World's Best Scientists 2026 revealed!

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Earth Science 40 5897 5457 296 281 177 5414

Meghan S. Miller publications per year

The chart shows the history of publications by Meghan S. Miller between 2000 and 2026, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Meghan S. Miller published across 27 years, from 2000 to 2026, averaging 8.1 papers a year. Output peaked at 19 publications in 2014. 13 of the 220 publications appeared in the last two years.

No. of publications
5 10 15
Bar chart. Horizontal axis: year, 2000 to 2026. Vertical axis: number of publications, 0 to 19. Peak 19 publications in 2014. 2000: 2 publications 2001: 1 publication 2002: 0 publications 2003: 1 publication 2004: 1 publication 2005: 2 publications 2006: 7 publications 2007: 2 publications 2008: 8 publications 2009: 4 publications 2010: 6 publications 2011: 4 publications 2012: 14 publications 2013: 15 publications 2014: 19 publications 2015: 16 publications 2016: 6 publications 2017: 9 publications 2018: 9 publications 2019: 13 publications 2020: 15 publications 2021: 13 publications 2022: 13 publications 2023: 11 publications 2024: 16 publications 2025: 12 publications 2026: 1 publication
2000 2026

220 publications in total across all disciplines

View publications per year as a table
Meghan S. Miller: publications per year, 2000 to 2026
Year Publications
2000 2
2001 1
2002 0
2003 1
2004 1
2005 2
2006 7
2007 2
2008 8
2009 4
2010 6
2011 4
2012 14
2013 15
2014 19
2015 16
2016 6
2017 9
2018 9
2019 13
2020 15
2021 13
2022 13
2023 11
2024 16
2025 12
2026 1
Total 220
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Meghan S. Miller publication distribution in Earth Science in 2026

The chart shows the distribution of publications by all Research.com ranked scientists in the field of Earth Science in 2026. The highlighted bar marks where Meghan S. Miller sits on this spectrum.

No. of scientists
100 200 300 400 500
Bar chart with 58 bars. Horizontal axis: publications, 38–47 to 603+. Vertical axis: number of scientists, 0 to 557. Most scientists, 557, have 128–137 publications. The last bar groups every scientist with 603 publications or more. The highlighted bar, 168–177 publications, is where this scientist sits. 38–47 publications: 5 scientists 48–57 publications: 33 scientists 58–67 publications: 94 scientists 68–77 publications: 161 scientists 78–87 publications: 278 scientists 88–97 publications: 376 scientists 98–107 publications: 404 scientists 108–117 publications: 484 scientists 118–127 publications: 540 scientists 128–137 publications: 557 scientists 138–147 publications: 491 scientists 148–157 publications: 495 scientists 158–167 publications: 458 scientists 168–177 publications: 490 scientists 178–187 publications: 414 scientists 188–197 publications: 401 scientists 198–207 publications: 333 scientists 208–217 publications: 292 scientists 218–227 publications: 290 scientists 228–237 publications: 262 scientists 238–247 publications: 243 scientists 248–257 publications: 208 scientists 258–267 publications: 185 scientists 268–277 publications: 147 scientists 278–287 publications: 128 scientists 288–297 publications: 119 scientists 298–307 publications: 120 scientists 308–317 publications: 107 scientists 318–327 publications: 93 scientists 328–337 publications: 87 scientists 338–347 publications: 64 scientists 348–357 publications: 87 scientists 358–367 publications: 60 scientists 368–377 publications: 60 scientists 378–387 publications: 34 scientists 388–397 publications: 50 scientists 398–407 publications: 44 scientists 408–417 publications: 31 scientists 418–427 publications: 39 scientists 428–437 publications: 27 scientists 438–447 publications: 36 scientists 448–457 publications: 27 scientists 458–467 publications: 29 scientists 468–477 publications: 30 scientists 478–487 publications: 19 scientists 488–497 publications: 15 scientists 498–507 publications: 18 scientists 508–517 publications: 19 scientists 518–527 publications: 16 scientists 528–537 publications: 10 scientists 538–547 publications: 11 scientists 548–557 publications: 14 scientists 558–567 publications: 11 scientists 568–577 publications: 7 scientists 578–587 publications: 14 scientists 588–597 publications: 5 scientists 598–602 publications: 4 scientists 603+ publications: 100 scientists
38–47 publications 603+

This scientist: 177 publications — 53rd percentile

53% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 603 publications or more.

