreads out from a vent but quickly crusts over. The crust can be smooth and Overview of lava cave formation wrinkly (Pahoehoe or Ropy lava) or if the lava is Observations of active lava flows has shown stiffer it may break into jagged fragments (Aa that there are two distinct ways in which lava lava). tubes or caves form: Liquid lava continues to flow beneath the Roofing of surface lava channels. This can crusted surface, inflating it and pushing out in happen in three ways (e.g. Peterson et al, front as lobes of pahoehoe or walls of rubbley 1994), see panel 2. aa. Sub-crustal drainage within thin lava lobes or Behind the advancing front the liquid flow sheets. (e.g. Hon et al, 1994), see panel 3 . becomes concentrated into linear streams: either surface channels or in tubes and Open Volcanic Vents are a rare type of cave chambers beneath the crust. The surface formed by the draining of the lava back into the channels may later crust over to form tubes. -
Processes Culminating in the 2015 Phreatic Explosion at Lascar Volcano, Chile, Monitored by Multiparametric Data Ayleen Gaete1, Thomas R
https://doi.org/10.5194/nhess-2019-189 Preprint. Discussion started: 25 June 2019 c Author(s) 2019. CC BY 4.0 License. Processes culminating in the 2015 phreatic explosion at Lascar volcano, Chile, monitored by multiparametric data Ayleen Gaete1, Thomas R. Walter1, Stefan Bredemeyer1,2, Martin Zimmer1, Christian Kujawa1, Luis Franco3, Juan San Martin4, Claudia Bucarey Parra3 5 1 GFZ German Research Centre for Geosciences, Telegrafenberg, 14473 Potsdam, Germany 2 GEOMAR Helmholtz Centre for Ocean Research Kiel, 24148 Kiel, Germany 3 Observatorio Volcanológico de Los Andes del Sur (OVDAS), Servicio Nacional de Geología y Minería (SERNAGEOMIN), Temuco, Chile. 4 Physics Science Department, Universidad de la Frontera, Casilla 54-D, Temuco, Chile. 10 Correspondence to: Ayleen Gaete ([email protected]) Abstract. Small steam-driven volcanic explosions are common at volcanoes worldwide but are rarely documented or monitored; therefore, these events still put residents and tourists at risk every year. Steam-driven explosions also occur frequently (once every 2-5 years on average) at Lascar volcano, Chile, where they are often spontaneous and lack any identifiable precursor activity. Here, for the first time at Lascar, we describe the processes culminating in such a sudden 15 volcanic explosion that occurred on October 30, 2015, which was thoroughly monitored by cameras, a seismic network, and gas (SO2 and CO2) and temperature sensors. Prior to the eruption, we retrospectively identified unrest manifesting as a gradual increase in the number of long-period (LP) seismic events in 2014, indicating an augmented level of activity at the volcano. Additionally, SO2 flux and thermal anomalies were detected before the eruption. -
The Origin and Emplacement of Domo Tinto, Guallatiri Volcano, Northern Chile Andean Geology, Vol
Andean Geology ISSN: 0718-7092 [email protected] Servicio Nacional de Geología y Minería Chile Watts, Robert B.; Clavero Ribes, Jorge; J. Sparks, R. Stephen The origin and emplacement of Domo Tinto, Guallatiri volcano, Northern Chile Andean Geology, vol. 41, núm. 3, septiembre, 2014, pp. 558-588 Servicio Nacional de Geología y Minería Santiago, Chile Available in: http://www.redalyc.org/articulo.oa?id=173932124004 How to cite Complete issue Scientific Information System More information about this article Network of Scientific Journals from Latin America, the Caribbean, Spain and Portugal Journal's homepage in redalyc.org Non-profit academic project, developed under the open access initiative Andean Geology 41 (3): 558-588. September, 2014 Andean Geology doi: 10.5027/andgeoV41n3-a0410.5027/andgeoV40n2-a?? formerly Revista Geológica de Chile www.andeangeology.cl The origin and emplacement of Domo Tinto, Guallatiri volcano, Northern Chile Robert B. Watts1, Jorge Clavero Ribes2, R. Stephen J. Sparks3 1 Office of Disaster Management, Jimmit, Roseau, Commonwealth of Dominica. [email protected] 2 Escuela de Geología, Universidad Mayor, Manuel Montt 367, Providencia, Santiago, Chile. [email protected] 3 Department of Earth Sciences, University of Bristol, Wills Memorial Building, Queens Road, Bristol. BS8 1RJ. United Kingdom. [email protected] ABSTRACT. Guallatiri Volcano (18°25’S, 69°05’W) is a large edifice located on the Chilean Altiplano near the Bo- livia/Chile border. This Pleistocene-Holocene construct, situated at the southern end of the Nevados de Quimsachata chain, is an andesitic/dacitic complex formed of early stage lava flows and later stage coulées and lava domes. -
