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Impact of eruptio V o l c a n o e s Prediction Part II Supervolcanoe

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V. o. s. l. c. e. a. o. n. Part II. Prediction. Impact of eruptions. Supervolcanoes. Prediction of Volcanic Eruptions. Long Term Prediction. Identify volcanoes and the frequency and style of their eruptions (a geological problem). - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Impact of eruptions

Impact of eruptions

Vo l c a noes

Prediction

Part II

Supervolcanoes

Page 2: Impact of eruptions

Prediction of Volcanic Eruptions

Identify volcanoes and the frequency and style of their eruptions (a geological problem).

Long Term Prediction

Establish the level of risk based on historic and geologic record.

Establish probabilities of eruption, style and location for individual volcanoes.

E.g., for individual volcanoes: determine most likely routes for lahars, nuees ardentes, lava flows, etc., and avoid construction in those areas.

Page 3: Impact of eruptions

Hazard zones have been distinguished around Mt. Shasta based on topography and past experience with eruptions.

Zone 1: areas likely to be affected most frequently. Most future flows from summit eruptions probably would stay within this zone.

Zone 1

Page 4: Impact of eruptions

Hazard zones have been distinguished around Mt. Shasta based on topography and past experience with eruptions.

Zone 1: areas likely to be affected most frequently. Most future flows from summit eruptions probably would stay within this zone.

Zone 2: areas likely to be affected by lava flows erupted from vents on the flank of the volcano or that move into zone 2 from zone 1.

Zone 2

Page 5: Impact of eruptions

Hazard zones have been distinguished around Mt. Shasta based on topography and past experience with eruptions.

Zone 2: areas likely to be affected by lava flows erupted from vents on the flank of the volcano or that move into zone 2 from zone 1.

Zone 1: areas likely to be affected most frequently. Most future flows from summit eruptions probably would stay within this zone.

Zone 3: areas likely to be affected infrequently and then only by long lava flows that originate at vents in zones 1 and 2

Zone 3

Page 6: Impact of eruptions

Short-term prediction

Based on the recognition of a pattern of events prior to previous eruptions.

Gas emissions: rates of emission and type of gas changes in some volcanoes.

Important gases include sulfur dioxide (SO2) and carbon dioxide (CO2)

Changes in concentration may reflect movement of the magma up the vent.

Page 7: Impact of eruptions

Surface tilting: recognition of changes in the land surface due to building pressure in the conduit.

A surface bulge appeared on Mt. St. Helens prior to its eruption.

April 26 May 2

April 8, 1980

Page 8: Impact of eruptions

Earthquakes: generated as the magma moves up the feeder conduit to the vent.

When viscous magma becomes stuck in the conduit strain energy builds as more magma tries to push out.

Movement takes place in a series of “jerks” as the rock material breaks. Each “jerk” produces an earthquake.

Magnitudes generally less than 5 M.

The more earthquakes the further the magma has moved.

Page 9: Impact of eruptions

Mount Spurr, Alaska:The 1992 Eruption of Crater Peak Vent

USGS

Black bars: earthquake frequency.

Red lines: volcanic eruptions.

Page 10: Impact of eruptions

A combination of approaches is likely the key to short-term prediction.

Page 11: Impact of eruptions

The impact of volcanic eruptions

Page 12: Impact of eruptions

Volcanic Hazards

Damage limited to the vicinity in the immediate area of the volcano.

Lava flows 

Commonly destroy property in Hawaii and Iceland.

Fatalities rare due to slow speed of advancing lava flow.

Page 13: Impact of eruptions

Ash fall

Extensive property damage and fatalities can result from heavy ash falls.

Significant ash in the upper atmosphere can circle the globe in a matter of weeks.

Mt. St. Helens’ ash cloud

More than 80 commercial jets have been damaged by flying through volcanic ash clouds.

Page 14: Impact of eruptions

An ashfall 10 million years ago killed these rhinos that are preserved at Ashfall Fossil Beds State Historic Park, Nebraska.

Death was not by burial but by lung failure due to inhaling the ash.

Page 15: Impact of eruptions

Pyroclastic flows

Lahars can also dam rivers and which can lead to extensive flooding.

Lahars are fast moving mudflows that can inundate urban areas that are nearby the eruption.

Page 16: Impact of eruptions

Lahars can be the most devastating outcome of many volcanoes.

