Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
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).
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.
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
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
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
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.