I. W. Roxburgh

5.7k total citations · 1 hit paper
130 papers, 2.2k citations indexed

About

I. W. Roxburgh is a scholar working on Astronomy and Astrophysics, Oceanography and Instrumentation. According to data from OpenAlex, I. W. Roxburgh has authored 130 papers receiving a total of 2.2k indexed citations (citations by other indexed papers that have themselves been cited), including 110 papers in Astronomy and Astrophysics, 23 papers in Oceanography and 23 papers in Instrumentation. Recurrent topics in I. W. Roxburgh's work include Stellar, planetary, and galactic studies (63 papers), Solar and Space Plasma Dynamics (52 papers) and Astro and Planetary Science (30 papers). I. W. Roxburgh is often cited by papers focused on Stellar, planetary, and galactic studies (63 papers), Solar and Space Plasma Dynamics (52 papers) and Astro and Planetary Science (30 papers). I. W. Roxburgh collaborates with scholars based in United Kingdom, France and United States. I. W. Roxburgh's co-authors include С. В. Воронцов, B. R. Durney, David S. De Young, J. J. Monaghan, J. Latham, P. A. Strittmatter, R. Samadi, J. S. Faulkner, R. F. Stein and Åke Nordlund and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

I. W. Roxburgh

124 papers receiving 2.1k citations

Hit Papers

Homogeneous Relativistic Cosmologies 1975 2026 1992 2009 1975 100 200 300

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
I. W. Roxburgh United Kingdom 23 2.0k 413 412 311 183 130 2.2k
H. M. Antia India 29 2.4k 1.2× 365 0.9× 221 0.5× 70 0.2× 153 0.8× 132 2.7k
Alfred Weigert Germany 4 1.6k 0.8× 400 1.0× 255 0.6× 84 0.3× 109 0.6× 20 1.8k
M. G. Lattanzi Italy 22 2.1k 1.1× 217 0.5× 922 2.2× 116 0.4× 132 0.7× 192 2.3k
Seppo Mikkola Finland 33 2.9k 1.5× 366 0.9× 305 0.7× 397 1.3× 54 0.3× 120 3.2k
P. P. Kronberg Canada 28 3.3k 1.6× 2.3k 5.6× 136 0.3× 113 0.4× 150 0.8× 91 3.6k
Daiichiro Sugimoto Japan 15 771 0.4× 210 0.5× 157 0.4× 198 0.6× 29 0.2× 76 1.1k
A. Bonanno Italy 29 2.6k 1.3× 1.9k 4.7× 159 0.4× 855 2.7× 109 0.6× 133 3.0k
M. R. Calabretta Australia 16 1.8k 0.9× 581 1.4× 244 0.6× 44 0.1× 48 0.3× 40 2.0k
G. Bertin Italy 27 2.0k 1.0× 390 0.9× 595 1.4× 215 0.7× 17 0.1× 111 2.2k
R. Beck Germany 42 5.6k 2.8× 2.7k 6.6× 350 0.8× 162 0.5× 105 0.6× 231 5.9k

Countries citing papers authored by I. W. Roxburgh

Since Specialization
Citations

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

Fields of papers citing papers by I. W. Roxburgh

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by I. W. Roxburgh. 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 I. W. Roxburgh. The network helps show where I. W. Roxburgh may publish in the future.