View publications distribution as a table
Number of Earth Science scientists by publication count, Research.com 2026 ranking edition. Based on 9,176 ranked scientists.
Publications Scientists This scientist
38–47 5
48–57 33
58–67 94
68–77 161
78–87 278
88–97 376
98–107 404
108–117 484
118–127 540
128–137 557
138–147 491
148–157 495
158–167 458
168–177 490 177
178–187 414
188–197 401
198–207 333
208–217 292
218–227 290
228–237 262
238–247 243
248–257 208
258–267 185
268–277 147
278–287 128
288–297 119
298–307 120
308–317 107
318–327 93
328–337 87
338–347 64
348–357 87
358–367 60
368–377 60
378–387 34
388–397 50
398–407 44
408–417 31
418–427 39
428–437 27
438–447 36
448–457 27
458–467 29
468–477 30
478–487 19
488–497 15
498–507 18
508–517 19
518–527 16
528–537 10
538–547 11
548–557 14
558–567 11
568–577 7
578–587 14
588–597 5
598–602 4
603+ 100
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Meghan S. Miller D-index placement in Earth Science in 2026

The chart shows the D-index (discipline H-index) distribution of Earth Science scientists ranked by Research.com in 2026. The highlighted bar marks where Meghan S. Miller sits on this spectrum.

No. of scientists
100 200 300
Bar chart with 77 bars. Horizontal axis: D-Index, 30 to 106+. Vertical axis: number of scientists, 0 to 389. Most scientists, 389, have 36 D-Index. The last bar groups every scientist with 106 D-Index or more. The highlighted bar, 40 D-Index, is where this scientist sits. 30 D-Index: 144 scientists 31 D-Index: 215 scientists 32 D-Index: 278 scientists 33 D-Index: 379 scientists 34 D-Index: 366 scientists 35 D-Index: 372 scientists 36 D-Index: 389 scientists 37 D-Index: 366 scientists 38 D-Index: 344 scientists 39 D-Index: 349 scientists 40 D-Index: 296 scientists 41 D-Index: 289 scientists 42 D-Index: 277 scientists 43 D-Index: 279 scientists 44 D-Index: 248 scientists 45 D-Index: 257 scientists 46 D-Index: 212 scientists 47 D-Index: 202 scientists 48 D-Index: 207 scientists 49 D-Index: 204 scientists 50 D-Index: 183 scientists 51 D-Index: 178 scientists 52 D-Index: 182 scientists 53 D-Index: 178 scientists 54 D-Index: 163 scientists 55 D-Index: 117 scientists 56 D-Index: 163 scientists 57 D-Index: 120 scientists 58 D-Index: 113 scientists 59 D-Index: 136 scientists 60 D-Index: 135 scientists 61 D-Index: 96 scientists 62 D-Index: 103 scientists 63 D-Index: 83 scientists 64 D-Index: 103 scientists 65 D-Index: 83 scientists 66 D-Index: 89 scientists 67 D-Index: 92 scientists 68 D-Index: 89 scientists 69 D-Index: 78 scientists 70 D-Index: 75 scientists 71 D-Index: 53 scientists 72 D-Index: 62 scientists 73 D-Index: 54 scientists 74 D-Index: 35 scientists 75 D-Index: 52 scientists 76 D-Index: 50 scientists 77 D-Index: 32 scientists 78 D-Index: 37 scientists 79 D-Index: 20 scientists 80 D-Index: 33 scientists 81 D-Index: 36 scientists 82 D-Index: 34 scientists 83 D-Index: 34 scientists 84 D-Index: 24 scientists 85 D-Index: 19 scientists 86 D-Index: 18 scientists 87 D-Index: 26 scientists 88 D-Index: 30 scientists 89 D-Index: 17 scientists 90 D-Index: 21 scientists 91 D-Index: 19 scientists 92 D-Index: 15 scientists 93 D-Index: 14 scientists 94 D-Index: 20 scientists 95 D-Index: 9 scientists 96 D-Index: 10 scientists 97 D-Index: 15 scientists 98 D-Index: 13 scientists 99 D-Index: 3 scientists 100 D-Index: 13 scientists 101 D-Index: 3 scientists 102 D-Index: 9 scientists 103 D-Index: 4 scientists 104 D-Index: 6 scientists 105 D-Index: 6 scientists 106+ D-Index: 98 scientists
30 D-Index 106+

This scientist: 40 D-Index — 38th percentile

38% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 106 D-Index or more.

