TY - JOUR
T1 - Geomorphological characterization of the 2014–2015 Holuhraun lava flow-field in Iceland
AU - Voigt, Joana R.C.
AU - Hamilton, Christopher W.
AU - Scheidt, Stephen P.
AU - Münzer, Ulrich
AU - Höskuldsson, Ármann
AU - Jónsdottir, Ingibjörg
AU - Thordarson, Thorvaldur
N1 - Funding Information:
We thank two anonymous reviewers and Stephen Self for their thoughtful reviews that greatly improved this manuscript. J.R.C.V. acknowledges the Geological Society of America (GSA) for supporting the field trip in 2016 with a Graduate Student Research Grant and the GSA Lipman Research Award and the Future Investigators in NASA Earth and Space Science and Technology program (Grant # NNH19ZDA001N-FINESST). C.W.H. acknowledges support from the NASA Planetary Science and Technology from Analog Research program (Grant # 80NSSC21K0011 ), NASA Planetary Geology and Geophysics program (Grant # NNX14AL54G ), the W.M. Keck Foundation, and a Fulbright–NSF Arctic Research Scholarship administered by Fulbright–Iceland . The authors also thank the Goddard Instrument Field Team (GIFT) for partially supporting J.R.C.V.'s participation in the field campaigns conducted during the summers of 2018 and 2019. We also acknowledge the Iceland subglacial Volcanoes interdisciplinary early warning system (IsViews), which was managed by the Ludwig Maximilians University, Munich, and funded by the Bavarian Ministry of Economic Affairs and Media, Energy and Technology ( ID 20-8-34102-15-2012 ). The team thanks the Icelandic Research Centre (Rannsóknamiðstöð Íslands) and the Vatnajökull National Park Service (Vatnajökulsþjóðgarður) for providing permission to work within the Holuhraun region; as well as Patrick Whelley, Jacob Richardson, Sarah Sutton, Gavin Tolometti, Catherine Neish, and many others for their assistance during summer field campaigns conducted in 2015–2019.
Funding Information:
We thank two anonymous reviewers and Stephen Self for their thoughtful reviews that greatly improved this manuscript. J.R.C.V. acknowledges the Geological Society of America (GSA) for supporting the field trip in 2016 with a Graduate Student Research Grant and the GSA Lipman Research Award and the Future Investigators in NASA Earth and Space Science and Technology program (Grant # NNH19ZDA001N-FINESST). C.W.H. acknowledges support from the NASA Planetary Science and Technology from Analog Research program (Grant # 80NSSC21K0011), NASA Planetary Geology and Geophysics program (Grant # NNX14AL54G), the W.M. Keck Foundation, and a Fulbright–NSF Arctic Research Scholarship administered by Fulbright–Iceland. The authors also thank the Goddard Instrument Field Team (GIFT) for partially supporting J.R.C.V.'s participation in the field campaigns conducted during the summers of 2018 and 2019. We also acknowledge the Iceland subglacial Volcanoes interdisciplinary early warning system (IsViews), which was managed by the Ludwig Maximilians University, Munich, and funded by the Bavarian Ministry of Economic Affairs and Media, Energy and Technology (ID 20-8-34102-15-2012). The team thanks the Icelandic Research Centre (Rannsóknamiðstöð Íslands) and the Vatnajökull National Park Service (Vatnajökulsþjóðgarður) for providing permission to work within the Holuhraun region; as well as Patrick Whelley, Jacob Richardson, Sarah Sutton, Gavin Tolometti, Catherine Neish, and many others for their assistance during summer field campaigns conducted in 2015–2019.