Co-authorship network of co-authors of I. W. Roxburgh

This figure shows the co-authorship network connecting the top 25 collaborators of I. W. Roxburgh. A scholar is included among the top collaborators of I. W. Roxburgh 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 I. W. Roxburgh. I. W. Roxburgh 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.
Ong, J. M. Joel, et al.. (2025). Resolving an Asteroseismic Catastrophe: Structural Diagnostics from p-mode Phase Functions off the Main Sequence. The Astrophysical Journal. 980(2). 199–199. 1 indexed citations
2.
Nielsen, M. B., G. R. Davies, Warrick H. Ball, et al.. (2021). PBjam: A Python Package for Automating Asteroseismology of Solar-like Oscillators*. The Astronomical Journal. 161(2). 62–62. 27 indexed citations
3.
Ong, J. M. Joel, Sarbani Basu, & I. W. Roxburgh. (2021). Mixed Modes and Asteroseismic Surface Effects. I. Analytic Treatment. The Astrophysical Journal. 920(1). 8–8. 13 indexed citations
4.
Roxburgh, I. W.. (2015). Surface layer independent model fitting by phase matching: theory and application to HD 49933 and HD 177153 (aka Perky). Springer Link (Chiba Institute of Technology). 16 indexed citations
5.
Roxburgh, I. W.. (2015). Scaled models, scaled frequencies, and model fitting. Astronomy and Astrophysics. 584. A71–A71.
6.
Roxburgh, I. W.. (2014). On the use of the average large separation in surface layer independent model fitting and mass estimation. Springer Link (Chiba Institute of Technology). 3 indexed citations
7.
Roxburgh, I. W. & С. В. Воронцов. (2013). On the use of the ratio of small to large separations in asteroseismic model fitting. Springer Link (Chiba Institute of Technology). 11 indexed citations
8.
Catala, C., T. Arentoft, M. Fridlund, et al.. (2010). PLATO: PLAnetary Transits and Oscillations of Stars The exoplanetary system explorer. elib (German Aerospace Center). 430. 15523. 4 indexed citations
9.
Roxburgh, I. W. & С. В. Воронцов. (2007). Acoustic wave reflection by stellar cores: can it be seen in the autocorrelation function of p-mode measurements?. Monthly Notices of the Royal Astronomical Society. 379(2). 801–806. 9 indexed citations
10.
Roxburgh, I. W.. (2005). The ratio of small to large separations of stellar p-modes. Astronomy and Astrophysics. 434(2). 665–669. 32 indexed citations
11.
Roxburgh, I. W. & С. В. Воронцов. (1999). Asteroseismological Constraints on Stellar Convective Cores. ASPC. 173. 257. 1 indexed citations
12.
Roxburgh, I. W. & С. В. Воронцов. (1997). ON THE FORMATION OF SPECTRAL LINE PROFILES OF SOLAR P MODES. Monthly Notices of the Royal Astronomical Society. 292(1). 2 indexed citations
13.
Roxburgh, I. W.. (1996). Solar astrophysics: an overview. Bulletin of the Astronomical Society of India. 24. 89. 4 indexed citations
14.
Singh, Harinder P., I. W. Roxburgh, & K. L. Chan. (1996). Numerical simulation of penetrative convection. Bulletin of the Astronomical Society of India. 24. 281. 4 indexed citations
15.
Schwartz, S. J. & I. W. Roxburgh. (1980). Instabilities in the solar wind. Philosophical Transactions of the Royal Society of London Series A Mathematical and Physical Sciences. 297(1433). 555–563. 1 indexed citations
16.
Roxburgh, I. W.. (1977). Testing relativity and gravitational theories by radar ranging to a heliocentric satellite. Philosophical Transactions of the Royal Society of London Series A Mathematical and Physical Sciences. 284(1326). 589–593. 1 indexed citations
17.
Durney, B. R. & I. W. Roxburgh. (1967). Rotating massive stars in general relativity. Proceedings of the Royal Society of London A Mathematical and Physical Sciences. 296(1445). 189–200. 4 indexed citations
18.
Latham, J. & I. W. Roxburgh. (1966). Disintegration of pairs of water drops in an electric field. Proceedings of the Royal Society of London A Mathematical and Physical Sciences. 295(1440). 84–97. 53 indexed citations
19.
Roxburgh, I. W., W. L. W. Sargent, & P. A. Strittmatter. (1966). Determination of rotational velocity and aspect for stars in clusters. Observatory. 86. 118–120. 2 indexed citations
20.
Roxburgh, I. W., J. S. Griffith, & P. A. Sweet. (1965). On Models of Non Spherical Stars I. The Theory of Rapildy Rotating Main Sequence Stars. With 3 Figures in the Text. 61. 203. 1 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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