H. Ardavan

440 total citations
41 papers, 272 citations indexed

About

H. Ardavan is a scholar working on Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics and Nuclear and High Energy Physics. According to data from OpenAlex, H. Ardavan has authored 41 papers receiving a total of 272 indexed citations (citations by other indexed papers that have themselves been cited), including 19 papers in Astronomy and Astrophysics, 19 papers in Atomic and Molecular Physics, and Optics and 11 papers in Nuclear and High Energy Physics. Recurrent topics in H. Ardavan's work include Pulsars and Gravitational Waves Research (15 papers), Orbital Angular Momentum in Optics (15 papers) and Cold Atom Physics and Bose-Einstein Condensates (6 papers). H. Ardavan is often cited by papers focused on Pulsars and Gravitational Waves Research (15 papers), Orbital Angular Momentum in Optics (15 papers) and Cold Atom Physics and Bose-Einstein Condensates (6 papers). H. Ardavan collaborates with scholars based in United Kingdom, United States and Russia. H. Ardavan's co-authors include John Singleton, Arzhang Ardavan, M. Hossein Partovi, Dorothy Halliday, W. Hayes and J. Fopma and has published in prestigious journals such as Nature, Journal of Applied Physics and The Astrophysical Journal.

In The Last Decade

H. Ardavan

39 papers receiving 249 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
H. Ardavan United Kingdom 11 124 123 103 40 36 41 272
W. Junker Germany 7 158 1.3× 31 0.3× 251 2.4× 50 1.3× 36 1.0× 7 361
D Tombolato Italy 9 144 1.2× 96 0.8× 19 0.2× 18 0.5× 23 0.6× 13 230
P. Bernard Switzerland 9 132 1.1× 60 0.5× 68 0.7× 29 0.7× 93 2.6× 27 284
V. B. Braginsky Russia 9 146 1.2× 98 0.8× 61 0.6× 16 0.4× 9 0.3× 19 226
Mitsuhiro Fukushima Japan 9 184 1.5× 92 0.7× 71 0.7× 16 0.4× 7 0.2× 21 235
D. M. Gould United Kingdom 5 385 3.1× 43 0.3× 157 1.5× 20 0.5× 23 0.6× 9 412
I. Bailey United Kingdom 6 152 1.2× 31 0.3× 114 1.1× 29 0.7× 32 0.9× 26 209
K. Tsubono Japan 9 150 1.2× 99 0.8× 29 0.3× 19 0.5× 10 0.3× 25 221
Marc Ollivier France 8 110 0.9× 106 0.9× 21 0.2× 41 1.0× 37 1.0× 28 226
K. Westpfahl Germany 8 273 2.2× 82 0.7× 150 1.5× 12 0.3× 11 0.3× 27 345

Countries citing papers authored by H. Ardavan

Since Specialization
Citations

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

Fields of papers citing papers by H. Ardavan

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of H. Ardavan

This figure shows the co-authorship network connecting the top 25 collaborators of H. Ardavan. A scholar is included among the top collaborators of H. Ardavan 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 H. Ardavan. H. Ardavan 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.
Ardavan, H.. (2024). Gamma-ray spectra of the Crab, Vela and Geminga pulsars fitted with SED of the emission from their current sheet. Journal of Cosmology and Astroparticle Physics. 2024(5). 67–67. 1 indexed citations
2.
Ardavan, H.. (2023). Congruity of the Crab Pulsar’s γ-ray spectrum with the spectral distribution of tightly focused caustics. Astronomy and Astrophysics. 672. A154–A154. 3 indexed citations
3.
Ardavan, H.. (2021). Radiation by the superluminally moving current sheet in the magnetosphere of a neutron star. Monthly Notices of the Royal Astronomical Society. 507(3). 4530–4563. 6 indexed citations
4.
Ardavan, H., et al.. (2009). Fundamental role of the retarded potential in the electrodynamics of superluminal sources: reply to comment. Journal of the Optical Society of America A. 26(10). 2109–2109. 1 indexed citations
5.
Ardavan, H., et al.. (2008). Fundamental role of the retarded potential in the electrodynamics of superluminal sources. Journal of the Optical Society of America A. 25(3). 543–543. 4 indexed citations
6.
Ardavan, H., et al.. (2008). Spectral properties of the nonspherically decaying radiation generated by a rotating superluminal source. Journal of the Optical Society of America A. 25(3). 780–780. 2 indexed citations
7.
Ardavan, H., et al.. (2007). Morphology of the nonspherically decaying radiation beam generated by a rotating superluminal source. Journal of the Optical Society of America A. 24(8). 2443–2443. 7 indexed citations
8.
Ardavan, H., Arzhang Ardavan, & John Singleton. (2004). Spectral and polarization characteristics of the nonspherically decaying radiation generated by polarization currents with superluminally rotating distribution patterns. Journal of the Optical Society of America A. 21(5). 858–858. 14 indexed citations
9.
Ardavan, H., et al.. (2003). Frequency spectrum of focused broadband pulses of electromagnetic radiation generated by polarization currents with superluminally rotating distribution patterns. Journal of the Optical Society of America A. 20(11). 2137–2137. 11 indexed citations
10.
Ardavan, H.. (1999). Method of handling the divergences in the radiation theory of sources that move faster than their waves. Journal of Mathematical Physics. 40(9). 4331–4336. 9 indexed citations
11.
Ardavan, H.. (1995). Splitting of the Alfven surface in a relativistic pulsar wind. Monthly Notices of the Royal Astronomical Society. 273(4). 1129–1132.
12.
Ardavan, H.. (1991). The near-field singularity predicted by the spiral Green’s function in acoustics and electrodynamics. Proceedings of the Royal Society of London Series A Mathematical and Physical Sciences. 433(1888). 451–459. 9 indexed citations
13.
Ardavan, H.. (1991). The breakdown of the linearized theory and the role of quadrupole sources in transonic rotor acoustics. Journal of Fluid Mechanics. 226. 591–624. 12 indexed citations
14.
Ardavan, H.. (1989). The speed-of-light catastrophe. Proceedings of the Royal Society of London A Mathematical and Physical Sciences. 424(1866). 113–141. 12 indexed citations
15.
Ardavan, H.. (1984). A singularity arising from the coherent generation of gravitational waves by electromagnetic waves.. 5–14. 2 indexed citations
16.
Ardavan, H.. (1981). Is the light cylinder the site of emission in pulsars?. Nature. 289(5793). 44–45. 6 indexed citations
17.
Ardavan, H.. (1979). The stellar-wind model of pulsar magnetospheres. Monthly Notices of the Royal Astronomical Society. 189(3). 397–412. 9 indexed citations
18.
Ardavan, H. & M. Hossein Partovi. (1977). Magnetic support against gravitational collapse: A static axisymmetric interior solution of the Einstein-Maxwell equations. Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields. 16(6). 1664–1677. 15 indexed citations
19.
Ardavan, H.. (1976). Quasi-Steady Pulsar Magnetospheres. Monthly Notices of the Royal Astronomical Society. 177(3). 661–672. 2 indexed citations
20.
Ardavan, H.. (1973). Dynamical Evolution of an Expanding Gas Cloud. The Astrophysical Journal. 184. 435–435. 3 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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