A hot midmantle anomaly in the area of the Indian Ocean Geoid Low

Abstract We investigate the upper mantle seismic discontinuities at 410 and 660 km depth beneath the Indian Ocean Geoid Low (IOGL). To map the discontinuities' topography, we use differential travel times of PP and SS waves and their precursors. Our final data set consists of 37 events with Mw ...

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Main Authors: Anne‐Sophie Reiss, Christine Thomas, Jac vanDriel, Björn Heyn
Format: Article
Language:English
Published: Wiley 2017-07-01
Series:Geophysical Research Letters
Subjects:
Online Access:https://doi.org/10.1002/2017GL073440
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author Anne‐Sophie Reiss
Christine Thomas
Jac vanDriel
Björn Heyn
author_facet Anne‐Sophie Reiss
Christine Thomas
Jac vanDriel
Björn Heyn
author_sort Anne‐Sophie Reiss
collection DOAJ
description Abstract We investigate the upper mantle seismic discontinuities at 410 and 660 km depth beneath the Indian Ocean Geoid Low (IOGL). To map the discontinuities' topography, we use differential travel times of PP and SS waves and their precursors. Our final data set consists of 37 events with Mw ≥ 5.8, which densely cover our investigation area, also with crossing ray paths. We use array methods to detect the low‐amplitude precursor signals. The best quality data show a deepened 410 km discontinuity in the center of the IOGL as well as a mostly elevated 660 km discontinuity beneath the northern Indian Ocean, which we interpret as a hot anomaly currently residing in the mantle transition zone. We conclude that the largest negative geoid anomaly might be caused by a combined effect of hot material in the midmantle below the innermost IOGL and cold material below 660 km farther south.
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publishDate 2017-07-01
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series Geophysical Research Letters
spelling doaj-art-bc177ecd9d1d4ff8964f1ce1aa57d7292025-08-20T01:51:46ZengWileyGeophysical Research Letters0094-82761944-80072017-07-0144136702671110.1002/2017GL073440A hot midmantle anomaly in the area of the Indian Ocean Geoid LowAnne‐Sophie Reiss0Christine Thomas1Jac vanDriel2Björn Heyn3Westfälische Wilhelms‐Universität Münster Münster GermanyWestfälische Wilhelms‐Universität Münster Münster GermanyUniversity College London London UKWestfälische Wilhelms‐Universität Münster Münster GermanyAbstract We investigate the upper mantle seismic discontinuities at 410 and 660 km depth beneath the Indian Ocean Geoid Low (IOGL). To map the discontinuities' topography, we use differential travel times of PP and SS waves and their precursors. Our final data set consists of 37 events with Mw ≥ 5.8, which densely cover our investigation area, also with crossing ray paths. We use array methods to detect the low‐amplitude precursor signals. The best quality data show a deepened 410 km discontinuity in the center of the IOGL as well as a mostly elevated 660 km discontinuity beneath the northern Indian Ocean, which we interpret as a hot anomaly currently residing in the mantle transition zone. We conclude that the largest negative geoid anomaly might be caused by a combined effect of hot material in the midmantle below the innermost IOGL and cold material below 660 km farther south.https://doi.org/10.1002/2017GL073440Indian Ocean Geoid Lowmantle discontinuitiesarray seismology
spellingShingle Anne‐Sophie Reiss
Christine Thomas
Jac vanDriel
Björn Heyn
A hot midmantle anomaly in the area of the Indian Ocean Geoid Low
Geophysical Research Letters
Indian Ocean Geoid Low
mantle discontinuities
array seismology
title A hot midmantle anomaly in the area of the Indian Ocean Geoid Low
title_full A hot midmantle anomaly in the area of the Indian Ocean Geoid Low
title_fullStr A hot midmantle anomaly in the area of the Indian Ocean Geoid Low
title_full_unstemmed A hot midmantle anomaly in the area of the Indian Ocean Geoid Low
title_short A hot midmantle anomaly in the area of the Indian Ocean Geoid Low
title_sort hot midmantle anomaly in the area of the indian ocean geoid low
topic Indian Ocean Geoid Low
mantle discontinuities
array seismology
url https://doi.org/10.1002/2017GL073440
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