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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Earth Science 55 2580 2349 1075 954 210 9988

Michael G. Henderson publications per year

The chart shows the history of publications by Michael G. Henderson between 1993 and 2026, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Michael G. Henderson published across 34 years, from 1993 to 2026, averaging 8.1 papers a year. Output peaked at 28 publications in 2013. 4 of the 275 publications appeared in the last two years.

No. of publications
5 10 15 20 25
Bar chart. Horizontal axis: year, 1993 to 2026. Vertical axis: number of publications, 0 to 28. Peak 28 publications in 2013. 1993: 2 publications 1994: 0 publications 1995: 2 publications 1996: 5 publications 1997: 3 publications 1998: 4 publications 1999: 1 publication 2000: 2 publications 2001: 7 publications 2002: 4 publications 2003: 5 publications 2004: 4 publications 2005: 4 publications 2006: 13 publications 2007: 13 publications 2008: 9 publications 2009: 5 publications 2010: 7 publications 2011: 1 publication 2012: 6 publications 2013: 28 publications 2014: 22 publications 2015: 10 publications 2016: 17 publications 2017: 13 publications 2018: 19 publications 2019: 11 publications 2020: 16 publications 2021: 10 publications 2022: 9 publications 2023: 15 publications 2024: 4 publications 2025: 2 publications 2026: 2 publications
1993 2026

275 publications in total across all disciplines

View publications per year as a table
Michael G. Henderson: publications per year, 1993 to 2026
Year Publications
1993 2
1994 0
1995 2
1996 5
1997 3
1998 4
1999 1
2000 2
2001 7
2002 4
2003 5
2004 4
2005 4
2006 13
2007 13
2008 9
2009 5
2010 7
2011 1
2012 6
2013 28
2014 22
2015 10
2016 17
2017 13
2018 19
2019 11
2020 16
2021 10
2022 9
2023 15
2024 4
2025 2
2026 2
Total 275
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Michael G. Henderson publications per year - data summary

  • Michael G. Henderson, a Earth Science scholar from Los Alamos National Laboratory, has 275 publications recorded across 34 years, from 1993 to 2026.
  • The oldest publication on record dates to 1993 and the most recent to 2026.
  • The most productive year is 2013, with 28 publications.
  • The least productive years with any output are 1999 and 2011, with 1 publication each.
  • 1 of the 34 years in the span carries no publications at all (1994).
  • The rate of publication averages 8.1 papers per year over the whole span, or 8.3 per year counting only the 33 years with at least one publication.
  • The last 5 years on the chart (2022-2026) hold 32 publications, 12% of the career total.
  • Split into equal eras - 1993-2004: 39 publications (3.3 per year); 2005-2016: 135 publications (11.3 per year); 2017-2026: 101 publications (10.1 per year).
  • Comparing the opening and closing eras, the overall trend of publication is rising.

Michael G. Henderson 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 Michael G. Henderson 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, 208–217 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: 210 publications — 67th percentile

67% 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
178–187 414
188–197 401
198–207 333
208–217 292 210
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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Michael G. Henderson publication distribution in Earth Science in 2026 - data summary

  • The chart plots the publication count of all 9,176 Earth Science scientists ranked by Research.com in 2026, grouped into 58 ranges running from 38–47 to 603+ publications.
  • Michael G. Henderson, a Earth Science scholar from Los Alamos National Laboratory, records 210 publications - the 67th percentile of the discipline.
  • 67% of ranked Earth Science scientists score the same or lower than Michael G. Henderson, and about 33% score higher.
  • The median of the discipline falls in the 168–177 publications range, and Michael G. Henderson ranks above the median.
  • The most crowded range is 128–137 publications, holding 557 scientists (6% of the field).
  • 58% of the field sits in the lowest quarter of the value range (up to 178–187 publications), so the distribution is heavily right-skewed and high scores are rare.
  • The final bar has no upper bound: it groups every scientist with 603 publications or more, 100 scientists in all (1% of the field).

