Volcanoes: from inception to eruption
Transcript of Volcanoes: from inception to eruption
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Volcanoes: from inception to eruptionDr Tom D. Pering
Department of Geography
University of Sheffield
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The Plan
Part A: Heat and Plate Tectonics.
Part B: Volcano Fundamentals.
Part C: Volcanic Hazards.
• First – what is a volcano?
• “Surficial manifestation of a planet or moon’s internal thermal processes through emission of solid, liquid or gaseous products at discrete surface locations”
• Definition not geomorphological, volcanoes have a variety of shapes.
• Interweaved you will see snippets of a mini documentary (not yet released) on volcanoes and volcanic fieldwork.
• Aim: to cover common GCSE/A Level content, but also provide you with a little bit extra.
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Part A: Heat and Plate Tectonics
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A: Heat and Plate Tectonics
1. Heat Generation • Volcanism is powered through heat.• Heat is generated within a planetary body in two main ways:
Radiation Tidal Forces
Decay of radioactive isotopes ininterior liberates heat, like a nuclearpower station or bomb!
Astronomical objects don’t just movewater on Earth, but also deform theinterior, liberating heat, like kneadingdough.
NASA/JPL Image.
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A: Heat and Plate Tectonics
2. Heat Loss • Convection through plate tectonics and
mantle plumes generates volcanism.
Conduction
Heat travels from the interior andthen through the crust.
Convection – Plate Tectonics
Material cycles from the interior tothe surface through plate tectonics –this where most is heat is lost.
Convection – Mantle Plumes
Mantle plumes rise from the core-mantle boundary thus dissipating heat– like a lava lamp.
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A: Heat and Plate Tectonics
3: Plate Tectonics & Margins• Animation of earthquakes, eruptions, and SO2 emissions -
http://volcano.si.axismaps.io/
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A: Heat and Plate Tectonics
3: Plate Tectonics & Margins
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A: Heat and Plate Tectonics
3: Plate Tectonics & Margins
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A: Heat and Plate Tectonics
3: Plate Tectonics & Margins
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A: Heat and Plate Tectonics
3: Plate Tectonics & Margins
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Part B: Volcano Fundamentals
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1. Classic Geomorphology
B: Volcano Fundamentals
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1. Classic Geomorphology
Mount Fuji, a stratovolcano in Japan.
• Stratovolcanoes: layers of viscous lava flows and pyroclastic rocks.
B: Volcano Fundamentals
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1. Classic Geomorphology
• Shield volcanoes: layers of fluid lava flows, convex profile and can be enormous.
Above: Fernandina volcano, a shield volcano of the Galapagos
Islands (Chuck Wood, 1979).
B: Volcano Fundamentals
Left: Kilauea summit area in 2020.
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B: Volcano Fundamentals
• 1: Low viscosity magmas such as Basalt, give rise to basaltic volcanism.• Most commonly produced at mid-ocean ridges and at hot spots.• These magmas create shield volcanoes!
2. Magma Type Overview
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B: Volcano Fundamentals
• 2. High viscosity magmas such as Andesite and Rhyolite give rise to silicic volcanism.
• Most commonly produced at subduction zone settings.• These magmas create stratovolcanoes!
2. Magma Type Overview
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B: Volcano Fundamentals
• Eruptive style is determined primarily by magma type, specifically its viscosity, which is determined by the amount of SiO2 (silica) present.
• SiO2 polymerises into SiO4 (silcate tetrahedra lattices), which impede flow of magma, making it more viscous.
2. Magma Type Overview
More Silica = Higher Viscosity
• Low silica (~ 50%) = Basalt• Medium silica (~ 50-65%) = Andesite• High silica (> 65%) = Rhyolite
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• A magma is a complex mixture of:• Melt (molten rock), Crystals (solid), Gas
B: Volcano Fundamentals
3. What is a magma?
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B: Volcano Fundamentals
4. Gases – Bob the Bubble
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B: Volcano Fundamentals
4. Gases
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B: Volcano Fundamentals
5. Basaltic (low viscosity) Volcanism
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B: Volcano Fundamentals
5. Basaltic (low viscosity) Volcanism
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B: Volcano Fundamentals
• Basaltic magmas have low viscosities.• The low magma viscosity allows the formation of larger bubbles during bubble
ascent. This leads to the formation of a number of different flow regimes which generated a number of different basaltic activity styles:
5. Basaltic (low viscosity) Volcanism
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B: Volcano Fundamentals
6. Silicic (high viscosity) Volcanism
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B: Volcano Fundamentals
• Higher viscosity magmas tend to restrict gas flow, leads to pressurisation, and the largest volcanic explosions!
• The lava dome case:
6. Silicic (high viscosity) Volcanism
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Interlude: MAGATH
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Interlude: MAGATH
• The key factors which act to control style of volcanic activity, how the activity may behave in the atmosphere, and how it is generated.
• Material (Molten Rock or Ice)
• Available Volatiles (Gases)
• Gravity
• Atmospheric Pressure
• Tectonic Environment
• Heat Generation Mechanism
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Part C: Volcanic Hazards
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C: Volcanic Hazards
• Local hazards:
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C: Volcanic Hazards
• Overview:• Eruption column – aviation & climate.
• Tephra fall – localised.
• Collapse of lava dome or eruption column to form pyroclastic density current.
• Collapse of volcano in debris avalanche.
• Mobilisation of ash to form lahars.
• Volcanoes can cause tsunami.
• Volcanic gases.
• Sub-glacial volcanoes can cause massive floods (Jökulhlaups).
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C: Volcanic Hazards
Left, gas unable to escape from a viscous magma. Right, a pyroclastic density current (PDC).
• Silicic volcanism - Pyroclastic Density Currents:• Gas can’t move freely within a magma and can find it difficult to escape (i.e., due
to high viscosity).• When gas can’t escape, pressure builds up, leading to large pyroclastic explosions
(i.e., vulcanian, sub-plinian, plinian).• Eruptions can lead to pyroclastic density currents (PDCs), where instability in
eruption columns causes column collapse.
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C: Volcanic Hazards
• Silicic volcanism - Pyroclastic Density Currents:
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C: Volcanic Hazards
• Silicic volcanism - Lahars:
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C: Volcanic Hazards
• Precursors - notes on uncertainty…• Forecasting versus prediction.
Encyclopedia of Volcanoes, Chapter 67.
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C: Volcanic Hazards
• Responding to risk:
What hazards? What intensity?What ‘assets’?
How vulnerable are they?
Resilience. Ability to Respond.
𝑅𝑖𝑠𝑘 =𝐻𝑎𝑧𝑎𝑟𝑑 × 𝐸𝑥𝑝𝑜𝑠𝑢𝑟𝑒 × 𝑉𝑢𝑙𝑛𝑒𝑟𝑎𝑏𝑖𝑙𝑖𝑡𝑦
𝐶𝑎𝑝𝑎𝑐𝑖𝑡𝑦
Where spatially?
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C: Volcanic Hazards
• We can reduce risk, through monitoring:
Gas ReleaseY
Seismicity
Deformation
Thermal
+
+
+
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C: Volcanic Hazards
• We can build sophisticated models:
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Pressurisation
StabilityMagma at surface
Magma movingat depth
Ground deformation
DOME COLLAPSERainfall
on dome
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C: Volcanic Hazards
A summary of recent important eruptions:
Taken from: Sigurdsson, H., 2000. History of Volcanology. In: Encyclopaedia of Volcanoes. P15-40
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Thanks & Summary
Part A: Heat and Plate TectonicsPart B: Volcano FundamentalsInterlude: MAGATHPart C: Volcanic Hazards