D. E. Shemansky

1.6k total citations · 1 hit paper
26 papers, 1.0k citations indexed

About

D. E. Shemansky is a scholar working on Astronomy and Astrophysics, Atmospheric Science and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, D. E. Shemansky has authored 26 papers receiving a total of 1.0k indexed citations (citations by other indexed papers that have themselves been cited), including 19 papers in Astronomy and Astrophysics, 6 papers in Atmospheric Science and 5 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in D. E. Shemansky's work include Astro and Planetary Science (17 papers), Planetary Science and Exploration (11 papers) and Atmospheric Ozone and Climate (6 papers). D. E. Shemansky is often cited by papers focused on Astro and Planetary Science (17 papers), Planetary Science and Exploration (11 papers) and Atmospheric Ozone and Climate (6 papers). D. E. Shemansky collaborates with scholars based in United States and Australia. D. E. Shemansky's co-authors include A. I. F. Stewart, Amanda Hendrix, C. J. Hansen, Robert A. West, L. W. Esposito, J. E. Colwell, W. R. Pryor, J. M. Ajello, D. T. Hall and Todd M. Tripp and has published in prestigious journals such as Nature, Science and Journal of Geophysical Research Atmospheres.

In The Last Decade

D. E. Shemansky

25 papers receiving 948 citations

Hit Papers

align trajectories sort by overperformance

What are hit papers?

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.

Enceladus' Water Vapor Plume

2006 414 citations L. W. Esposito, J. E. Colwell et al. profile →

Author Peers

Peers are selected by citation overlap in the author's most active subfields. citations · hero ref

Author						Papers	Cites
D. E. Shemansky	877	250	120	101	54	26	1.0k
L. M. Trafton	741 0.8×	275 1.1×	77 0.6×	91 0.9×	100 1.9×	76	873
Timothy A. Cassidy	1.3k 1.5×	260 1.0×	172 1.4×	64 0.6×	31 0.6×	53	1.4k
G. Moragas‐Klostermeyer	1.3k 1.4×	201 0.8×	139 1.2×	105 1.0×	65 1.2×	42	1.4k
S. Engel	1.2k 1.3×	329 1.3×	49 0.4×	76 0.8×	78 1.4×	22	1.3k
N. Altobelli	1.4k 1.6×	253 1.0×	80 0.7×	54 0.5×	61 1.1×	87	1.5k
Lorenz Roth	1.1k 1.3×	238 1.0×	159 1.3×	35 0.3×	38 0.7×	57	1.2k
S. H. Way	1.2k 1.4×	460 1.8×	63 0.5×	115 1.1×	185 3.4×	13	1.3k
Hasso B. Niemann	1.4k 1.6×	419 1.7×	103 0.9×	85 0.8×	132 2.4×	20	1.5k
L. Herath	587 0.7×	327 1.3×	65 0.5×	103 1.0×	163 3.0×	11	804
Gregorio J. Molina‐Cuberos	909 1.0×	169 0.7×	83 0.7×	110 1.1×	44 0.8×	69	1.1k

Countries citing papers authored by D. E. Shemansky

Since Specialization

Citations

This map shows the geographic impact of D. E. Shemansky'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. E. Shemansky with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. E. Shemansky more than expected).

Fields of papers citing papers by D. E. Shemansky

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by D. E. Shemansky. 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. E. Shemansky. The network helps show where D. E. Shemansky may publish in the future.

