G. Belmont

2.8k total citations
74 papers, 2.0k citations indexed

About

G. Belmont is a scholar working on Astronomy and Astrophysics, Molecular Biology and Nuclear and High Energy Physics. According to data from OpenAlex, G. Belmont has authored 74 papers receiving a total of 2.0k indexed citations (citations by other indexed papers that have themselves been cited), including 68 papers in Astronomy and Astrophysics, 29 papers in Molecular Biology and 13 papers in Nuclear and High Energy Physics. Recurrent topics in G. Belmont's work include Ionosphere and magnetosphere dynamics (65 papers), Solar and Space Plasma Dynamics (56 papers) and Geomagnetism and Paleomagnetism Studies (29 papers). G. Belmont is often cited by papers focused on Ionosphere and magnetosphere dynamics (65 papers), Solar and Space Plasma Dynamics (56 papers) and Geomagnetism and Paleomagnetism Studies (29 papers). G. Belmont collaborates with scholars based in France, United States and United Kingdom. G. Belmont's co-authors include L. Rezeau, P. Canu, F. Sahraoui, M. L. Goldstein, N. Cornilleau‐Wehrlin, N. Aunai, C. Lacombe, R. Smets, J. L. Pinçon and A. Balogh and has published in prestigious journals such as Physical Review Letters, Journal of Geophysical Research Atmospheres and The Astrophysical Journal.

In The Last Decade

G. Belmont

74 papers receiving 1.8k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
G. Belmont France 26 1.9k 830 364 187 102 74 2.0k
J. Dorelli United States 27 1.7k 0.9× 592 0.7× 326 0.9× 256 1.4× 75 0.7× 85 1.8k
F. Sahraoui France 31 2.4k 1.2× 1.1k 1.3× 272 0.7× 189 1.0× 50 0.5× 72 2.5k
D. Sundkvist United States 14 1.4k 0.7× 484 0.6× 316 0.9× 113 0.6× 82 0.8× 26 1.5k
S. Eriksson United States 27 1.8k 0.9× 759 0.9× 190 0.5× 256 1.4× 110 1.1× 97 1.8k
P. Canu France 27 2.5k 1.3× 991 1.2× 213 0.6× 396 2.1× 149 1.5× 93 2.6k
F. Pantellini United States 19 1.6k 0.8× 395 0.5× 199 0.5× 86 0.5× 90 0.9× 168 1.6k
G. G. Howes United States 26 2.6k 1.3× 755 0.9× 808 2.2× 59 0.3× 78 0.8× 76 2.7k
K. H. Glaßmeier Germany 24 2.1k 1.1× 1.2k 1.4× 136 0.4× 399 2.1× 64 0.6× 61 2.2k
A. N. McClymont United States 23 1.9k 1.0× 545 0.7× 267 0.7× 65 0.3× 61 0.6× 58 2.1k
K. Murawski Poland 25 1.8k 0.9× 619 0.7× 146 0.4× 65 0.3× 62 0.6× 164 2.0k

Countries citing papers authored by G. Belmont

Since Specialization
Citations

This map shows the geographic impact of G. Belmont'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 G. Belmont with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. Belmont more than expected).

Fields of papers citing papers by G. Belmont

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by G. Belmont. 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 G. Belmont. The network helps show where G. Belmont may publish in the future.

