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.
Composition and radiative properties of grains in molecular clouds and accretion disks
1994645 citationsJames B. Pollack, D. P. Simonelli et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
Countries citing papers authored by D. P. Simonelli
Since
Specialization
Citations
This map shows the geographic impact of D. P. Simonelli'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. P. Simonelli with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. P. Simonelli more than expected).
This network shows the impact of papers produced by D. P. Simonelli. 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. P. Simonelli. The network helps show where D. P. Simonelli may publish in the future.
Co-authorship network of co-authors of D. P. Simonelli
This figure shows the co-authorship network connecting the top 25 collaborators of D. P. Simonelli.
A scholar is included among the top collaborators of D. P. Simonelli 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. P. Simonelli. D. P. Simonelli 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.
Simonelli, D. P., B. J. Buratti, M. D. Hicks, et al.. (2004). The Roughness of Phoebe as Determined by Cassini VIMS.3 indexed citations
2.
McEwen, A. S., P. E. Geissler, M. P. Milazzo, et al.. (2001). Cassini and Galileo Imaging Observations of Io. elib (German Aerospace Center). 1824.1 indexed citations
3.
Williams, D. A., J. Radebaugh, L. Keszthelyi, et al.. (2001). Mapping of the Chaac-Camaxtli Region of Io. Lunar and Planetary Science Conference. 1220.1 indexed citations
4.
McEwen, A. S., E. P. Turtle, L. Keszthelyi, et al.. (2001). Galileo SSI Images of Io During the I31 and I32 Flybys. AGU Fall Meeting Abstracts. 2001.1 indexed citations
5.
Phillips, C. B., A. S. McEwen, L. Keszthelyi, et al.. (2000). Volcanic Resurfacing Rates and Styles on Io. DPS. 32.2 indexed citations
6.
Pappalardo, R. T., et al.. (1998). The Search for Active Resurfacing on Europa and Io. DPS.
7.
Phillips, C. B., A. S. McEwen, G. V. Hoppa, et al.. (1998). Change Detection on Europa and Io from Voyager and Galileo Images. LPI. 1732.1 indexed citations
8.
Simonelli, D. P., J. Veverka, A. S. McEwen, & Galileo Imaging Team. (1997). Porosity Variations on Io: Galileo SSI Observations of the Satellite's Opposition Surge. DPS.1 indexed citations
9.
McEwen, A. S., L. Keszthelyi, D. P. Simonelli, et al.. (1997). Observations of Io by SSI During the First Half of the Galileo Tour of Jupiter. LPI. 909.1 indexed citations
10.
McEwen, A. S., et al.. (1997). 17 Years of Surface Changes on Io: Galileo SSI Results. LPI. 907.4 indexed citations
11.
McEwen, A. S., et al.. (1997). Io Plume Observations with Galileo and HST. LPI. 911.6 indexed citations
12.
Pollack, J. B., et al.. (1991). Optical properties of grains in molecular clouds and accretion disks. 560.2 indexed citations
13.
Simonelli, D. P., J. B. Pollack, & Christopher P. McKay. (1989). Heating of Dust Falling Onto the Solar Nebula II: Energy-Balance Models. Bulletin of the American Astronomical Society. 21. 975.1 indexed citations
14.
Simonelli, D. P., James B. Pollack, Christopher P. McKay, R. T. Reynolds, & Audrey L. Summers. (1989). The carbon budget in the outer solar nebula. Icarus. 82(1). 1–35.33 indexed citations
15.
Simonelli, D. P., J. B. Pollack, & Christopher P. McKay. (1988). Heating of Interstellar Dust by the Solar Nebula Accretion Shock. Bulletin of the American Astronomical Society. 20. 815.1 indexed citations
16.
Simonelli, D. P. & Joseph Veverka. (1987). Io: Comparison of photometric scans produced by the Minnaert and Hapke functions. NASA STI Repository (National Aeronautics and Space Administration). 223.2 indexed citations
17.
Simonelli, D. P.. (1987). Voyager Photometry of IO. PhDT.
18.
Simonelli, D. P. & J. Veverka. (1984). Accurate Albedos of the Brightest Regions on Io. Bulletin of the American Astronomical Society. 16. 405–407.1 indexed citations
19.
Veverka, J., S. W. Squyres, P. C. Thomas, D. P. Simonelli, & David Morrison. (1980). Photometric studies of the satellites of Jupiter using Voyager imaging data.. 336–337.
20.
Simonelli, D. P., J. Veverka, P. Thomas, & D. Morrison. (1979). Voyager Search for Post-Eclipse Brightening on Io.. Bulletin of the American Astronomical Society. 11. 598.6 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.