World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
128
Citations
46244
World Ranking
607
National Ranking
335

S. J. Bame publication distribution in Physics in 2026

The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where S. J. Bame sits on this spectrum.

103–122 publications: 7 scientists 123–142 publications: 10 scientists 143–162 publications: 31 scientists 163–182 publications: 35 scientists 183–202 publications: 53 scientists 203–222 publications: 81 scientists 223–242 publications: 85 scientists 243–262 publications: 112 scientists 263–282 publications: 114 scientists 283–302 publications: 126 scientists 303–322 publications: 136 scientists 323–342 publications: 162 scientists 343–362 publications: 155 scientists 363–382 publications: 156 scientists 383–402 publications: 134 scientists 403–422 publications: 145 scientists 423–442 publications: 147 scientists 443–462 publications: 131 scientists 463–482 publications: 131 scientists 483–502 publications: 116 scientists 503–522 publications: 106 scientists 523–542 publications: 103 scientists 543–562 publications: 87 scientists 563–582 publications: 84 scientists 583–602 publications: 94 scientists 603–622 publications: 70 scientists 623–642 publications: 76 scientists 643–662 publications: 60 scientists 663–682 publications: 54 scientists 683–702 publications: 60 scientists 703–722 publications: 48 scientists 723–742 publications: 64 scientists 743–762 publications: 48 scientists 763–782 publications: 37 scientists 783–802 publications: 43 scientists 803–822 publications: 34 scientists 823–842 publications: 36 scientists 843–862 publications: 32 scientists 863–882 publications: 32 scientists 883–902 publications: 31 scientists 903–922 publications: 25 scientists 923–942 publications: 15 scientists 943–962 publications: 24 scientists 963–982 publications: 13 scientists 983–1,002 publications: 21 scientists 1,003–1,022 publications: 21 scientists 1,023–1,042 publications: 16 scientists 1,043–1,062 publications: 9 scientists 1,063–1,082 publications: 19 scientists 1,083–1,102 publications: 11 scientists 1,103–1,122 publications: 17 scientists 1,123–1,142 publications: 11 scientists 1,143–1,162 publications: 7 scientists 1,163–1,182 publications: 4 scientists 1,183–1,202 publications: 10 scientists 1,203–1,222 publications: 8 scientists 1,223–1,242 publications: 16 scientists 1,243–1,262 publications: 4 scientists 1,263–1,282 publications: 10 scientists 1,283–1,302 publications: 5 scientists 1,303–1,322 publications: 7 scientists 1,323–1,342 publications: 4 scientists 1,343–1,362 publications: 8 scientists 1,363–1,382 publications: 6 scientists 1,383–1,402 publications: 7 scientists 1,403–1,422 publications: 3 scientists 1,423–1,442 publications: 4 scientists 1,443–1,462 publications: 4 scientists 1,463–1,468 publications: 3 scientists 1,469+ publications: 100 scientists
103 publications 1,469+

This scientist: 384 publications — 35th percentile

35% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 1,469 publications or more.

S. J. Bame D-index placement in Physics in 2026

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

70–71 D-Index: 76 scientists 72–73 D-Index: 110 scientists 74–75 D-Index: 143 scientists 76–77 D-Index: 153 scientists 78–79 D-Index: 144 scientists 80–81 D-Index: 167 scientists 82–83 D-Index: 167 scientists 84–85 D-Index: 166 scientists 86–87 D-Index: 132 scientists 88–89 D-Index: 155 scientists 90–91 D-Index: 134 scientists 92–93 D-Index: 137 scientists 94–95 D-Index: 102 scientists 96–97 D-Index: 112 scientists 98–99 D-Index: 110 scientists 100–101 D-Index: 116 scientists 102–103 D-Index: 97 scientists 104–105 D-Index: 103 scientists 106–107 D-Index: 87 scientists 108–109 D-Index: 90 scientists 110–111 D-Index: 67 scientists 112–113 D-Index: 78 scientists 114–115 D-Index: 75 scientists 116–117 D-Index: 67 scientists 118–119 D-Index: 69 scientists 120–121 D-Index: 60 scientists 122–123 D-Index: 59 scientists 124–125 D-Index: 53 scientists 126–127 D-Index: 42 scientists 128–129 D-Index: 41 scientists 130–131 D-Index: 33 scientists 132–133 D-Index: 32 scientists 134–135 D-Index: 45 scientists 136–137 D-Index: 19 scientists 138–139 D-Index: 24 scientists 140–141 D-Index: 28 scientists 142–143 D-Index: 31 scientists 144–145 D-Index: 22 scientists 146–147 D-Index: 20 scientists 148–149 D-Index: 12 scientists 150–151 D-Index: 16 scientists 152–153 D-Index: 24 scientists 154–155 D-Index: 23 scientists 156–157 D-Index: 15 scientists 158–159 D-Index: 15 scientists 160–161 D-Index: 11 scientists 162–163 D-Index: 17 scientists 164–165 D-Index: 12 scientists 166–167 D-Index: 11 scientists 168–169 D-Index: 9 scientists 170–171 D-Index: 9 scientists 172–173 D-Index: 11 scientists 174–175 D-Index: 4 scientists 176–177 D-Index: 8 scientists 178–179 D-Index: 5 scientists 180–181 D-Index: 3 scientists 182–183 D-Index: 4 scientists 184 D-Index: 4 scientists 185+ D-Index: 99 scientists
70 D-Index 185+

This scientist: 128 D-Index — 84th percentile

84% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 185 D-Index or more.