Michael G. Henderson 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 Michael G. Henderson 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, 55 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: 55 D-Index — 73rd percentile

73% 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
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 55
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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Michael G. Henderson D-index placement in Earth Science in 2026 - data summary

  • The chart plots the discipline H-index (D-index) of all 9,176 Earth Science scientists ranked by Research.com in 2026, grouped into 77 ranges running from 30 to 106+ D-Index.
  • Michael G. Henderson, a Earth Science scholar from Los Alamos National Laboratory, records 55 D-Index - the 73rd percentile of the discipline.
  • 73% of ranked Earth Science scientists score the same or lower than Michael G. Henderson, and about 27% score higher.
  • The median of the discipline falls in the 44 D-Index range, and Michael G. Henderson ranks above the median.
  • The most crowded range is 36 D-Index, holding 389 scientists (4% of the field).
  • 62% of the field sits in the lowest quarter of the value range (up to 49 D-Index), so the distribution is heavily right-skewed and high scores are rare.
  • The final bar has no upper bound: it groups every scientist with 106 D-Index or more, 98 scientists in all (1% of the field).

Research.com Recognitions

  • 2016 - IEEE Fellow For contributions to the application of high-voltage DC and flexible AC transmission systems

Overview

Michael G. Henderson is a researcher affiliated with Los Alamos National Laboratory in the United States. Their work predominantly spans the fields of Physics and Astronomy as well as Earth and Planetary Sciences, with particular focus on subfields such as Astronomy and Astrophysics, Geophysics, Atmospheric Science, Molecular Biology, and Aerospace Engineering.

The scientist's research primarily addresses topics including:

  • Ionosphere and magnetosphere dynamics
  • Solar and Space Plasma Dynamics
  • Atmospheric Ozone and Climate
  • Geomagnetism and Paleomagnetism Studies
  • Earthquake Detection and Analysis
  • Astro and Planetary Science
  • Atmospheric and Environmental Gas Dynamics

Michael G. Henderson has contributed to several recent publications. Notable papers include:

  • "The impact of cold electrons and cold ions in magnetospheric physics," 2021, Journal of Atmospheric and Solar-Terrestrial Physics
  • "Physical Processes of Meso-Scale, Dynamic Auroral Forms," 2020, Space Science Reviews
  • "Solving the auroral-arc-generator question by using an electron beam to unambiguously connect critical magnetospheric measurements to auroral images," 2020, Journal of Atmospheric and Solar-Terrestrial Physics
  • "Why Are There so Few Reports of High-Energy Electron Drift Resonances? Role of Radial Phase Space Density Gradients," 2020, Journal of Geophysical Research Space Physics
  • "Episodic Occurrence of Field-Aligned Energetic Ions on the Dayside," 2020, Geophysical Research Letters

The frequent publication venues for Henderson include:

  • Journal of Geophysical Research Space Physics
  • Zenodo (CERN European Organization for Nuclear Research)
  • Journal of Atmospheric and Solar-Terrestrial Physics
  • Frontiers in Astronomy and Space Sciences
  • Geophysical Research Letters

Collaborations have been a significant part of their career, with regular co-authors being:

  • G. D. Reeves
  • Steven K. Morley
  • G. Cunningham
  • Gian Luca Delzanno
  • D. L. Turner

In 2016, Michael G. Henderson was recognized as an IEEE Fellow for contributions related to high-voltage DC and flexible AC transmission systems.

Best Publications

  • Rapid local acceleration of relativistic radiation-belt electrons by magnetospheric chorus

    R. M. Thorne;W Li;B Ni;Q. Ma

  • The Magnetic Electron Ion Spectrometer (MagEIS) Instruments Aboard the Radiation Belt Storm Probes (RBSP) Spacecraft

    J. B. Blake;P. A. Carranza;S. G. Claudepierre;J. H. Clemmons

  • Electron Acceleration in the Heart of the Van Allen Radiation Belts

    G. D. Reeves;Harlan E. Spence;M. G. Henderson;S. K. Morley

  • Helium, Oxygen, Proton, and Electron (HOPE) Mass Spectrometer for the Radiation Belt Storm Probes Mission

    H. O. Funsten;R. M. Skoug;A. A. Guthrie;E. A. MacDonald

  • Science Goals and Overview of the Radiation Belt Storm Probes (RBSP) Energetic Particle, Composition, and Thermal Plasma (ECT) Suite on NASA’s Van Allen Probes Mission

    H. E. Spence;G. D. Reeves;D. N. Baker;J. B. Blake

  • A long-lived relativistic electron storage ring embedded in Earth's outer Van Allen belt.

