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.
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
19961.8k citationsJames B. Pollack et al.profile →
Countries citing papers authored by James B. Pollack
Since
Specialization
Citations
This map shows the geographic impact of James B. Pollack'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 James B. Pollack with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites James B. Pollack more than expected).
Fields of papers citing papers by James B. Pollack
This network shows the impact of papers produced by James B. Pollack. 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 James B. Pollack. The network helps show where James B. Pollack may publish in the future.
Co-authorship network of co-authors of James B. Pollack
This figure shows the co-authorship network connecting the top 25 collaborators of James B. Pollack.
A scholar is included among the top collaborators of James B. Pollack 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 James B. Pollack. James B. Pollack 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.
Dalton, J. B., James B. Pollack, David Grinspoon, Bruno Bézard, & C. de Bérgh. (2000). Distribution of Chlorine in the Lower Atmosphere of Venus. 32.2 indexed citations
2.
Forget, F., G. B. Hansen, & James B. Pollack. (1995). Low Brightness Temperatures of Martian Polar Caps. DPS. 27.6 indexed citations
3.
Bell, James F., et al.. (1994). Wavelength calibration techniques and subtle surface and atmospheric absorption features in the Mariner 6, 7 IRS reflectance data. Lunar and Planetary Science Conference. 87.2 indexed citations
4.
Forget, F. & James B. Pollack. (1993). Impact of the CO2 and H2O clouds of the Martian polar hood on the polar energy balance. DPS. 25. 13–14.1 indexed citations
5.
Encrenaz, T., P. Drossart, Bruno Bézard, et al.. (1992). The H 2 O Abundance in the Lower Atmosphere of Venus from NIMS-Galileo. DPS. 24.1 indexed citations
6.
Pollack, James B., et al.. (1991). Simulations of the Seasonal Pressure Changes on Mars with a General Circulation Model. Bulletin of the American Astronomical Society. 23. 1214.1 indexed citations
7.
Leach, R., R. Greeley, & James B. Pollack. (1989). Saltation thresholds and entrainment of fine particles at Earth and Martian pressures. NASA STI Repository (National Aeronautics and Space Administration). 90. 14997.5 indexed citations
8.
Colburn, D. S., James B. Pollack, & R. M. Haberle. (1988). Diurnal variations in optical depth at Mars: Observations and interpretations. NASA STI/Recon Technical Report N. 88. 25420.4 indexed citations
9.
Pollack, James B. & R. M. Haberle. (1988). Simulations of the General Circulation of the Martian Atmosphere. Bulletin of the American Astronomical Society. 20. 859.77 indexed citations
10.
Greeley, R., et al.. (1980). Venus aeolian processes: saltation studies and the Venusian wind tunnel.. 275–277.3 indexed citations
11.
Toon, O. B., B. N. Khare, James B. Pollack, & Carl Sagan. (1978). Martian Surface Composition: Comparison of Remote Spectral Studies and In-Situ X-Ray Fluorescence Analysis. Bulletin of the American Astronomical Society. 10. 115.1 indexed citations
12.
Haberle, R. M., Conway Β. Leovy, & James B. Pollack. (1978). The Martian Polar Cap Winds and the Formation of High Latitude Surface Features. Bulletin of the American Astronomical Society. 10. 553.3 indexed citations
13.
Greeley, R., et al.. (1974). Wind tunnel studies of Martian aeolian processes. Proceedings of the Royal Society of London A Mathematical and Physical Sciences. 341(1626). 331–360.79 indexed citations
14.
Pollack, James B., O. B. Toon, & Carl Sagan. (1974). Physical Properties of the Particles Composing the Great Martian Dust Storm of 1971. Bulletin of the American Astronomical Society. 6. 370.4 indexed citations
15.
Pollack, James B., et al.. (1974). Estimates of the Minimum Wind Needed to Raise Dust on Mars. Bulletin of the American Astronomical Society. 6. 370.1 indexed citations
16.
Pollack, James B.. (1974). Models of temperature structure and general circulation. NASA Technical Reports Server (NASA). 340. 72.2 indexed citations
17.
Iversen, James D., B. R. White, R. Greeley, & James B. Pollack. (1973). Simulations of Martian Eolian Phenomena in the Atmospheric Wind Tunnel. NASA Special Publication. 336. 191.16 indexed citations
18.
Pollack, James B., et al.. (1970). A reexamination of the stability of goethite on Mars.. Bulletin of the American Astronomical Society. 2. 239.2 indexed citations
19.
Goldstein, R. M., James B. Pollack, & Carl Sagan. (1967). Radar Doppler spectroscopy of Mars. I.. The Astronomical Journal.6 indexed citations
20.
Sagan, Carl & James B. Pollack. (1967). A Windblown Dust Model of Martian Surface Features and Seasonal Changes.. American Journal of Sociology. 255. 33.9 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.