Co-authorship network of co-authors of D. E. Shemansky

This figure shows the co-authorship network connecting the top 25 collaborators of D. E. Shemansky. A scholar is included among the top collaborators of D. E. Shemansky 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. E. Shemansky. D. E. Shemansky is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

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20 of 20 papers shown

Esposito, L. W., J. E. Colwell, Amanda Hendrix, et al.. (2015). Deriving the Structure and Composition of Enceladus’ Plume from Cassini UVIS Observations. DPS. 1 indexed citations

Kammer, Joshua A., D. E. Shemansky, X. Zhang, & Yuk L. Yung. (2013). Composition of Titan's upper atmosphere from Cassini UVIS EUV stellar occultations. Planetary and Space Science. 88. 86–92. 14 indexed citations

Sittler, E. C., C. Bertucci, A. J. Coates, et al.. (2008). Energy Deposition Processes in Titan's Upper Atmosphere. NASA Technical Reports Server (NASA). 1 indexed citations

Shemansky, D. E.. (2006). Atmospheric Structure of Saturn and Titan: Results from the Cassini UVIS Experiment. 36. 2756. 1 indexed citations

Hendrix, Amanda, L. W. Esposito, J. E. Colwell, et al.. (2005). Cassini UltraViolet Imaging Spectrograph (UVIS) Observations of Enceladus' Plume. AGUFM. 2005. 1 indexed citations

Shemansky, D. E., et al.. (2005). Fine‐structure physical chemistry modeling of Uranus H₂ X quadrupole emission. Geophysical Research Letters. 32(2). 5 indexed citations

Shemansky, D. E., et al.. (2004). Cassini UVIS Observatory Phase spectral imaging of the Saturn system. 35. 2500. 1 indexed citations

Shemansky, D. E., J. M. Ajello, & I. Kanik. (1995). Electron Excitation Function of the N 2 Second Positive System. The Astrophysical Journal. 452. 472–472. 37 indexed citations

Shemansky, D. E., I. Kanik, & J. M. Ajello. (1995). Fine-Structure Branching in N 2 C 4 1 Sigma + U (0). The Astrophysical Journal. 452. 480–480. 30 indexed citations

10.

Shemansky, D. E., et al.. (1993). Detection of the hydroxyl radical in the Saturn magnetosphere. Nature. 363(6427). 329–331. 121 indexed citations

11.

Ajello, J. M., G. K. James, & D. E. Shemansky. (1991). Cross sections for production of H(2p, 2s, 1s) by electron collisional dissociation of H2. The Astrophysical Journal. 371. 422–422. 44 indexed citations

12.

Shemansky, D. E.. (1990). Critical quantities for solar system science in atomic and molecular reactions. AIP conference proceedings. 206. 163–176. 3 indexed citations

13.

Hall, D. T. & D. E. Shemansky. (1988). The Evidence Against an Inner Solar System Source of Atomic Hydrogen. Bulletin of the American Astronomical Society. 20. 836. 3 indexed citations

14.

Shemansky, D. E.. (1988). Correction to “Energy branching in the Io plasma Torus: The failure of neutral cloud theory”. Journal of Geophysical Research Atmospheres. 93(A6). 5991–5991. 4 indexed citations

15.

Hall, D. T., et al.. (1986). Helium in Collisional Equilibrium with an Electron Gas. Bulletin of the American Astronomical Society. 18. 1004. 1 indexed citations

16.

Bagenal, F. & D. E. Shemansky. (1985). Ion Partitioning in the Io Torus: Voyager I PLS vs. UVS Experiments. Bulletin of the American Astronomical Society. 17. 694. 1 indexed citations

17.

Shemansky, D. E., et al.. (1984). Pioneer 10 and Voyager Observations of the Interstellar Medium in Scattered Emission of the He 584 A and H Lyα 1216 A Lines. International Astronomical Union Colloquium. 81. 24–27. 20 indexed citations

18.

Brown, Robert A., D. E. Shemansky, & R. E. Johnson. (1983). A deficiency of O III in the Io plasma torus. The Astrophysical Journal. 264. 309–309. 37 indexed citations

19.

Shemansky, D. E. & Robert A. Brown. (1982). A Deficiency of OIII in the Io Plasma Torus.. Bulletin of the American Astronomical Society. 14. 763. 19 indexed citations

20.

Shemansky, D. E. & B. R. Sandel. (1980). Radial Dependence of the Io Plasma Torus Spectrum in the EUV.. Bulletin of the American Astronomical Society. 12. 674. 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.

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