Water and debris rushed down the slopes, picking up more debris along the way.

A relatively small eruption of Nevada del Ruiz, Columbia, in 1985, generated a lahar when the volcano melted a 2.5 km2 area of snow and ice.

Page 17: Impact of eruptions

A 5 metre wall of water and debris slammed into the town of Amero, 72 km from the volcano.

The lahar killed 28,700 people and destroyed over 5,000 structures in the city.

Page 18: Impact of eruptions

Nuée ardentes destroy life and property in their paths.

60 people, thousands of animals and fish, and hundreds of acres of lumber were destroyed by ash flows from Mt. St. Helens.

A Nuée Ardent killed 20,000 people when Mt. Vesuvius exploded and shed a pyroclastic flow across the village of Pompeii in 79 AD.

Page 19: Impact of eruptions

People and animals died instantly from the rushing cloud of hot gas and ash.

Page 20: Impact of eruptions

Landslides

Landslides can be generated when a volcano collapses during an eruption.

During the Mt. St. Helens eruption 2.3 km3 of debris slid down the mountain at speeds up to 240 km/hr.

The slide traveled over 24 km and left a 45 m deep deposit.

350,000 years ago Mt. Shasta experienced a similar eruption and landslide that was 20 times greater than that of Mt. St. Helens.

Page 21: Impact of eruptions

Volcanic Gases

In addition to making magma more explosive, volcanic eruptions also include gases that can be deadly to all life.

CO2, SO2 and CO are the most abundant of harmful gases.

Page 22: Impact of eruptions

Volcanoes release more than 130 to 230 million tonnes of CO2 into the atmosphere every year

Humans add CO2 at the rate of approximately 22 billion tonnes per year (150 times the rate of volcanic production)

Human CO2 production is equal to that if 17,000 volcanoes like Kilauea were erupting every year.

SO2 emissions can have direct effects on life in the vicinity of a volcano.

An eruption in 1783 of Laki Crater (Iceland) produced a sulfurous haze that lasted for 9 months and killed 75% of all livestock and 24% of the Icelandic population.

Page 23: Impact of eruptions

Mammoth Mountain is a relatively young volcano that is emitting large volumes of CO2.

Gas concentrations in the soil in some areas near the mountain are high enough to kill trees and small animals.

Page 24: Impact of eruptions

If the air that we breath has more than 10% CO2 it becomes deadly because it displaces the Oxygen that we need for respiration.

Lake Nios, Cameroon, is a very deep lake within a volcanic crater.

The lake is so deep that hydrostatic pressure forces CO2 to remain at the lake bottom.

When the pressure of the CO2 exceeds a certain limit the gas rapidly bubbles up out of the lake and flows as an invisible gas cloud down the adjacent slopes.

On August 61, 1986 such a gas release flowed 19 km suffocating 1,700 people along its route.

Page 25: Impact of eruptions

The fountain in the background lifts CO2 up to the surface so that it no longer accumulates.

Lake Nyos 10 days after the 1986 eruption

Page 26: Impact of eruptions

Tsunamis

Caused by the displacement of seawater by eruptions of volcanic islands and submarine volcanoes.

Krakatoa (1883 eruption) killed 36,000 people by the tsunami, alone (the most deadly outcome of the eruption).

This is the newly forming summit of Krakatoa, growing where the 1883 eruption blew the top off of the original volcano.

Page 27: Impact of eruptions

Global Climate Change

Due to ash and gas that may spend years in the upper atmosphere; reduces incoming solar radiation.

SO2 from an eruption forms tiny droplets of sulfuric acid

in the upper atmosphere.

The droplets significantly increase global albedo…..a negative radiative forcing that leads to cooling.

Mt. Pinatubo (1991) released 22 million metric tons of SO2 and reduced the Earth’s average temperature by 0.5 degrees Celsius in the year following the eruption.

Page 28: Impact of eruptions

Tambora (1815 eruption) was followed in 1816 by the “year without a summer”.

Average global temperature is estimated to have been reduced by 3 degrees Celsius.

A series of eruptions of Tambora (Indonesia) extruded up to 150 km3 of magma (solid equivalent), much of it into the atmosphere.

Page 29: Impact of eruptions

Food shortages and starvation are attributed to the deaths of 80,000 people.

In June of 1816 there was widespread snowfall throughout the eastern United States.

