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A hornito on the surface of a lava flow erupted form Kīlauea in 2015. Hornitos are spatter deposits formed at small openings above lava tubes. USGS image.
Introduction
Basaltic lava flows have two major types of morphological forms, ‘a‘ā and pāhoehoe. Pāhoehoe lava flows typically have smooth ropy surfaces, while ‘a‘ā flows are made of very rough and spiny blocks of lava called clinker. Beyond these forms, a number of other smaller structures may be found on the surface of lava flows, although most of these features are generally more common on pāhoehoe flows. Together, these surface features reveal important information of the specific dynamics that occurred during the eruption and emplacement of these flows.
Surface Features
Vesicles
Vesicles form from volcanic gases (mostly water, H2O; carbon dioxide, CO2, and sulfur dioxide SO2) escaping and expanding from molten lava. The upper portion of lava flows are typically vesicular, and are a result of gas bubbles growing within the flow and then rising towards the surface. Sometimes vesicles are elongated and shaped like pipes.

Vesicular surface of a basaltic lava flow from Sunset Crater Volcano National Monument. John St. James photo on Flickr.

Close up of vesicles in a basaltic lava flow from Craters of the Moon National Monument. John St. James photo on Flickr.
Hornitos
A hornito (“little oven” in Spanish) is a small mound or spire of spatter that formed on a lava flow or lava lake. They are rootless in that they develop away from volcanic vents when pressure forces some of the underlying molten lava through cracks or openings in the congealed surface and sometimes occur above a lava tube. They are mostly found on pāhoehoe lava flows.

Two hornitos in Craters of the Moon National Monument. Niles JH and Others. 2011. Geologic Map of the Core Visitation Area of Craters of the Moon National Monument and Preserve, South-central Idaho, with Descriptions of 38 Points of Geologic Interest.

A cross-section of a hornito above a lava tube, Kīlauea Volcano, Hawai’i Volcanoes National Park. USGS photo.
Levee
Lava levees are natural banks along the sides of lava flowing in a channel. They develop on the chilled margins of a lava flow and may be higher than the surface of the flowing lava flow if flow rate decreases.

Small overflows of lava over a levee on a lava channel during the 2018 eruption of Kīlauea. Overflows can add to the height of levels. USGS Hawaii Volcano Observatory photo.
Pressure Ridges
Pressure ridges are elongated, usually arcuate, ridges on the crust of a lava flow formed by laterally directed pressure.

Pressure ridges on one of the lava flows that erupted from Capulin Volcano approximately 54,200 years ago. NPS photo.
Festoon
A festoon is a subtype of pressure ridge. Festoons are formed by movement of underlying molten lava. They can be small features ranging from a few inches (cm) to large features that are 10s–100s ft (meters) in size.

Festoon on a lava erupted from Kīlauea Volcano, Hawai’i Volcanoes National Park in 2003. Width of festoon is about 3.3 ft (1 m). USGS photo.
Tumulus
Tumuli (pl.) are small (usually less than 33 ft; 10 m) dome-shaped structures that are mostly found on the surfaces of pāhoehoe flows. They are formed when pressure within an inflating lava flow buckles up its solidified crust. Molten lava may sometimes be squeezed out through a crack in a tumulus. Unlike hornitos, tumuli aren’t usually found above lava tubes.

Molten lava escaping out of a tumulus on a lava flow during an eruption from Kīlauea Volcano, Hawai’i Volcanoes National Park in 2016. The tumulus is about 10 ft (3 m) tall. USGS photo.

A tumulus on the Lost Jim lava flow that erupted between 1,000 and 2,000 years ago in Bering Land Bridge National Preserve. USGS Alaska Volcano Observatory photo by Tim Orr.
Squeeze-up
Squeeze-ups are small extrusions of viscous lava through a crack or opening in the solid crust of a lava flow. They are either bulbous and look like a mass of toothpaste squeezed from a tube or are linear wedges in the core of tumuli.

A squeeze-up on a lava flow erupted from Kīlauea Volcano, Hawai’i Volcanoes National Park in 2003. USGS photo.

A squeeze-up in Craters of the Moon National Monument. John St. James Photo on Flickr.
Tree Molds
Tree molds are fossils found in lava flows where lava envelopes a tree and forms an impression of it before the tree is burnt away by the hot lava.

A large tree mold in Craters of the Moon National Monument. Niles JH and Others. 2011. Geologic Map of the Core Visitation Area of Craters of the Moon National Monument and Preserve, South-central Idaho, with Descriptions of 38 Points of Geologic Interest
Flow Glaze
The outermost part of young unweathered lava flows typically retains its glassy rind, which most commonly has a shiny black color. But sometimes the glassy rinds on the surface of young lava flows have an unusual hue such as iridescent blue. Blue flow glazes are known from lava flows erupted from Kīlauea in Hawai’i Volcanoes National Park and the Blue Dragon Flow in Craters of the Moon National Monument. The blue color likely results from the refractive index of the glass and may be a result of the presence of titanium in tiny magnetite crystals embedded in the clear brown volcanic glass.

Flow glaze on the Blue Dragon Flow in Craters of the Moon National Monument. Niles JH and Others. 2011. Geologic Map of the Core Visitation Area of Craters of the Moon National Monument and Preserve, South-central Idaho, with Descriptions of 38 Points of Geologic Interest.
Featured Parks
Bering Land Bridge National Preserve (BELA), Alaska—[BELA Geodiversity Atlas] [BELA Park Home] [BELA npshistory.com]
Capulin Volcano National Monument (CAVO), New Mexico—[CAVO Geodiversity Atlas] [CAVO ParkHome ] [CAVO npshistory.com]
Craters of the Moon National Monument (CRMO), Idaho—[CRMO Geodiversity Atlas] [CRMO ParkHome] [CRMO npshistory.com]
Hawai’i Volcanoes National Park (HAVO), Hawai’i—[HAVO Geodiversity Atlas] [HAVO ParkHome] [HAVO npshistory.com]
Sunset Crater Volcano National Monument (SUCR), Arizona—[SUCR Geodiversity Atlas] [SUCR ParkHome] [SUCR npshistory.com]
Volcanoes, Craters, and Lava Flows
Where this belongs
- Bering Land Bridge National Preserve
- Capulin Volcano National Monument
- Craters Of The Moon National Monument & Preserve
- Hawaiʻi Volcanoes National Park
- Kaloko-Honokōhau National Historical Park
- Kalaupapa National Historical Park
Where this page came from
This page was imported from National Park Service. Produced by the U.S. National Park Service and, as a work of the United States government, in the public domain.
Nobody has written it yet — it is the source material at a new address, which is why search engines are asked to skip it and why no one earns from it. It is up for grabs: take it on, and it is yours to rewrite and to earn from.
I disse publikationerBering Land Bridge National PreserveHawaiʻi Volcanoes National ParkCraters Of The Moon National Monument & PreserveKalaupapa National Historical ParkCapulin Volcano National Monument
Licens: CC0 1.0 (offentligt eje) · Bearbejdet efter www.nps.gov
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