Co-authorship network of co-authors of G. Belmont

This figure shows the co-authorship network connecting the top 25 collaborators of G. Belmont. A scholar is included among the top collaborators of G. Belmont based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with G. Belmont. G. Belmont is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Denton, R. E., R. B. Torbert, Hiroshi Hasegawa, et al.. (2021). Two‐Dimensional Velocity of the Magnetic Structure Observed on July 11, 2017 by the Magnetospheric Multiscale Spacecraft. Journal of Geophysical Research Space Physics. 126(3). 4 indexed citations
2.
Califano, F., et al.. (2020). A multi-fluid model of the magnetopause. Annales Geophysicae. 38(2). 275–286. 2 indexed citations
3.
Belmont, G., et al.. (2019). Crossing of Plasma Structures by Spacecraft: A Path Calculator. Journal of Geophysical Research Space Physics. 124(12). 10119–10140. 4 indexed citations
4.
Rezeau, L. & G. Belmont. (2018). Reconnexion magnétique entre le vent solaire et la magnétosphère terrestre : la mission MMS. HAL (Le Centre pour la Communication Scientifique Directe). 20–25. 2 indexed citations
5.
Rezeau, L., et al.. (2017). Analyzing the Magnetopause Internal Structure: New Possibilities Offered by MMS Tested in a Case Study. Journal of Geophysical Research Space Physics. 123(1). 227–241. 9 indexed citations
6.
Smets, R., N. Aunai, G. Belmont, C. Boniface, & J. Fuchs. (2014). On the relationship between quadrupolar magnetic field and collisionless reconnection. Physics of Plasmas. 21(6). 6 indexed citations
7.
Aunai, N., G. Belmont, & R. Smets. (2013). First demonstration of an asymmetric kinetic equilibrium for a thin current sheet. Physics of Plasmas. 20(11). 7 indexed citations
8.
Sahraoui, F., et al.. (2011). Observation and theoretical modeling of electron scale solar wind turbulence. Comptes Rendus Physique. 12(2). 132–140. 5 indexed citations
9.
Aunai, N., G. Belmont, & R. Smets. (2011). Energy budgets in collisionless magnetic reconnection: Ion heating and bulk acceleration. Physics of Plasmas. 18(12). 31 indexed citations
10.
Sahraoui, F., M. L. Goldstein, G. Belmont, P. Canu, & L. Rezeau. (2010). Three dimensional anisotropic k-spectra of turbulence at sub-proton scales in the solar wind. AGUFM. 2010. 14 indexed citations
11.
Goldstein, M. L., et al.. (2010). Three Dimensional AnisotropickSpectra of Turbulence at Subproton Scales in the Solar Wind. Physical Review Letters. 105(13). 131101–131101. 308 indexed citations
12.
Sahraoui, F., G. Belmont, A. Roux, et al.. (2010). Multi-spacecraft investigation of space turbulence: Lessons from Cluster and input to the Cross-Scale mission. Planetary and Space Science. 59(7). 585–591. 8 indexed citations
13.
Sahraoui, F., G. Belmont, L. Rezeau, et al.. (2006). Anisotropic Turbulent Spectra in the Terrestrial Magnetosheath as Seen by the Cluster Spacecraft. Physical Review Letters. 96(7). 75002–75002. 160 indexed citations
14.
Sahraoui, F., Jean‐Louis Pinçon, G. Belmont, et al.. (2003). ULF wave identification in the magnetosheath: The k‐filtering technique applied to Cluster II data. Journal of Geophysical Research Atmospheres. 108(A9). 90 indexed citations
15.
Rezeau, L., F. Sahraoui, E. d’Humières, et al.. (2001). A case study of low-frequency waves at the magnetopause. Annales Geophysicae. 19(10/12). 1463–1470. 14 indexed citations
16.
Delcourt, Dominique & G. Belmont. (1998). Ion dynamics at the earthward termination of the magnetotail current sheet. Journal of Geophysical Research Atmospheres. 103(A3). 4605–4613. 17 indexed citations
17.
Mazelle, C. & G. Belmont. (1993). Determination of electron polytropic indices in the environment of comet P/Halley. Geophysical Research Letters. 20(2). 157–160. 9 indexed citations
18.
Lacombe, C., F. Pantellini, D. Hubert, et al.. (1992). Mirror and Alfvénic waves observed by ISEE 1-2 during crossings of the Earth's bow shock. Annales Geophysicae. 10(10). 772–784. 80 indexed citations
19.
Belmont, G., D. Hubert, C. Lacombe, & F. Pantellini. (1992). Mirror mode and other compressive ULF modes.. ESASP. 346. 263–267. 6 indexed citations
20.
Etcheto, J., G. Belmont, P. Canu, & J. G. Trotignon. (1983). Active sounder experiments on GEOS and ISEE. ESA Special Publication. 195. 39–46. 15 indexed citations

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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