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.
JUpiter ICy moons Explorer (JUICE): An ESA mission to orbit Ganymede and to characterise the Jupiter system
2012422 citationsLeigh N. Fletcher et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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Countries citing papers authored by Leigh N. Fletcher
Since
Specialization
Citations
This map shows the geographic impact of Leigh N. Fletcher'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 Leigh N. Fletcher with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Leigh N. Fletcher more than expected).
Fields of papers citing papers by Leigh N. Fletcher
This network shows the impact of papers produced by Leigh N. Fletcher. 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 Leigh N. Fletcher. The network helps show where Leigh N. Fletcher may publish in the future.
Co-authorship network of co-authors of Leigh N. Fletcher
This figure shows the co-authorship network connecting the top 25 collaborators of Leigh N. Fletcher.
A scholar is included among the top collaborators of Leigh N. Fletcher 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 Leigh N. Fletcher. Leigh N. Fletcher is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Fletcher, Leigh N., et al.. (2019). Compositional Mapping of Europa with VLT/SPHERE. Lunar and Planetary Science Conference. 2019(2326). 2046.1 indexed citations
Irwin, P. G. J., et al.. (2017). Identifying the source of colour and featural changes in Jupiter's atmosphere from MUSE/VLT. European Planetary Science Congress.1 indexed citations
15.
Pater, Imke de, Philip Marcus, Statia Luszcz‐Cook, et al.. (2016). Vertical Wind Shear in Neptune's Atmosphere Explained with a Modified Thermal Wind Equation. 48.
16.
Orton, Glenn S., Leigh N. Fletcher, F. M. Flasar, & R. K. Achterberg. (2014). Variations of Zonal Thermal Waves in Saturn from Cassini CIRS Observations. EGUGA. 2488.1 indexed citations
17.
Hesman, B. E., G. L. Bjoraker, Pedro V. Sada, et al.. (2011). Elusive Ethylene Detected in Saturn's Northern Storm Region. Oxford University Research Archive (ORA) (University of Oxford). 2011. 1222.1 indexed citations
18.
Hofstadter, Mark, G. S. Orton, Leigh N. Fletcher, et al.. (2009). Infrared and Microwave Observations of Uranus: Implications for Temperature, Composition, Circulation and a Standard Calibration Model for Herschel. 41.1 indexed citations
19.
Read, P. L., et al.. (2007). Zonal Mean Dynamics On Saturn From Cassini And Voyager Data.3 indexed citations
20.
Parrish, P., Glenn S. Orton, P. A. Yanamandra-Fisher, et al.. (2005). Saturn's atmospheric structure: the intercomparison of Cassini/CIRS-derived temperatures with ground-based determinations. 37.2 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.