The normal growing season experienced repeated frosts as cold air extended much more southerly than normal.

The global population was about 1 billion people in 1816.

Our current population is a little over 6 billion.

The 1816 fatality rate would have resulted in a death toll of nearly 500,000 people due to starvation.

Page 30: Impact of eruptions

The concentration mercury in ice cores from glaciers in Wyoming record a peak in atmospheric mercury that corresponds to the Tambora eruption.

The atmospheric impact caused the “year without a summer” along with 80,000 deaths due to famine and disease.

Page 31: Impact of eruptions

Approximately 260,000 people have been killed by volcanoes in historic times…most by a handful of individual eruptions.

Page 32: Impact of eruptions

Volcanic Explosivity Index

Page 33: Impact of eruptions

http://pubs.usgs.gov/publications/msh/comparisons.html

Page 34: Impact of eruptions

Super Volcanoes

While not defined officially, lets say any eruption that ejects 1000 km3 or more of pyroclastic material (i.e., VEI 8 or more).

According to M.R. Rampino super eruptions take place, on average, every 50,000 years. Three of the best known eruptions are compared below.

Page 35: Impact of eruptions

Toba: the world’s largest Quaternary caldera.

The Australian Plate is subducting beneath the Eurasian plate at a rate of 6.7 cm/yr.

Page 36: Impact of eruptions

Today Toba is a caldera or depression that is occupied by Lake Toba.

It is 100 km long and 30 km wide.

Toba last erupted about 75,000 years ago with the largest eruption of the last 2 million years.

Page 37: Impact of eruptions

840,000 years ago

500,000 years ago

Three eruptive events have been recognized.

74,000 years ago

Each producing a caldera.

Samosir Island, rising 750 m above the lake, is a dome built from lava following the last eruption.

Page 38: Impact of eruptions

The eruption ejected 2,800 cubic km of material and the pyroclastic flows covered an area of at least 20,000 square km.

In the immediate vicinity of the volcano ash deposits reach 600 metres in thickness

Ash fall from the eruption covers an area of at least 4 million square km; half the area of the continental United States.

Global cooling is estimated at between 3 and 5 degrees Celsius with regional cooling of 15 degrees C.

Tropical plant life would have been all but eliminated

Temperate forests would loose 50% of all trees.

Page 39: Impact of eruptions

It is estimated that the growing population of homo sapiens (i.e., us) was reduced from 100,000 individuals to as few as 3,000 individuals (97% of all humans were lost!).

This reduction had been estimated for approximately the time of Toba’s eruption on the basis of genetic studies and is termed the “human population bottleneck”.

Page 40: Impact of eruptions

Yellowstone Caldera

Known for its hot springs and geysers, Yellowstone National Park, is likely the most popular super volcano in the world.

The park sits on an active caldera that rises and sinks in response to magma movement and pressure fluctuations within the Earth.

Over recent years the surface has risen by as much as a metre and sunk back by 1/3 of a metre.

Thousands of small earthquakes are produced as earth surface moves.

Page 41: Impact of eruptions

The magma chamber is only 5 to 13 km below the land surface.

The caldera is 80 km long and 50 km wide.

Page 42: Impact of eruptions

The caldera and its magma chamber are due to a hot spot in the mantle that has moved several hundred kilometres over the past 12.5 million years.

The movement is due to the drift of the north American continent over the hot spot.

Ancient, inactive calderas mark the path of the hot spot.

Page 43: Impact of eruptions

The current caldera was formed with an eruption 640,000 years ago (the Lava Creek Eruption).

This eruption ejected 1,000 km3 of pyroclastic debris.

An earlier eruption (the Huckleberry Ridge Eruption, 2 million years ago) ejected 2,500 km3

of pyroclastic debris.

A smaller eruption happened 1.3 million years ago, releasing 280 km3 of debris.

Page 44: Impact of eruptions

Eruptions appear to have a 600,000 year period (that long between eruptions) so we’re overdue for another one.

Previous eruptions spread ash over thousands of km2 across the US.

Page 45: Impact of eruptions

Heightened monitoring of the Yellowstone Caldera in recent years has led to media concern of an impending eruption.

Government officials and geologists indicate that there have been no clear indicators of high risk at this time.

If such an eruption were to take place, North America and the rest of the world could experience another “Dark Ages”.