S. B. Charnley

2.2k total citations
36 papers, 1.3k citations indexed

About

S. B. Charnley is a scholar working on Astronomy and Astrophysics, Spectroscopy and Atmospheric Science. According to data from OpenAlex, S. B. Charnley has authored 36 papers receiving a total of 1.3k indexed citations (citations by other indexed papers that have themselves been cited), including 32 papers in Astronomy and Astrophysics, 15 papers in Spectroscopy and 12 papers in Atmospheric Science. Recurrent topics in S. B. Charnley's work include Astro and Planetary Science (23 papers), Astrophysics and Star Formation Studies (22 papers) and Molecular Spectroscopy and Structure (14 papers). S. B. Charnley is often cited by papers focused on Astro and Planetary Science (23 papers), Astrophysics and Star Formation Studies (22 papers) and Molecular Spectroscopy and Structure (14 papers). S. B. Charnley collaborates with scholars based in United States, United Kingdom and Australia. S. B. Charnley's co-authors include Scott Rodgers, A. G. G. M. Tielens, T. J. Millar, M. E. Kress, Eric Herbst, Paul D. Brown, D. A. Williams, L. A. M. Nejad, J. E. Dyson and T. W. Hartquist and has published in prestigious journals such as The Astrophysical Journal, Geophysical Research Letters and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

S. B. Charnley

36 papers receiving 1.3k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
S. B. Charnley United States 18 1.1k 785 548 473 40 36 1.3k
Å. Hjalmarson Sweden 20 1.2k 1.1× 936 1.2× 688 1.3× 545 1.2× 49 1.2× 69 1.6k
M. A. Frerking United States 20 1.5k 1.4× 879 1.1× 592 1.1× 554 1.2× 26 0.7× 81 2.0k
F. Baas Netherlands 20 1.1k 1.1× 613 0.8× 446 0.8× 356 0.8× 36 0.9× 54 1.4k
Per Friberg United States 22 1.1k 1.1× 981 1.2× 789 1.4× 552 1.2× 16 0.4× 56 1.7k
W. M. Irvine United States 18 858 0.8× 753 1.0× 522 1.0× 411 0.9× 30 0.8× 28 1.2k
H. E. Matthews United States 19 883 0.8× 656 0.8× 478 0.9× 368 0.8× 35 0.9× 53 1.2k
J. E. Dickens United States 14 758 0.7× 611 0.8× 422 0.8× 377 0.8× 28 0.7× 20 973
R. Terzieva United States 10 777 0.7× 516 0.7× 459 0.8× 357 0.8× 34 0.8× 12 987
G. Fedoseev Netherlands 21 1.0k 0.9× 751 1.0× 636 1.2× 484 1.0× 17 0.4× 48 1.3k
N. F. W. Ligterink Switzerland 22 965 0.9× 825 1.1× 383 0.7× 441 0.9× 46 1.1× 62 1.2k

Countries citing papers authored by S. B. Charnley

Since Specialization
Citations

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

Fields of papers citing papers by S. B. Charnley

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by S. B. Charnley. 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 S. B. Charnley. The network helps show where S. B. Charnley may publish in the future.

