D. E. Shemansky

8.9k total citations · 1 hit paper
164 papers, 6.9k citations indexed

About

D. E. Shemansky is a scholar working on Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics and Atmospheric Science. According to data from OpenAlex, D. E. Shemansky has authored 164 papers receiving a total of 6.9k indexed citations (citations by other indexed papers that have themselves been cited), including 118 papers in Astronomy and Astrophysics, 57 papers in Atomic and Molecular Physics, and Optics and 37 papers in Atmospheric Science. Recurrent topics in D. E. Shemansky's work include Astro and Planetary Science (95 papers), Planetary Science and Exploration (47 papers) and Atomic and Molecular Physics (45 papers). D. E. Shemansky is often cited by papers focused on Astro and Planetary Science (95 papers), Planetary Science and Exploration (47 papers) and Atomic and Molecular Physics (45 papers). D. E. Shemansky collaborates with scholars based in United States, France and Canada. D. E. Shemansky's co-authors include A. L. Broadfoot, J. M. Ajello, B. R. Sandel, D. F. Strobel, Gerald R. Smith, Xianming Liu, T. M. Donahue, J. B. Holberg, S. K. Atreya and D. T. Hall and has published in prestigious journals such as Nature, Science and The Journal of Chemical Physics.

In The Last Decade

D. E. Shemansky

158 papers receiving 5.9k citations

Hit Papers

align trajectories

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.