    D. N. Baker;S. G. Kanekal;V. C. Hoxie;M. G. Henderson

  • Geomagnetic storms driven by ICME- and CIR-dominated solar wind

    Michael H. Denton;Michael H. Denton;Joseph E. Borovsky;R. M. Skoug;M. F. Thomsen

  • Are north‐south aligned auroral structures an ionospheric manifestation of bursty bulk flows?

    M. G. Henderson;G. D. Reeves;J. S. Murphree

  • Coronal mass ejections, magnetic clouds, and relativistic magnetospheric electron events: ISTP

    D. N. Baker;T. I. Pulkkinen;X. Li;S. G. Kanekal

  • On the relationship between relativistic electron flux and solar wind velocity: Paulikas and Blake revisited

    Geoffrey D. Reeves;Steven K. Morley;Reiner H. W. Friedel;Michael G. Henderson

  • Evolution and slow decay of an unusual narrow ring of relativistic electrons near L~3.2 following the September 2012 magnetic storm

    R. M. Thorne;W. Li;B. Ni;Q. Ma

  • Cassini plasma spectrometer thermal ion measurements in Saturn's inner magnetosphere

    R. J. Wilson;R. L. Tokar;M. G. Henderson;T. W. Hill

  • Gradual diffusion and punctuated phase space density enhancements of highly relativistic electrons: Van Allen Probes observations

    D. N. Baker;A. Jaynes;X. Li;M. G. Henderson

  • Van Allen Probes observation of localized drift resonance between poloidal mode ultra‐low frequency waves and 60 keV electrons

    S. G. Claudepierre;I. R. Mann;K. Takahashi;J. F. Fennell

  • Modeling radiation belt electron dynamics during GEM challenge intervals with the DREAM3D diffusion model

    Weichao Tu;G.S. Cunningham;Y. Chen;M.G. Henderson

  • The relativistic electron response at geosynchronous orbit during the January 1997 magnetic storm

    G. D. Reeves;R. H. W. Friedel;R. D. Belian;M. M. Meier

  • Magnetospheric and auroral activity during the 18 April 2002 sawtooth event

    M. G. Henderson;G. D. Reeves;R. Skoug;M .F. Thomsen

  • Radial propagation of substorm injections

    G. D. Reeves;M. G. Henderson;P. S. McLachlan;R. D. Belian

  • Competing source and loss mechanisms due to wave-particle interactions in Earth's outer radiation belt during the 30 September to 3 October 2012 geomagnetic storm

    D. L. Turner;V. Angelopoulos;W. Li;J. Bortnik

  • On the cause and extent of outer radiation belt losses during the 30 September 2012 dropout event

    D. L. Turner;V. Angelopoulos;S. K. Morley;M. G. Henderson

  • First energetic neutral atom images from Polar

    M. G. Henderson;G. D. Reeves;Harlan E. Spence;R. B. Sheldon

Frequent Co-Authors

Geoffrey D. Reeves
Geoffrey D. Reeves Los Alamos National Laboratory
Harlan E. Spence
Harlan E. Spence University of New Hampshire
Michael H. Denton
Michael H. Denton Space Science Institute
Michelle F. Thomsen
Michelle F. Thomsen Planetary Science Institute
Daniel N. Baker
Daniel N. Baker University of Colorado Boulder
Craig Kletzing
Craig Kletzing University of Iowa
Vania K. Jordanova
Vania K. Jordanova Los Alamos National Laboratory
J. B. Blake
J. B. Blake The Aerospace Corporation
William S. Kurth
William S. Kurth University of Iowa
Drew L. Turner
Drew L. Turner Johns Hopkins University Applied Physics Laboratory

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