This map shows the geographic impact of D. MacDougall'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 D. MacDougall with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. MacDougall more than expected).
This network shows the impact of papers produced by D. MacDougall. 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 D. MacDougall. The network helps show where D. MacDougall may publish in the future.
Co-authorship network of co-authors of D. MacDougall
This figure shows the co-authorship network connecting the top 25 collaborators of D. MacDougall.
A scholar is included among the top collaborators of D. MacDougall 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 D. MacDougall. D. MacDougall is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
MacDougall, D. & D. Phinney. (1977). Noble Gases and Particle Tracks in Olivine Crystals from Murchison and Cold Bokkeveld. LPI. 8. 605.
3.
MacDougall, D., et al.. (1977). Angra Dos Reis Revisited: Particle Tracks and Their Implications. Metic. 12. 284.1 indexed citations
4.
Price, P. B., et al.. (1975). Track Studies Bearing on Solar System Regoliths. 3. 3449–3469.15 indexed citations
5.
Hutcheon, I. D., D. MacDougall, & P. B. Price. (1974). Improved determination of the long-term average Fe spectrum from ≡ 1 to ≡ 460 MeV/amu.. Lunar and Planetary Science Conference Proceedings. 3. 2561–2576.4 indexed citations
6.
Hutcheon, I. D., D. MacDougall, & John S. Stevenson. (1974). Apollo 17 particle track studies: surface residence times and fission track ages for orange glass and large boulders.. Lunar and Planetary Science Conference Proceedings. 3. 2597–2608.6 indexed citations
7.
Hutcheon, I. D., D. MacDougall, P. B. Price, et al.. (1974). Rock 72315: A New Lunar Standard For Solar Flare and Micrometeorite Exposure. Lunar and Planetary Science Conference. 5. 378.1 indexed citations
8.
MacDougall, D. & P. B. Price. (1974). Low-energy particle irradiation and possible age indicator for components of carbonaceous chondrites. Meteoritics and Planetary Science. 9. 370.4 indexed citations
9.
MacDougall, D., I. D. Hutcheon, & P. B. Price. (1974). Irradiation Records in Orange Glass and Two Boulders From Apollo 17. LPI. 5. 483.4 indexed citations
10.
Arrhenius, Gustaf, et al.. (1974). Record of primordial growth environment in olivine crystals from carbonaceous chondrites. Meteoritics and Planetary Science. 9. 313.6 indexed citations
MacDougall, D., R. S. Rajan, I. D. Hutcheon, & P. B. Price. (1973). Irradiation history and accretionary processes in lunar and meteoritic breccias. Lunar and Planetary Science Conference Proceedings. 4. 2319.8 indexed citations
15.
Price, P. Buford, Jonathan H. Chan, I. D. Hutcheon, et al.. (1973). Low-energy heavy ions in the solar system. Lunar and Planetary Science Conference Proceedings. 4. 2347.6 indexed citations
16.
Arrhenius, Gustaf, D. MacDougall, L. L. Wilkening, et al.. (1971). The exposure history of the Apollo 12 regolith. Lunar and Planetary Science Conference Proceedings. 2. 2583.25 indexed citations
Arrhenius, Gustaf, et al.. (1970). Mixing of the lunar regolith and cosmic ray spectra - Evidence from particle-track studies. NASA Technical Reports Server (NASA). 1. 2295.11 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.