Skip to main content Accessibility help
×
Hostname: page-component-77c89778f8-vpsfw Total loading time: 0 Render date: 2024-07-21T07:21:32.970Z Has data issue: false hasContentIssue false

35 - Lava Flows

from Part VII - Silicate Flows

Published online by Cambridge University Press:  26 October 2017

David E. Loper
Affiliation:
Florida State University
Get access

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.

    Type
    Chapter
    Information
    Geophysical Waves and Flows
    Theory and Applications in the Atmosphere, Hydrosphere and Geosphere
    , pp. 367 - 378
    Publisher: Cambridge University Press
    Print publication year: 2017

    Access options

    Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

    Save book to Kindle

    To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

    Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

    Find out more about the Kindle Personal Document Service.

    • Lava Flows
    • David E. Loper, Florida State University
    • Book: Geophysical Waves and Flows
    • Online publication: 26 October 2017
    • Chapter DOI: https://doi.org/10.1017/9781316888858.043
    Available formats
    ×

    Save book to Dropbox

    To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

    • Lava Flows
    • David E. Loper, Florida State University
    • Book: Geophysical Waves and Flows
    • Online publication: 26 October 2017
    • Chapter DOI: https://doi.org/10.1017/9781316888858.043
    Available formats
    ×

    Save book to Google Drive

    To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

    • Lava Flows
    • David E. Loper, Florida State University
    • Book: Geophysical Waves and Flows
    • Online publication: 26 October 2017
    • Chapter DOI: https://doi.org/10.1017/9781316888858.043
    Available formats
    ×