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.
The Mathematical Theory of Non-Uniform Gases
19622.1k citationsSydney Chapman, T. G. Cowling et al.profile →
Countries citing papers authored by Sydney Chapman
Since
Specialization
Citations
This map shows the geographic impact of Sydney Chapman'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 Sydney Chapman with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Sydney Chapman more than expected).
This network shows the impact of papers produced by Sydney Chapman. 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 Sydney Chapman. The network helps show where Sydney Chapman may publish in the future.
Co-authorship network of co-authors of Sydney Chapman
This figure shows the co-authorship network connecting the top 25 collaborators of Sydney Chapman.
A scholar is included among the top collaborators of Sydney Chapman 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 Sydney Chapman. Sydney Chapman is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Whitworth, A. P., A. S. Bhattal, Sydney Chapman, M. J. Disney, & J. A. Turner. (1994). Fragmentation of shocked interstellar gas layers.. ORCA Online Research @Cardiff (Cardiff University). 290. 421–427.
3.
Akasofu, S.‐I. & Sydney Chapman. (1972). Solar-terrestrial physics : an account of the wave and particle radiations from the quiet and the active sun, and of the consequent terrestrial phenomena. CERN Document Server (European Organization for Nuclear Research).7 indexed citations
Chapman, Sydney, et al.. (1968). Solar and lunar daily geomagnatic variations at San Fernando and Greenwich in relation to the associated electric current systems. Vandenhoeck & Ruprecht eBooks.2 indexed citations
Chapman, Sydney. (1961). Dynamical and Other Aspects of Cosmic Gases of Low Density. 669.1 indexed citations
10.
Akasofu, S.‐I. & Sydney Chapman. (1961). A neutral line discharge theory of the aurora polaris. Philosophical Transactions of the Royal Society of London Series A Mathematical and Physical Sciences. 253(1031). 359–406.39 indexed citations
11.
Akasofu, Syun‐Ichi & Sydney Chapman. (1961). A study of magnetic storms and auroras. ScholarWorks - UA (University of Alaska System).5 indexed citations
Chapman, Sydney. (1959). Cosmic examples of heat conduction in very rare rotating or expanding gases. Annales de Geophysique. 15. 434.1 indexed citations
14.
Chapman, Sydney. (1959). IGY. University of Michigan Press eBooks.10 indexed citations
Chapman, Sydney & D. W. N. Stibbs. (1953). Solar Eclipses and the Aurora Borealis. Sky and Telescope. 13. 35.2 indexed citations
18.
Chapman, Sydney. (1952). Theories of the aurora polaris. 8. 205.9 indexed citations
19.
Chapman, Sydney & T. G. Cowling. (1951). The mathematical theory of non-uniform gases : notes added in 1951. Cambridge University Press eBooks.2 indexed citations
20.
Chapman, Sydney, et al.. (1951). Geomagnetic and related phenomena. University Press eBooks.9 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.