Co-authorship network of co-authors of S. B. Charnley

This figure shows the co-authorship network connecting the top 25 collaborators of S. B. Charnley. A scholar is included among the top collaborators of S. B. Charnley 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 S. B. Charnley. S. B. Charnley 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.
Cordiner, Martin, Gerónimo Villanueva, H. Wiesemeyer, et al.. (2022). Phosphine in the Venusian Atmosphere: A Strict Upper Limit From SOFIA GREAT Observations. Geophysical Research Letters. 49(22). 17 indexed citations
2.
Taquet, V., E. S. Wirström, S. B. Charnley, et al.. (2017). Chemical complexity induced by efficient ice evaporation in the Barnard 5 molecular cloud. Astronomy and Astrophysics. 607. A20–A20. 36 indexed citations
3.
Thelen, Alexander E., C. A. Nixon, N. J. Chanover, et al.. (2017). Spatial variations in Titan’s atmospheric temperature: ALMA and Cassini comparisons from 2012 to 2015. Icarus. 307. 380–390. 14 indexed citations
4.
Molter, Edward, C. A. Nixon, Martin Cordiner, et al.. (2016). ALMA OBSERVATIONS OF HCN AND ITS ISOTOPOLOGUES ON TITAN. The Astronomical Journal. 152(2). 42–42. 37 indexed citations
5.
Elsila, Jamie E., et al.. (2013). Compound-Specific Isotopic Ratios of Amino Acids in CM and CR Chondrites. NASA STI Repository (National Aeronautics and Space Administration). 1281. 1 indexed citations
6.
Charnley, S. B. & Scott Rodgers. (2008). Nitrogen Superfractionation in Interstellar Chemistry. Lunar and Planetary Science Conference. 2233. 1 indexed citations
7.
Rodgers, Scott, S. B. Charnley, Robert G. Smith, & H. M. Butner. (2007). Chemical chronology of the Southern Coalsack. Monthly Notices of the Royal Astronomical Society. 379(2). 807–815. 1 indexed citations
8.
Coulson, I. M., H. M. Butner, G. H. Moriarty‐Schieven, et al.. (2005). Deep Impact: Submillimetre Spectroscopic HCN Observations of 9P/Tempel-1 from JCMT. 1. 8524–268. 1 indexed citations
9.
Rodgers, Scott, H. M. Butner, S. B. Charnley, & P. Ehrenfreund. (2003). The HNC/HCN ratio in comets: Observations of C/2002 C1 (Ikeya-Zhang). Advances in Space Research. 31(12). 2577–2582. 5 indexed citations
10.
Charnley, S. B.. (2001). Interstellar Organic Chemistry. 34. 139. 7 indexed citations
11.
Rodgers, Scott & S. B. Charnley. (2001). Chemical Differentiation in Regions of Massive Star Formation. The Astrophysical Journal. 546(1). 324–329. 101 indexed citations
12.
Hollenbach, D. J., et al.. (1999). Summary of Research. STIN. 99. 81101. 11 indexed citations
13.
Smith, Robert G., et al.. (1998). H[TINF]2[/TINF]O Ice in the Envelopes of OH/IR Stars. The Astronomical Journal. 115(6). 2509–2514. 9 indexed citations
14.
Charnley, S. B.. (1995). Gas-grain processes in the envelopes of late-type stars. Astrophysics and Space Science. 224(1-2). 439–440. 1 indexed citations
15.
Millar, T. J., J. M. C. Rawlings, Alec Bennett, Paul D. Brown, & S. B. Charnley. (1991). GAS-PHASE REACTIONS AND RATE COEFFICIENTS FOR USE IN ASTROCHEMISTRY - THE UMIST RATEFILE. UCL Discovery (University College London). 87(3). 585–619. 29 indexed citations
16.
Millar, T. J., Eric Herbst, & S. B. Charnley. (1991). The formation of oxygen-containing organic molecules in the Orion compact ridge. The Astrophysical Journal. 369. 147–147. 111 indexed citations
17.
Nejad, L. A. M., D. A. Williams, & S. B. Charnley. (1990). Dynamical models of molecular clouds: nitrogen chemistry. Monthly Notices of the Royal Astronomical Society. 246(1). 183–190. 42 indexed citations
18.
Charnley, S. B., J. E. Dyson, T. W. Hartquist, & D. A. Williams. (1990). Chemical evolution in molecular clump-stellar wind interfaces. Monthly Notices of the Royal Astronomical Society. 243(3). 405–412. 14 indexed citations
19.
Brown, Paul D. & S. B. Charnley. (1990). Chemical models of interstellar gas-grain processes. I. Modelling and the effect of accretion on gas abundances and mantle composition in dense clouds.. Monthly Notices of the Royal Astronomical Society. 244(3). 432–443. 51 indexed citations
20.
Charnley, S. B., J. E. Dyson, T. W. Hartquist, & D. A. Williams. (1988). Chemical limit cycles for models of a region of low-mass star formation. Monthly Notices of the Royal Astronomical Society. 235(4). 1257–1271. 16 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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