M. H�non

1.0k citations
9 papers · 716 · h-index 8

Impact in

    • Astro and Planetary Science
    • Stellar, planetary, and galactic studies
    • Astrophysics and Star Formation Studies
    • Astrophysical Phenomena and Observations
    • Pulsars and Gravitational Waves Research
    • Gamma-ray bursts and supernovae

Papers in

M. H�non

9 papers receiving 666 citations

Peers

M. H�non
Comparison fields: 5 of 98
  • Astronomy and Astrophysics 493
  • Instrumentation 42
  • Statistical and Nonlinear Physics 145
  • Aerospace Engineering 199
  • Nuclear and High Energy Physics 54
Replace J. M. A. Danby with:
J. M. A. Danby United States
L. G. Taff United States
Giovanni F. Gronchi Italy
R. Broucke United States
Josep J. Masdemont Spain
Gerhard Scheifele Switzerland
Niels Oppermann Germany
Gérard Gómez Spain
William L. Burke United States
Balša Terzić United States
M. H�non relative to J. M. A. Danby United States J. M. A. Danby's profile →
Citations per field
00.5×7.3×
J. M. A. Danby · 1×
Citations per year

Countries citing papers authored by M. H�non

Since Specialization
Citations

This map shows the geographic impact of M. H�non's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by M. H�non with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. H�non more than expected).

Fields of papers citing papers by M. H�non

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by M. H�non. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by M. H�non. The network helps show where M. H�non may publish in the future.

Co-authors

The 1 scholars most cited alongside M. H�non, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with M. H�non Line = papers co-authored together M. H�non links everyone, so they are left out of the graph.

All Works

9 of 9 papers shown
#Work
1 1971301
2 198698
3 197192
4 197674
5 197373
6 197738
7 197721
8 199216
9 19773

About M. H�non

M. H�non is a scholar working on Statistical and Nonlinear Physics, Astronomy and Astrophysics, Aerospace Engineering, Geometry and Topology and Computer Networks and Communications, having authored 9 papers that have together received 716 indexed citations. Recurring topics across this work include Quantum chaos and dynamical systems (5 papers), Spacecraft Dynamics and Control (4 papers), Astro and Planetary Science (4 papers), Advanced Differential Equations and Dynamical Systems (3 papers), Stellar, planetary, and galactic studies (3 papers), Scientific Research and Discoveries (2 papers), Statistical Mechanics and Entropy (1 paper) and Advanced Data Storage Technologies (1 paper). The work is most often cited by research in Astronomy and Astrophysics (493 citations), Instrumentation (42 citations), Statistical and Nonlinear Physics (145 citations), Aerospace Engineering (199 citations) and Nuclear and High Energy Physics (54 citations). M. H�non has collaborated with scholars based in France and United States. Frequent co-authors include Jean-Marc Petit. Their work appears in journals such as Celestial Mechanics and Dynamical Astronomy, Journal of Statistical Physics and Astrophysics and Space Science.

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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