World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
99
Citations
40572
World Ranking
1699
National Ranking
893

John C. Raymond 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 John C. Raymond 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: 935 publications — 90th percentile

90% of scientists in this discipline score the same or lower.

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

John C. Raymond 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 John C. Raymond 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: 99 D-Index — 55th percentile

55% 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

  • 2017 - Fellow of American Geophysical Union (AGU)
  • 2009 - Fellow of American Physical Society (APS) Citation For his outstanding contributions to the understanding of a broad range of astrophysical processes in the solar corona, supernova remnants, Xray binaries, and other objects
  • 1997 - Fellow of the American Association for the Advancement of Science (AAAS)

Overview

John C. Raymond is affiliated with Harvard University in the United States and has contributed extensively to the field of Physics and Astronomy. Their academic output spans 264 publications, with a particular focus on Astronomy and Astrophysics, which accounts for 211 of these works. Other notable subfields include Nuclear and High Energy Physics, Atomic and Molecular Physics and Optics, General Health Professions, and Instrumentation.

The main research topics addressed by John C. Raymond encompass a diverse array of subjects:

  • Gamma-ray bursts and supernovae
  • Astrophysics and Cosmic Phenomena
  • Solar and Space Plasma Dynamics
  • Astrophysical Phenomena and Observations
  • Stellar, planetary, and galactic studies
  • Astro and Planetary Science
  • Pulsars and Gravitational Waves Research

Among the more recent publications, the following are noteworthy for their scope and impact:

  • The origin of Galactic cosmic rays as revealed by their composition, 2021, Monthly Notices of the Royal Astronomical Society
  • An Obscured, Seyfert 2-like State of the Stellar-mass Black Hole GRS 1915+105 Caused by Failed Disk Winds, 2020, The Astrophysical Journal
  • Line Emission Mapper (LEM): Probing the physics of cosmic ecosystems, 2022, arXiv (Cornell University)
  • Defining the Middle Corona, 2023, Solar Physics
  • The Role of Turbulence for Heating Plasmas in Eruptive Solar Flares, 2020, The Astrophysical Journal

Frequent co-authors in their work include:

  • D. Milisavljević
  • J. M. Mïller
  • Yeimy J. Rivera
  • Robert A. Fesen
  • Abderahmen Zoghbi

John C. Raymond's research has appeared in a variety of publication venues, with the highest number of papers published in:

  • The Astrophysical Journal
  • arXiv (Cornell University)
  • The Astrophysical Journal Letters
  • Monthly Notices of the Royal Astronomical Society
  • Frontiers in Astronomy and Space Sciences

Throughout their career, John C. Raymond has been recognized by several professional organizations. They were named a Fellow of the American Geophysical Union (AGU) in 2017. In 2009, they were elected Fellow of the American Physical Society (APS) for their contributions to understanding a broad range of astrophysical processes in the solar corona, supernova remnants, X-ray binaries, and other objects. Additionally, they were named Fellow of the American Association for the Advancement of Science (AAAS) in 1997.

Best Publications

  • Collisional Plasma Models with APEC/APED: Emission-Line Diagnostics of Hydrogen-like and Helium-like Ions

    Randall K. Smith;Nancy S. Brickhouse;Duane A. Liedahl;John C. Raymond

  • Soft X-ray spectrum of a hot plasma.

    John C. Raymond;Barham W. Smith

  • Radiative Bow Shock Models of Herbig-Haro Objects

    Patrick Hartigan;John Raymond;Lee Hartmann

  • The Ultraviolet Coronagraph Spectrometer for the Solar and Heliospheric Observatory

    J. L. Kohl;R. Esser;L. D. Gardner;S. Habbal

  • UVCS/SOHO Empirical Determinations of Anisotropic Velocity Distributions in the Solar Corona

    J. L. Kohl;G. Noci;E. Antonucci;G. Tondello

  • First Results from the SOHO Ultraviolet Coronagraph Spectrometer

    J. L. Kohl;G. Noci;E. Antonucci;G. Tondello

  • UBVRI Light Curves of 44 Type Ia Supernovae

    Saurabh Jha;Saurabh Jha;Robert P. Kirshner;Peter Challis;Peter M. Garnavich

  • An Empirical Model of a Polar Coronal Hole at Solar Minimum

    S. R. Cranmer;J. L. Kohl;G. Noci;E. Antonucci

  • The optical emission from a fast shock wave with application to supernova remnants.

    R. A. Chevalier;R. P. Kirshner;J. C. Raymond

  • Mass-loss rates, ionization fractions, shock velocities, and magnetic fields of stellar jets

    Patrick Hartigan;Jon A. Morse;John Raymond

  • The Expansion Asymmetry and Age of the Cassiopeia A Supernova Remnant

    R. A. Fesen;M. C. Hammell;J. Morse;R. A. Chevalier

  • Direct Observations of the Magnetic Reconnection Site of an Eruption on 2003 November 18

    J Lin;YK Ko;L Sui;JC Raymond

  • The Expansion Asymmetry and Age of the Cassiopeia A Supernova Remnant

    Robert A. Fesen;Molly C. Hammell;Jon Morse;Roger A. Chevalier

  • Dynamical and Physical Properties of a Post-Coronal Mass Ejection Current Sheet

    Yuan-Kuen Ko;John C. Raymond;Jun Lin;Gareth Lawrence

  • Optical emission from a fast shock wave - The remnants of Tycho's supernova and SN 1006

    R. A. Chevalier;J. C. Raymond

  • Ultraviolet spectroscopy of the extended solar corona

    John L. Kohl;Giancarlo Noci;Steven R. Cranmer;John C. Raymond

  • The magnetic nature of disk accretion onto black holes

    Jon M. Miller;John Raymond;Andy Fabian;Danny Steeghs

  • Balmer-dominated Spectra of Nonradiative Shocks in the Cygnus Loop, RCW 86, and Tycho Supernova Remnants

    Parviz Ghavamian;Parviz Ghavamian;Parviz Ghavamian;John Raymond;R. Chris Smith;Patrick Hartigan

  • X-ray emission from cataclysmic variables with accretion disks. I - Hard X-rays. II - EUV/soft X-ray radiation

    J. Patterson;J. C. Raymond

  • Plasma Properties in Coronal Holes Derived from Measurements of Minor Ion Spectral Lines and Polarized White Light Intensity

    Ruth Esser;Silvano Fineschi;Danuta Dobrzycka;Shadia R. Habbal

Frequent Co-Authors

William P. Blair
William P. Blair Johns Hopkins University
Lee Hartmann
Lee Hartmann University of Michigan–Ann Arbor
Knox S. Long
Knox S. Long Space Telescope Science Institute
Andrea K. Dupree
Andrea K. Dupree Harvard University
Jon M. Miller
Jon M. Miller University of Michigan–Ann Arbor
John H. Black
John H. Black Chalmers University of Technology
A. C. Fabian
A. C. Fabian University of Cambridge
Angelos Vourlidas
Angelos Vourlidas Johns Hopkins University Applied Physics Laboratory
Roger J. Davis
Roger J. Davis University of Massachusetts Chan Medical School
Robert P. Kirshner
Robert P. Kirshner Harvard University

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