Explosive 2 Flashcards

(34 cards)

1
Q

What often follows large Plinian eruptions?

A

Caldera collapse (Mazama-type) often follows large Plinian eruptions.

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2
Q

What does the size of a caldera indicate?

A

It provides a qualitative indication of the area of the magma body beneath the volcano.

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3
Q

What is the typical range of gas content in magma during explosive eruptions?

A

2 to 7% gas content is typical.

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4
Q

What are typical exit velocities in Plinian eruptions?

A

Exit velocities range from 200 to 600 m/s (supersonic).

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5
Q

Name the three main regions of a Plinian eruption column.

A

Gas Thrust Region, Convective Region, and Umbrella Region.

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6
Q

What happens in the Gas Thrust Region?

A

Rapid vertical movement of gas and magma fragments, powered by gas expansion (decompression).

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7
Q

Where does the fragmentation surface occur?

A

Usually a few hundred meters below the surface.

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8
Q

When does the Gas Thrust Region end?

A

When gas pressure (Pgas) equals atmospheric pressure (Patm).

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9
Q

Why does the eruption column become buoyant?

A

Because as particles fall out, the column density decreases and the hot gases become less dense than air.

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10
Q

What defines the Convective Region?

A

Air entrainment and heating make the plume less dense than the surrounding air, allowing it to rise convectively.

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11
Q

What determines how high an eruption column rises?

A

Mainly the mass flux rate and atmospheric temperature gradient.

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12
Q

What was the estimated volume discharge rate during the 1991 Pinatubo eruption?

A

Approximately 210,000 m³/s.

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13
Q

What was the calculated column height (HT) for the Pinatubo eruption?

A

About 40 km.

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14
Q

How does column width change with height?

A

It increases approximately 0.2–0.5 times the column height due to air entrainment.

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15
Q

At what atmospheric boundary does the umbrella region often form?

A

At the tropopause (between troposphere and stratosphere).

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16
Q

What determines whether an eruption column convects or collapses?

A

The relative densities of the eruption column and surrounding atmosphere.

17
Q

What gas compositions make convection more difficult?

A

Higher CO₂/H₂O ratios make plumes too dense for convection.

18
Q

Why is air entrainment important?

A

It dilutes the ash and lowers the density of the eruption column to allow convection.

19
Q

Where does air entrainment occur?

A

At the interface between the eruption column and surrounding air.

20
Q

How does vent radius affect air entrainment?

A

Narrow vents enhance air entrainment; wide vents entrain proportionally less air.

21
Q

What controls heating efficiency during entrainment?

A

Grain size—smaller grains lose heat more rapidly, increasing heating efficiency.

22
Q

What is terminal fall velocity (TFV)?

A

The velocity at which a clast falls through the air when upward and downward forces balance.

23
Q

How does wind affect eruption plumes?

A

Wind determines the direction and shape of the umbrella region and disperses ash downwind.

24
Q

What causes column collapse?

A

Decreased eruption velocity or increased vent width, reducing air entrainment and stability.

25
What are the two main column collapse scenarios?
1) Vent widens, reducing stability; 2) Water content drops, lowering eruption velocity.
26
Who documented the Vesuvius 79 AD eruption?
Pliny the Younger, in letters to the historian Tacitus.
27
What were the main eruption units of Vesuvius 79 AD?
EU1 (basal surge), EU2 (White Pumice), EU3 (Grey Pumice).
28
What does EU2 represent?
A Plinian eruption phase producing well-bedded white pumice.
29
What does EU3 represent?
A more intense phase with grey pumice and column heights up to 32 km.
30
What caused the compositional change between EU2 and EU3?
The eruption scoured deeper into the zoned magma chamber, tapping more mafic magma.
31
What caused the pyroclastic flows during the Vesuvius eruption?
Column collapse during high discharge phases.
32
What was the likely cause of the phreatomagmatic deposits at Vesuvius?
Interaction between magma and groundwater from a regional aquifer.
33
How deep was the magma chamber at Vesuvius?
Approximately 3–5 km deep.
34
What was the aftermath of the 79 AD eruption?
Thousands died, the area was abandoned and rediscovered in 1595; excavation began in 1748.