Publisher Copyright:
© 2021 The Author(s)
PY - 2021/11
Y1 - 2021/11
N2 - The 2014–2015 Holuhraun eruption extruded >1 km3 of lava in a barren region of the Icelandic highlands. Due to its large volume and the abundance of data for this eruption, Holuhraun is an ideal site to investigate fissure-fed eruption products for comparison with other large lava flow-fields on Earth and other planetary bodies. To characterize lava morphologies associated with this event, we used 0.01–0.5 m/pixel image data, acquired from aerial surveys and small Unoccupied Aircraft Systems (sUAS) to create a 1:800-scale facies map that was ground-truthed using field observations during the summers of 2015–2019. Each facies region exhibits similar attributes in the remote sensing data, including albedo, surface texture, and geomorphology. However, at our mapping scale of 1:800, the facies typically include mixtures of lava types. Results show that transitional lava types (e.g., rubbly pāhoehoe, slabby pāhoehoe, and spiny pāhoehoe) dominate the 2014–2015 Holuhraun lava flow-field (83.82 km2), rather than the traditional end-members of ʻaʻā and classical pāhoehoe. At 1:800-scale, we distinguish the following eight facies (with the percentage of total flow-field area shown in parentheses): rubbly (57.35%), spiny (25.96%), undifferentiated rubbly–spiny (9.59%), shelly (5.58%), pāhoehoe (1.24%), flat-lying–knobby (0.58%), vent-proximal edifice (0.19%), and channel interior (0.16%). Field observations show that initial coherent pāhoehoe surfaces were episodically disrupted to produce slabby and rubbly textures that resemble ʻaʻā in remote sensing data. Our observations also show that continued solidification of the lava beneath brecciated surfaces can cause the surfaces of disrupted lobes to stabilize, or restabilize and undergo inflation. These factors complicate the use of surface texture as a direct indicator of emplacement style, which can change over the course of an eruption. This complexity has important implications for reconstructing the emplacement history of flow-fields on Earth and other planetary bodies.
AB - The 2014–2015 Holuhraun eruption extruded >1 km3 of lava in a barren region of the Icelandic highlands. Due to its large volume and the abundance of data for this eruption, Holuhraun is an ideal site to investigate fissure-fed eruption products for comparison with other large lava flow-fields on Earth and other planetary bodies. To characterize lava morphologies associated with this event, we used 0.01–0.5 m/pixel image data, acquired from aerial surveys and small Unoccupied Aircraft Systems (sUAS) to create a 1:800-scale facies map that was ground-truthed using field observations during the summers of 2015–2019. Each facies region exhibits similar attributes in the remote sensing data, including albedo, surface texture, and geomorphology. However, at our mapping scale of 1:800, the facies typically include mixtures of lava types. Results show that transitional lava types (e.g., rubbly pāhoehoe, slabby pāhoehoe, and spiny pāhoehoe) dominate the 2014–2015 Holuhraun lava flow-field (83.82 km2), rather than the traditional end-members of ʻaʻā and classical pāhoehoe. At 1:800-scale, we distinguish the following eight facies (with the percentage of total flow-field area shown in parentheses): rubbly (57.35%), spiny (25.96%), undifferentiated rubbly–spiny (9.59%), shelly (5.58%), pāhoehoe (1.24%), flat-lying–knobby (0.58%), vent-proximal edifice (0.19%), and channel interior (0.16%). Field observations show that initial coherent pāhoehoe surfaces were episodically disrupted to produce slabby and rubbly textures that resemble ʻaʻā in remote sensing data. Our observations also show that continued solidification of the lava beneath brecciated surfaces can cause the surfaces of disrupted lobes to stabilize, or restabilize and undergo inflation. These factors complicate the use of surface texture as a direct indicator of emplacement style, which can change over the course of an eruption. This complexity has important implications for reconstructing the emplacement history of flow-fields on Earth and other planetary bodies.
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U2 - 10.1016/j.jvolgeores.2021.107278
DO - 10.1016/j.jvolgeores.2021.107278
M3 - Article
AN - SCOPUS:85111918330
SN - 0377-0273
VL - 419
JO - Journal of Volcanology and Geothermal Research
JF - Journal of Volcanology and Geothermal Research
M1 - 107278
ER -