A new paleomagnetic constraint on the duration of a twin caldera-forming eruption sequence: a potential solution to an enduring problem in decoding >VEI 7 eruption timescales

Abstract New paleomagnetic results from the twin caldera-forming Mamaku–Ohakuri eruption deposits in the Taupō Volcanic Zone of New Zealand show that the entire pyroclastic sequence accumulated within a geomagnetic excursion event. The deposits are predominately unconsolidated and include multiple a...

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Main Authors: Darren M. Gravley, Takeshi Hasegawa, Nobutatsu Mochizuki, Chie Kusu, Makoto Okada
Format: Article
Language:English
Published: SpringerOpen 2025-07-01
Series:Earth, Planets and Space
Subjects:
Online Access:https://doi.org/10.1186/s40623-025-02179-9
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author Darren M. Gravley
Takeshi Hasegawa
Nobutatsu Mochizuki
Chie Kusu
Makoto Okada
author_facet Darren M. Gravley
Takeshi Hasegawa
Nobutatsu Mochizuki
Chie Kusu
Makoto Okada
author_sort Darren M. Gravley
collection DOAJ
description Abstract New paleomagnetic results from the twin caldera-forming Mamaku–Ohakuri eruption deposits in the Taupō Volcanic Zone of New Zealand show that the entire pyroclastic sequence accumulated within a geomagnetic excursion event. The deposits are predominately unconsolidated and include multiple airfall ash units and two caldera-forming ignimbrites. The older Mamaku ignimbrite is moderately welded and has been previously correlated with the ~240 ka Mamaku excursion. By utilizing a refined technique to extract samples from multiple units in the eruption sequence (including the Mamaku ignimbrite) and measuring mean characteristic remanent magnetization directions, we establish that the entire sequence may have occurred over decades to centuries, and that the geomagnetic directional changing rate probably fluctuated significantly during the excursion, up to several degrees per day. More research is required, but we argue that sequences of relatively rapidly deposited pyroclastic material have significant potential in not only refining the timescales of volcano explosivity index (VEI) 7 and larger VEI 8 eruptions, but also as an alternative recorder that could progress some well-documented and unanswered questions in paleomagnetic research, like the stop-and-go character of the geomagnetic field direction during excursions and reversals. Graphical Abstract
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spelling doaj-art-47e66266572d48fbbf6a1d0c6a9ffaf62025-08-20T03:03:38ZengSpringerOpenEarth, Planets and Space1880-59812025-07-0177111410.1186/s40623-025-02179-9A new paleomagnetic constraint on the duration of a twin caldera-forming eruption sequence: a potential solution to an enduring problem in decoding >VEI 7 eruption timescalesDarren M. Gravley0Takeshi Hasegawa1Nobutatsu Mochizuki2Chie Kusu3Makoto Okada4School of Earth and Environment, University of CanterburyDepartment of Earth Science, Ibaraki UniversityDepartment of Earth and Environmental Science, Faculty of Advanced Science and Technology, Kumamoto UniversityDepartment of Earth Science, Ibaraki UniversityDepartment of Earth Science, Ibaraki UniversityAbstract New paleomagnetic results from the twin caldera-forming Mamaku–Ohakuri eruption deposits in the Taupō Volcanic Zone of New Zealand show that the entire pyroclastic sequence accumulated within a geomagnetic excursion event. The deposits are predominately unconsolidated and include multiple airfall ash units and two caldera-forming ignimbrites. The older Mamaku ignimbrite is moderately welded and has been previously correlated with the ~240 ka Mamaku excursion. By utilizing a refined technique to extract samples from multiple units in the eruption sequence (including the Mamaku ignimbrite) and measuring mean characteristic remanent magnetization directions, we establish that the entire sequence may have occurred over decades to centuries, and that the geomagnetic directional changing rate probably fluctuated significantly during the excursion, up to several degrees per day. More research is required, but we argue that sequences of relatively rapidly deposited pyroclastic material have significant potential in not only refining the timescales of volcano explosivity index (VEI) 7 and larger VEI 8 eruptions, but also as an alternative recorder that could progress some well-documented and unanswered questions in paleomagnetic research, like the stop-and-go character of the geomagnetic field direction during excursions and reversals. Graphical Abstracthttps://doi.org/10.1186/s40623-025-02179-9Caldera-forming eruption durationGeomagnetic excursionPaleomagnetic mean directionMamaku–Ohakuri eruption sequence
spellingShingle Darren M. Gravley
Takeshi Hasegawa
Nobutatsu Mochizuki
Chie Kusu
Makoto Okada
A new paleomagnetic constraint on the duration of a twin caldera-forming eruption sequence: a potential solution to an enduring problem in decoding >VEI 7 eruption timescales
Earth, Planets and Space
Caldera-forming eruption duration
Geomagnetic excursion
Paleomagnetic mean direction
Mamaku–Ohakuri eruption sequence
title A new paleomagnetic constraint on the duration of a twin caldera-forming eruption sequence: a potential solution to an enduring problem in decoding >VEI 7 eruption timescales
title_full A new paleomagnetic constraint on the duration of a twin caldera-forming eruption sequence: a potential solution to an enduring problem in decoding >VEI 7 eruption timescales
title_fullStr A new paleomagnetic constraint on the duration of a twin caldera-forming eruption sequence: a potential solution to an enduring problem in decoding >VEI 7 eruption timescales
title_full_unstemmed A new paleomagnetic constraint on the duration of a twin caldera-forming eruption sequence: a potential solution to an enduring problem in decoding >VEI 7 eruption timescales
title_short A new paleomagnetic constraint on the duration of a twin caldera-forming eruption sequence: a potential solution to an enduring problem in decoding >VEI 7 eruption timescales
title_sort new paleomagnetic constraint on the duration of a twin caldera forming eruption sequence a potential solution to an enduring problem in decoding vei 7 eruption timescales
topic Caldera-forming eruption duration
Geomagnetic excursion
Paleomagnetic mean direction
Mamaku–Ohakuri eruption sequence
url https://doi.org/10.1186/s40623-025-02179-9
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