L. G. Evans
About
In The Last Decade
L. G. Evans
92 papers receiving 747 citations
Peers
Comparison fields: 5 of 54
- Astronomy and Astrophysics 595
- Radiation 282
- Aerospace Engineering 130
- Ecology 76
- Atmospheric Science 52
Countries citing papers authored by L. G. Evans
This map shows the geographic impact of L. G. Evans'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 L. G. Evans with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites L. G. Evans more than expected).
Fields of papers citing papers by L. G. Evans
This network shows the impact of papers produced by L. G. Evans. 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 L. G. Evans. The network helps show where L. G. Evans may publish in the future.
Co-authorship network of co-authors of L. G. Evans
This figure shows the co-authorship network connecting the top 25 collaborators of L. G. Evans. A scholar is included among the top collaborators of L. G. Evans 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 L. G. Evans. L. G. Evans is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 0 | |
| 2 | 0 | |
| 3 | Chlorine on the Surface of Mercury: Implications for Mercury's Surface Evolution | 4 |
| 4 | Estimation of Hydrogen Concentration in Lunar South Polar Regions | 1 |
| 5 | Evidence for Diurnally Varying Hydration at the Moon's Equator from the Lunar Exploration Neutron Detector (LEND) | 4 |
| 6 | Bulk Insolation Models as Predictors for Locations for High Lunar Hydrogen Concentrations | 0 |
| 7 | Variable Sodium on the Surface of Mercury: Implications for Surface Chemistry and the Exosphere | 2 |
| 8 | The Iron Content of Mercury's Surface from MESSENGER X-Ray Spectrometry | 1 |
| 9 | Testing of Lunar Permanently Shadowed Regions for Water Ice | 1 |
| 10 | Surface Abundances of K, Th, and U on Mercury and Implications for Planet Formation and Evolution | 1 |
| 11 | Implications of the MESSENGER Discovery of High Sulfur Abundance on the Surface of Mercury | 4 |
| 12 | Neutron Suppression Regions at Lunar Poles, as Local Areas of Water-Rich Permafrost | 2 |
| 13 | X-Ray and Gamma-Ray Spectrometer Observations of the Elemental Composition of the Equatorial Region of Mercury: Testing Formation Models | 2 |
| 14 | First Estimate of Mercury's Surface Iron Abundance from Neutron Spectroscopy | 2 |
| 15 | Lunar Exploration Neutron Detector (LEND) for NASA Lunar Reconnaissance Orbiter | 1 |
| 16 | Constraints on the Distribution of Hydrogen in the Polar Regions of Mars and Implications for Ice Formation Processes | 3 |
| 17 | The Composition of 433 Eros: A Mineralogical-Chemical Synthesis | 2 |
| 18 | The X-Ray/Gamma-Ray Spectrometer for the NEAR Mission | 1 |
| 19 | Determination of elemental composition in geochemical exploration using a 14-MeV neutron generator | 4 |
| 20 | Analytical methods in determining elemental composition from the Apollo X-ray and gamma-ray spectrometer data. | 4 |
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.