World's Best Scientists 2026 revealed!
Arnold O. Benz

Arnold O. Benz

D-Index & Metrics

Physics

D-Index
89
Citations
26383
World Ranking
2332
National Ranking
51

Arnold O. Benz 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 Arnold O. Benz 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: 424 publications — 42nd percentile

42% of scientists in this discipline score the same or lower.

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

Arnold O. Benz 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 Arnold O. Benz 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: 89 D-Index — 38th percentile

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

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

Overview

Arnold O. Benz is affiliated with ETH Zurich in Switzerland and has a research focus primarily within the field of Physics and Astronomy. Their work encompasses several subfields, including Astronomy and Astrophysics, Artificial Intelligence, Spectroscopy, Computational Mechanics, and Safety, Risk, Reliability and Quality.

The scientist's research covers a range of topics within space and astrophysical studies. Key areas include:

  • Solar and Space Plasma Dynamics
  • Astro and Planetary Science
  • Stellar, planetary, and galactic studies
  • Ionosphere and magnetosphere dynamics
  • Solar Radiation and Photovoltaics
  • Astrophysics and Star Formation Studies
  • Gamma-ray bursts and supernovae

Arnold O. Benz has been published across several frequent academic venues, emphasizing their research's focus. These venues include:

  • Astronomische Nachrichten
  • Astronomy and Astrophysics
  • The Astrophysical Journal
  • The Astrophysical Journal Letters
  • Springer Link (Chiba Institute of Technology)

Some recent publications exemplify the scope of their research:

  • The Spectrometer/Telescope for Imaging X-rays (STIX), 2020, Astronomy and Astrophysics
  • Water in star-forming regions: physics and chemistry from clouds to disks as probed by Herschel spectroscopy, 2021, Astronomy and Astrophysics
  • The Formation of Electron Outflow Jets with Power-law Energy Distribution in Guide-field Magnetic Reconnection, 2021, The Astrophysical Journal
  • Peculiar Radio-X-Ray Relationship in Active Stars, 2022, The Astrophysical Journal Letters
  • ALMA small-scale features in the quiet Sun and active regions, 2021, Springer Link (Chiba Institute of Technology)

Their collaborative efforts involve frequent co-authors across multiple publications. Notable collaborators include:

  • Säm Krucker
  • H. Che
  • G. P. Zank
  • Ivica Skokić
  • D. Sudar

Best Publications

  • The Reuven Ramaty High-Energy Solar Spectroscopic Imager (Rhessi)

    R. P. Lin;B. R. Dennis;G. J. Hurford;D. M. Smith

  • The Herschel-Heterodyne Instrument for the Far-Infrared (HIFI)

    Th. de Graauw;Th. de Graauw;F. P. Helmich;T. G. Phillips;J. Stutzki

  • On coronal oscillations

    B. Roberts;P. M. Edwin;A. O. Benz

  • Flare Observations

    Arnold O. Benz

  • RADIO EMISSION FROM SOLAR FLARES

    T. S. Bastian;A. O. Benz;Dale Gary

  • Plasma Astrophysics: Kinetic Processes in Solar and Stellar Coronae

    Arnold O. Benz

  • Water in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

    E. F. van Dishoeck;L. E. Kristensen;A. O. Benz;E. A. Bergin

  • Energy Distribution of Heating Processes in the Quiet Solar Corona

    Säm Krucker;Säm Krucker;Arnold O. Benz

  • X-ray/microwave relation of different types of active stars

    Manuel Guedel;Arnold O. Benz

  • Millisecond Radio Spikes

    A. O. Benz

  • Water in star-forming regions with the Herschel Space Observatory (WISH). I. Overview of key program and first results

    E. F. van Dishoeck;L. E. Kristensen;A. O. Benz;E. A. Bergin

  • Recent Advances in Understanding Particle Acceleration Processes in Solar Flares

    Valentina V. Zharkova;Karpar Arzner;Arnold O. Benz;Philippa Browning

  • Physical Processes in Magnetically Driven Flares on the Sun, Stars, and Young Stellar Objects

    Arnold O. Benz;Manuel Güdel

  • Herschel Survey of Galactic OH+, H2O+, and H3O+: Probing the Molecular Hydrogen Fraction and Cosmic-Ray Ionization Rate

    N. Indriolo;D.A. Neufeld;M. Gerin;P. Schilke

  • Water in star-forming regions with Herschel (WISH). II. Evolution of 557 GHz 110-101 emission in low-mass protostars

    L. E. Kristensen;E. F. Van Dishoeck;E. A. Bergin;R. Visser

  • Recent Advances in Understanding Particle Acceleration Processes in Solar Flares

    V. V. Zharkova;K. Arzner;A. O. Benz;P. Browning

  • Water in star forming regions with Herschel (WISH) III. Far-infrared cooling lines in low-mass young stellar objects

    A. Karska;G. J. Herczeg;E. F. van Dishoeck;S. F. Wampfler

  • Energy Distribution of Microevents in the Quiet Solar Corona

    Arnold O. Benz;Säm Krucker

  • Solar flare radio pulsations as a signature of dynamic magnetic reconnection

    B. Kliem;A.O. Benz;M. Karlicky

  • The Herschel-Heterodyne Instrument for the Far-Infrared (HIFI): instrument and pre-launch testing

    Thijs de Graauw;Thijs de Graauw;Nick Whyborn;Frank Helmich;Pieter Dieleman

Frequent Co-Authors

F. F. S. van der Tak
F. F. S. van der Tak Netherlands Institute for Space Research
E. F. van Dishoeck
E. F. van Dishoeck Leiden University
René Liseau
René Liseau Chalmers University of Technology
Javier R. Goicoechea
Javier R. Goicoechea Spanish National Research Council
Carsten Dominik
Carsten Dominik University of Amsterdam
Säm Krucker
Säm Krucker University of California, Berkeley
Brunella Nisini
Brunella Nisini National Institute for Astrophysics
Dariusz C. Lis
Dariusz C. Lis California Institute of Technology
Jes K. Jørgensen
Jes K. Jørgensen University of Copenhagen
David A. Neufeld
David A. Neufeld Johns Hopkins University

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