View D-Index distribution as a table
Number of Earth Science scientists by D-index, Research.com 2026 ranking edition. Based on 9,176 ranked scientists.
D-Index Scientists This scientist
30 144
31 215
32 278
33 379
34 366
35 372
36 389
37 366
38 344
39 349
40 296 40
41 289
42 277
43 279
44 248
45 257
46 212
47 202
48 207
49 204
50 183
51 178
52 182
53 178
54 163
55 117
56 163
57 120
58 113
59 136
60 135
61 96
62 103
63 83
64 103
65 83
66 89
67 92
68 89
69 78
70 75
71 53
72 62
73 54
74 35
75 52
76 50
77 32
78 37
79 20
80 33
81 36
82 34
83 34
84 24
85 19
86 18
87 26
88 30
89 17
90 21
91 19
92 15
93 14
94 20
95 9
96 10
97 15
98 13
99 3
100 13
101 3
102 9
103 4
104 6
105 6
106+ 98
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Overview

Meghan S. Miller is affiliated with the Australian National University in Australia, specializing in Earth and Planetary Sciences with a focus on geophysics. Their research portfolio includes significant contributions in various subfields such as geophysics, geology, artificial intelligence, ocean engineering, and environmental chemistry.

The primary themes of their work revolve around earthquake and tectonic studies, high-pressure geophysics and materials, geological and geochemical analysis, and seismic wave analysis. Additional research interests include geological and geophysical studies, seismic imaging, inversion techniques, and seismology in general. These topics highlight a broad yet focused engagement with the physical properties and dynamic behaviors of the Earth's interior.

Meghan S. Miller has published extensively in prominent scientific venues, frequently contributing to journals such as Seismological Research Letters, Zenodo (CERN European Organization for Nuclear Research), Geophysical Research Letters, Geochemistry Geophysics Geosystems, and the Journal of Geophysical Research Solid Earth. These recurring publication venues underscore a consistent engagement with the academic community focused on geosciences and seismic research.

Collaboration forms a significant part of Miller's academic output, with frequent co-authors including Pepen Supendi, Sri Widiyantoro, Nicholas Rawlinson, Ping Zhang, and Ruth Murdie. This network reflects a collaborative approach across multiple research groups and geographic regions.

Recent notable publications by Meghan S. Miller include:

  • Global quieting of high-frequency seismic noise due to COVID-19 pandemic lockdown measures, 2020, Science
  • A comparison of oceanic and continental mantle lithosphere, 2020, Physics of The Earth and Planetary Interiors
  • Fate of Forearc Lithosphere at Arc-Continent Collision Zones: Evidence From Local Earthquake Tomography of the Sunda-Banda Arc Transition, Indonesia, 2020, Geophysical Research Letters
  • SASSY21: A 3-D Seismic Structural Model of the Lithosphere and Underlying Mantle Beneath Southeast Asia From Multi-Scale Adjoint Waveform Tomography, 2022, Journal of Geophysical Research Solid Earth
  • A Detailed Earthquake Catalog for Banda Arc-Australian Plate Collision Zone Using Machine-Learning Phase Picker and an Automated Workflow, 2022, The Seismic Record

Best Publications

  • Present-day motion of the Sierra Nevada block and some tectonic implications for the Basin and Range province, North American Cordillera

    Timothy H. Dixon;Meghan Miller;Frederic Farina;Hongzhi Wang

  • Kinematics of slab tear faults during subduction segmentation and implications for Italian magmatism

    Gideon Rosenbaum;Massimo Gasparon;Francesco P. Lucente;Angelo Peccerillo

  • Global quieting of high-frequency seismic noise due to COVID-19 pandemic lockdown measures.