Caves in New Mexico and the Southwest Issue 34
Lite fall 2013 Caves in New Mexico and the Southwest issue 34 The Doll’s Theater—Big Room route, Carlsbad Cavern. Photo by Peter Jones, courtesy of Carlsbad Caverns National Park. In This Issue... Caves in New Mexico and the Southwest Cave Dwellers • Mapping Caves Earth Briefs: Suddenly Sinkholes • Crossword Puzzle New Mexico’s Most Wanted Minerals—Hydromagnesite New Mexico’s Enchanting Geology Classroom Activity: Sinkhole in a Cup Through the Hand Lens • Short Items of Interest NEW MEXICO BUREAU OF GEOLOGY & MINERAL RESOURCES A DIVISION OF NEW MEXICO TECH http://geoinfo.nmt.edu/publications/periodicals/litegeology/current.html CAVES IN NEW MEXICO AND THE SOUTHWEST Lewis Land Cave Development flowing downward from the surface. Epigenic A cave is a naturally-formed underground cavity, usually caves can be very long. with a connection to the surface that humans can enter. The longest cave in the Caves, like sinkholes, are karst features. Karst is a type of world is the Mammoth landform that results when circulating groundwater causes Cave system in western voids to form due to dissolution of soluble bedrock. Karst Kentucky, with a surveyed terrain is characterized by sinkholes, caves, disappearing length of more than 400 streams, large springs, and underground drainage. miles (643 km). The largest and most common caves form by dissolution of In recent years, limestone or dolomite, and are referred to as solution caves. scientists have begun to Limestone and dolomite rock are composed of the minerals recognize that many caves calcite (CaCO ) and dolomite (CaMg(CO ) ), which are 3 3 2 are hypogenic in origin, soluble in weak acids such as carbonic acid (H CO ), and are 2 3 meaning that they were thus vulnerable to dissolution by groundwater. -
Raw Sewage and Solid Waste Dumps in Lava Tube Caves of Hawaii Island
William R. Halliday - Raw sewarge and sold waste dumps in lave tube caves of Hawaii Island. Journal of Cave and Karst Studies, v. 65, n. 1, p. 68-75. RAW SEWAGE AND SOLID WASTE DUMPS IN LAVA TUBE CAVES OF HAWAII ISLAND WILLIAM R. HALLIDAY Hawaii Speleological Survey, 6530 Cornwall Court, Nashville, TN 37205 USA [email protected] Lava tubes on the island of Hawaii (and elsewhere) are possible subsurface point sources of contamina- tion in addition to more readily identifiable sources on the surface. Human and animal waste, and haz- ardous and toxic substances dumped into lava tube caves are subject to rapid transport during flood events, which are the dominant type of groundwater flow through Hawaiian lava tubes. Although these waste materials may not be a major source of pollution when compared with some surface sources, this potential hazard should be evaluated much as in the case of karstic floodwater conduits. This paper explores the interaction of water flow and solid waste dumps and sewage in lava tubes and lava tube caves of Hawaii Island, Hawaii - an island almost as large as the state of Connecticut (Fig. 1)-and resulting potential threats to groundwater quality. In recent years, Hawaiian cavers and speleologists have become increasingly concerned about these occurrences. Some of the solid waste dumps can be seen to contain partially empty containers of toxic and/or hazardous substances (Fig. 2), including automotive and agricultural waste. Stinking raw sewage speaks for itself (Fig. 3), and members of the Hawaii chapter of the National Speleological Society have been shown the top of a septic tank or cesspool near Keaau said to consist of an unlined segment of lava tube cave.