Book contents
- Frontmatter
- Contents
- Preface
- Part I Introductory Material
- Part II Kinematics, Dynamics and Rheology
- Part III Waves in Non-Rotating Fluids
- Part IV Waves in Rotating Fluids
- Part V Non-Rotating Flows
- Part VI Flows in Rotating Fluids
- Part VII Silicate Flows
- 29 Equations Governing Silicate Flows
- 30 Cooling the Earth
- 31 Cooling the Mantle
- 32 Cooling the Core
- 33 Overview of Volcanic Flows
- 34 Flow in Volcanic Conduits
- 35 Lava Flows
- Part VIII Fundaments
35 - Lava Flows
from Part VII - Silicate Flows
Published online by Cambridge University Press: 26 October 2017
- Frontmatter
- Contents
- Preface
- Part I Introductory Material
- Part II Kinematics, Dynamics and Rheology
- Part III Waves in Non-Rotating Fluids
- Part IV Waves in Rotating Fluids
- Part V Non-Rotating Flows
- Part VI Flows in Rotating Fluids
- Part VII Silicate Flows
- 29 Equations Governing Silicate Flows
- 30 Cooling the Earth
- 31 Cooling the Mantle
- 32 Cooling the Core
- 33 Overview of Volcanic Flows
- 34 Flow in Volcanic Conduits
- 35 Lava Flows
- Part VIII Fundaments
Summary
Commonly andesitic and rhyolitic magmas rise up discrete conduits, whereas basaltic magma often – at least during the early stages of an eruption phase – rises to the surface through a magmatic dike (also called a rift or fissure): a linear crack extending from a magma chamber at depth to the surface. Typically as magma erupts from a dike, outgassed volatiles (mainly water) produce a linear fire fountain composed of incandescent blobs of lava.
After magma reaches the surface, its subsequent behavior depends largely whether the eruption is effusive or explosive. A discussion of the possible styles of lava flow is found in Griffiths (2000). Effusive eruptions lead to the production of lava which flows relatively gently downslope, initially in the form of a planar sheet. We will consider a simple model of lava sheet flow in the following section.
On the other hand, explosive eruptions display a variety of behaviors depending on the speed, mass flow and composition of the erupting magma. Some of these behaviors are explored in § 35.2.
Lava Sheet Flow
In this section we will develop a simple model of subaerial (that is, on land, as opposed to under the sea) lava sheet flow: a sheet of hot basaltic lava flowing steadily down a slope (in the x direction) from a magmatic dike.
Our simple model will ignore
• variations in topography;
• horizontal variations in the lava surface;
• fluid inertia;
• loss of heat to the ground;
• radiative cooling;
• variations in the ambient temperature;
• effects of rain;
• the dynamic effect of crystals suspended in the liquid lava;
• buoyancy effects; and
• variations of thermal conductivity with temperature.
In order to simplify the analysis further, we will assume that the cool upper layer of lava is rafted along with the flow, rather than being anchored to the ground at the sides. The weight of this rafted layer is borne by the liquid beneath, so that there is a vertical hydrostatic balance. This rafted layer may deform as needed in order to adjust to the flow of the liquid beneath.
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- Information
- Geophysical Waves and FlowsTheory and Applications in the Atmosphere, Hydrosphere and Geosphere, pp. 367 - 378Publisher: Cambridge University PressPrint publication year: 2017