    Thomas Lecocq;Stephen P. Hicks;Koen Van Noten;Kasper van Wijk

  • Continuing Colorado plateau uplift by delamination-style convective lithospheric downwelling

    A. Levander;B. Schmandt;M. S. Miller;K. Liu

  • Dynamics of continental accretion

    Louis-Noel Moresi;Peter Graham Betts;Meghan Samantha Miller;Ross A Cayley

  • Evolutionary aspects of lithosphere discontinuity structure in the western U.S.

    Alan Levander;Meghan S. Miller

  • Spatial and temporal evolution of the subducting Pacific plate structure along the western Pacific margin

    Meghan Miller;Brian Kennett;Virginia Toy;Virginia Toy

  • Three-dimensional numerical models of the influence of a buoyant oceanic plateau on subduction zones

    Wendy Mason;Louis-Noel Moresi;Peter Betts;M Miller

  • Isostasy, dynamic topography, and the elevation of the Apennines of Italy

    Claudio Faccenna;Thorsten W. Becker;Meghan S. Miller;Enrico Serpelloni

  • Crustal Structure of Active Deformation Zones in Africa: Implications for Global Crustal Processes

    Cynthia J Ebinger;Derek Keir;Derek Keir;Ian D Bastow;Kathryn A Whaler

  • New kinematic models for Pacific‐North America Motion from 3 Ma to Present, II: Evidence for a “Baja California Shear Zone”

    Timothy H. Dixon;Farina Farina;Charles DeMets;Francisco Suarez-Vidal

  • The geophysical signatures of the West African Craton

    Mark W. Jessell;Mark W. Jessell;Graham C. Begg;Meghan S. Miller

  • Formation of cratonic mantle keels by arc accretion: Evidence from S receiver functions

    Meghan S. Miller;David W. Eaton

  • Three-dimensional visualization of a near-vertical slab tear beneath the southern Mariana arc

    Meghan S. Miller;Alexei Gorbatov;Brian L. N. Kennett

  • Static and dynamic support of western United States topography

    Thorsten W. Becker;Claudio Faccenna;Eugene D. Humphreys;Anthony R. Lowry

  • Subduction-driven recycling of continental margin lithosphere

    A. Levander;Maximiliano Bezada;F. Niu;E. D. Humphreys

  • Heterogeneity within the subducting Pacific slab beneath the Izu-Bonin-Mariana arc: Evidence from tomography using 3D ray tracing inversion techniques

    Meghan Miller;A. Gorbatov;Brian Kennett

  • Imaging changes in morphology, geometry, and physical properties of the subducting Pacific plate along the Izu–Bonin–Mariana arc

    Meghan Samantha Miller;Meghan Samantha Miller;Brian Kennett;G S Lister

  • Seismic imaging of the Cocos plate subduction zone system in central Mexico

    YoungHee Kim;Meghan S. Miller;Frederick Pearce;Robert W. Clayton

  • Upper mantle structure beneath the Caribbean‐South American plate boundary from surface wave tomography

    Meghan S. Miller;Alan Levander;Fenglin Niu;Aibing Li

  • Isostasy, dynamic topography, and the elevation of the Apennines of Italy: insights into deformation of subducting lithosphere

    Claudio Faccenna;Thorsten Becker;Meghan Miller;Enrico Serpelloni

Frequent Co-Authors

Thorsten W. Becker
Thorsten W. Becker The University of Texas at Austin
Alan Levander
Alan Levander Rice University
Louis Moresi
Louis Moresi Australian National University
Peter G Betts
Peter G Betts Monash University
Fenglin Niu
Fenglin Niu Rice University
Eugene D. Humphreys
Eugene D. Humphreys University of Oregon
Louis-Noel Moresi
Louis-Noel Moresi University of Melbourne
Hrvoje Tkalčić
Hrvoje Tkalčić Australian National University
Claudio Faccenna
Claudio Faccenna Dresdner Grundwasserforschungszentrum
Brian Kennett
Brian Kennett Australian National University

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