Extreme Ultraviolet Observations from Voyager 1 Encounter with Jupiter

1979 640 citations B. R. Sandel, D. E. Shemansky et al. profile →

Peers

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

#	Work	Indexed citations
1	Isotope dependence of thec³Π_u−b³Σ${}_{u}^{+}$ andD¹Π${}_{u}^{+}$−B′¹Σ${}_{u}^{+}$ predissociation rates of molecular hydrogen 2018 ·Journal of Physics Communications ·Xianming Liu, D. E. Shemansky, (unknown), (unknown), (unknown)	0
2	Excitation by Electron Impact: Energies, Spectra, Emission Yields, Cross-sections, and H(1s) Kinetic Energy Distributions 2017 ·The Astrophysical Journal Supplement Series ·Xianming Liu, D. E. Shemansky, (unknown), (unknown), P. V. Johnson, C. P. Malone, M. A. Khakoo	3
3	Energies, transition probabilities, predissociation rates, and lifetimes of the ${{\rm{H}}}_{2}$, HD, and ${{\rm{D}}}_{2}$ $c{}^{3}{{\rm{\Pi }}}_{u}^{-}$ state 2017 ·Journal of Physics B Atomic Molecular and Optical Physics ·Xianming Liu, D. E. Shemansky, (unknown), (unknown), P. V. Johnson, C. P. Malone	1
4	Investigation of diurnal variability of water vapor in Enceladus' plume by the Cassini ultraviolet imaging spectrograph 2017 ·Geophysical Research Letters ·C. J. Hansen, L. W. Esposito, K. M. Aye, J. E. Colwell, Amanda Hendrix, Ganna Portyankina, D. E. Shemansky	17
5	SPECTRA, EMISSION YIELDS, CROSS SECTIONS, AND KINETIC ENERGY DISTRIBUTIONS OF HYDROGEN ATOMS FROM H₂ – EXCITATION BY ELECTRON IMPACT 2016 ·The Astrophysical Journal ·Xianming Liu, D. E. Shemansky, (unknown), P. V. Johnson, C. P. Malone, J. M. Ajello	5
6	A NEW UNDERSTANDING OF THE EUROPA ATMOSPHERE AND LIMITS ON GEOPHYSICAL ACTIVITY 2014 ·The Astrophysical Journal ·D. E. Shemansky, Yuk L. Yung, Xianming Liu, (unknown), C. J. Hansen, Amanda Hendrix, L. W. Esposito	19
7	Probing Titan's Upper Atmosphere: Observations from Cassini UVIS 2011 ·Joshua A. Kammer, D. E. Shemansky, (unknown), Y. L. Yung	1
8	Saturn Auroral Images and Movies from Cassini UVIS 2009 ·Open Repository and Bibliography (University of Liège) ·W. R. Pryor, L. W. Esposito, A. I. F. Stewart, (unknown), W. E. McClintock, G. M. Holsclaw, S. Eriksson, J. M. Ajello, (unknown), C. J. Hansen, Amanda Hendrix, D. E. Shemansky, J. T. Clarke, J. D. Nichols, Jacques Gustin, Denis Grodent, Jean‐Claude Gérard, J. E. Colwell, G. B. Hospodarsky, D. G. Mitchell	2
9	Auroral Movies and Spectroscopy from Cassini UVIS 2007 ·Open Repository and Bibliography (University of Liège) ·W. R. Pryor, R. G. West, Ian Stewart, L. W. Esposito, (unknown), (unknown), J. E. Colwell, K. Larsen, G. M. Holsclaw, D. E. Shemansky, J. M. Ajello, C. J. Hansen, John Clarke, Jacques Gustin, Denis Grodent, Jean‐Claude Gérard	1
10	The High Altitude Sunlit Titan Ionosphere 2005 ·AGUFM ·(unknown), D. E. Shemansky, (unknown)	2
11	Titan solar reflection and emission properties in the EUV/FUV 2004 ·AGU Fall Meeting Abstracts ·(unknown), D. E. Shemansky, Yuk L. Yung, (unknown)	1
12	Cassini ultraviolet imaging spectrometer observations of the Venus dayglow. 1999 ·Bulletin of the American Astronomical Society ·A. I. F. Stewart, L. W. Esposito, C. Barth, J. E. Colwell, G. M. Lawrence, W. E. McClintock, W. R. Pryor, H. U. Keller, A. Korth, H. Lauche, M. C. Festou, A. L. Lane, (unknown), J. N. Maki, R. A. West, H. Jahn, Ralf Reulke, (unknown), D. E. Shemansky, Y. L. Yung	1
13	Initial Jupiter Atmosphere Results from the Galileo Ultraviolet Spectrometer Experiment 1996 ·W. R. Pryor, C. W. Hord, C. A. Barth, A. I. F. Stewart, W. E. McClintock, K. E. Simmons, J. M. Ajello, R. A. West, W. Kent Tobiska, D. E. Shemansky, B. R. Sandel, J. T. Clarke	3
14	The abundance of O(2+) in the Jovian magnetosphere 1992 ·Geophysical Research Letters ·F. Bagenal, D. E. Shemansky, R. L. McNutt, (unknown), A. Eviatar	3
15	A Search for Cometesimal Derived Atmosphere on the Moon 1990 ·D. E. Shemansky	1
16	Search for [OI] 6300 Å Emission from Io 1989 ·Bulletin of the American Astronomical Society ·N. M. Schneider, D. E. Shemansky, Ka Chun Yu	5
17	The Ultraviolet Reflection Spectrum of Uranus 1986 ·Bulletin of the American Astronomical Society ·D. F. Strobel, J. C. McConnell, R. V. Yelle, D. E. Shemansky, Y. L. Yung	1
18	Escape of Io's Atmosphere and its Impact on the Plasma Torus 1985 ·Bulletin of the American Astronomical Society ·W. H. Smyth, M. R. Combi, D. E. Shemansky	1
19	Hydrogen Blow-Off from Uranus; an Extrapolation from Jupiter and Saturn 1984 ·Bulletin of the American Astronomical Society ·D. E. Shemansky, Gerald R. Smith	2
20	Radiative Transfer of Internal Sources: Application to the Lyman a Dayglow on Jupiter 1983 ·Bulletin of the American Astronomical Society ·G. R. Gladstone, D. E. Shemansky	2

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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