Research.com Recognitions

  • 1984 - Fellow of American Geophysical Union (AGU)
  • 1971 - Fellow of the American Association for the Advancement of Science (AAAS)
  • 1963 - Fellow of American Physical Society (APS)

Overview

S. J. Bame is affiliated with Los Alamos National Laboratory in the United States. Their professional record shows recognition by several notable scientific organizations over the course of their career.

They have been honored as a Fellow of the American Physical Society (APS) since 1963. Subsequently, they were elected Fellow of the American Association for the Advancement of Science (AAAS) in 1971. Later, in 1984, they were also named a Fellow of the American Geophysical Union (AGU).

The available record does not provide specific details regarding their research topics, publications, or their collaboration network. However, their connection to Los Alamos National Laboratory indicates involvement in scientific research likely of a technical or physical science nature.

There is no published information on recent papers, frequent co-authors, or venues where they have published. Similarly, no book publications or identified main fields or subfields of study are recorded in this data.

Despite the limited bibliographic information, the awards and fellowships reflect sustained participation and recognition within key scientific communities spanning physics, geophysics, and broad scientific advancement.

Best Publications

  • Solar Wind Electron Proton Alpha Monitor (SWEPAM) for the Advanced Composition Explorer

    D. J. McComas;S. J. Bame;P. Barker;W. C. Feldman

  • Evidence for magnetic field reconnection at the Earth's magnetopause

    B. U. Ö. Sonnerup;G. Paschmann;I. Papamastorakis;N. Sckopke

  • Geomagnetic activity associated with earth passage of interplanetary shock disturbances and coronal mass ejections

    J. T. Gosling;D. J. McComas;J. L. Phillips;S. J. Bame

  • Solar wind electrons

    W. C. Feldman;J. R. Asbridge;S. J. Bame;M. D. Montgomery

  • Plasma acceleration at the earth's magnetopause - Evidence for reconnection

    G. Paschmann;I. Papamastorakis;N. Sckopke;G. Haerendel

  • Outward flow of protons from the Earth's bow shock

    J. R. Asbridge;S. J. Bame;I. B. Strong

  • The magnetospheric boundary layer: Site of plasma, momentum and energy transfer from the magnetosheath into the magnetosphere

    T. E. Eastman;E. W. Hones;S. J. Bame;J. R. Asbridge

  • Bidirectional solar wind electron heat flux events

    J. T. Gosling;D. N. Baker;S. J. Bame;W. C. Feldman

  • Structure of the low‐latitude boundary layer

    N. Sckopke;G. Paschmann;G. Haerendel;B. U. Ö Sonnerup

  • Evolution of ion distributions across the nearly perpendicular bow shock: Specularly and non‐specularly reflected‐gyrating ions

    N. Sckopke;G. Paschmann;S. J. Bame;J. T. Gosling

  • Discovery of Jovian dust streams and interstellar grains by the Ulysses spacecraft

    E. Grün;H. A. Zook;M. Baguhl;A. Balogh

  • Electron velocity distributions near the Earth's bow shock

    W. C. Feldman;R. C. Anderson;S. J. Bame;S. P. Gary

  • Characteristics of the plasma sheet in the Earth's magnetotail

    S. J. Bame;J. R. Asbridge;H. E. Felthauser;E. W. Hones

  • Observations of two distinct populations of bow shock ions in the upstream solar wind

    J. T. Gosling;J. R. Asbridge;S. J. Bame;G. Paschmann

  • Lion roars and nonoscillatory drift mirror waves in the magnetosheath

    B. T. Tsurutani;E. J. Smith;R. R. Anderson;K. W. Ogilvie

  • Plasma and magnetic field characteristics of magnetic flux transfer events

    G. Paschmann;G. Haerendel;I. Papamastorakis;N. Sckopke

  • SOLAR WIND ELECTRONS: VELA 4 MEASUREMENTS.

    Michael D. Montgomery;S. J. Bame;A. J. Hundhausen

  • Measurements of magnetotail plasma flow made with Vela 4B

    E. W. Hones;J. R. Asbridge;S. J. Bame;M. D. Montgomery

  • Observations of reconnection of interplanetary and lobe magnetic field lines at the high‐latitude magnetopause

    J. T. Gosling;M. F. Thomsen;S. J. Bame;R. C. Elphic

  • Coronal streamers in the solar wind at 1 AU

    J. T. Gosling;G. Borrini;J. R. Asbridge;S. J. Bame

Frequent Co-Authors

J. T. Gosling
J. T. Gosling University of Colorado Boulder
J. R. Asbridge
J. R. Asbridge Los Alamos National Laboratory
David J. McComas
David J. McComas Princeton University
W. C. Feldman
W. C. Feldman Los Alamos National Laboratory
Edward J. Smith
Edward J. Smith California Institute of Technology
Michelle F. Thomsen
Michelle F. Thomsen Planetary Science Institute
Edward W. Hones
Edward W. Hones Los Alamos National Laboratory
Christopher T. Russell
Christopher T. Russell University of California, Los Angeles
G. Paschmann
G. Paschmann Max Planck Society
Daniel N. Baker
Daniel N. Baker University of Colorado Boulder

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