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 Hugh S. Hudson sits on this spectrum.
This scientist: 652 publications — 74th percentile
74% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 1,469 publications or more.
The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Hugh S. Hudson sits on this spectrum.
This scientist: 93 D-Index — 46th percentile
46% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
Hugh S. Hudson is affiliated with the University of Glasgow in the United Kingdom, with a research focus primarily in the domain of Physics and Astronomy. Their work spans several subfields, including Astronomy and Astrophysics, Nuclear and High Energy Physics, Oceanography, Atomic and Molecular Physics and Optics, as well as Atmospheric Science. Their research topics emphasize Solar and Space Plasma Dynamics, Astro and Planetary Science, Stellar, Planetary, and Galactic Studies, Ionosphere and Magnetosphere Dynamics, Gamma-ray Bursts and Supernovae, Astrophysics and Cosmic Phenomena, and Geophysics and Gravity Measurements.
Hudson has contributed to numerous publications and their frequent coauthors include L. Fletcher, I. G. Hannah, S. M. White, Säm Krucker, and Paulo J. A. Simões. Their research has been published repeatedly in venues such as arXiv (Cornell University), Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal, Solar Physics, and The Astrophysical Journal Letters.
Notable recent papers authored or coauthored by Hudson include:
Throughout their career, Hudson has been recognized as a Fellow of the American Physical Society (APS) in 1994, with a citation for observational and interpretational studies of solar processes, including energetic emissions during flares and time variations of solar irradiance.
R. P. Lin;B. R. Dennis;G. J. Hurford;D. M. Smith
Ronald L. Moore;Alphonse C. Sterling;Hugh S. Hudson;James R. Lemen
Lyndsay Fletcher;Brian R. Dennis;Hugh S. Hudson;Sam Krucker
L. Fletcher;B. R. Dennis;H. S. Hudson;S. Krucker
K. Hurley;S. E. Boggs;S. E. Boggs;D. M. Smith;R. C. Duncan
H. S. Hudson
Richard C. Canfield;Hugh S. Hudson;David E. McKenzie
R. P. Lin;H. S. Hudson
Alphonse C. Sterling;Hugh S. Hudson
R. P. Lin;S. Krucker;G. J. Hurford;D. M. Smith;D. M. Smith
Saku Tsuneta;Hirohisa Hara;Toshifumi Shimizu;Loren W. Acton
Richard C. Willson;Hugh S. Hudson
R. C. Willson;S. Gulkis;M. Janssen;H. S. Hudson
Masumi Shimojo;Shizuyo Hashimoto;Kazunari Shibata;Tadashi Hirayama
Säm Krucker;H. S. Hudson;L. Glesener;S. M. White;S. M. White
H. S. Hudson
D. E. McKenzie;H. S. Hudson
L. Fletcher;L. Fletcher;H. S. Hudson
R. P. Lin;H. S. Hudson
H. S. Hudson;T. W. Jones;R. P. Lin
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