P. M. Fry
About
In The Last Decade
P. M. Fry
70 papers receiving 1.2k citations
Peers
Comparison fields: 5 of 33
- Astronomy and Astrophysics 1.1k
- Atmospheric Science 520
- Molecular Biology 123
- Global and Planetary Change 110
- Spectroscopy 93
Countries citing papers authored by P. M. Fry
This map shows the geographic impact of P. M. Fry'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 P. M. Fry with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites P. M. Fry more than expected).
Fields of papers citing papers by P. M. Fry
This network shows the impact of papers produced by P. M. Fry. 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 P. M. Fry. The network helps show where P. M. Fry may publish in the future.
Co-authorship network of co-authors of P. M. Fry
This figure shows the co-authorship network connecting the top 25 collaborators of P. M. Fry. A scholar is included among the top collaborators of P. M. Fry 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 P. M. Fry. P. M. Fry is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 1 | |
| 2 | 0 | |
| 3 | 3 | |
| 4 | 10 | |
| 5 | 5 | |
| 6 | The Nature of South Polar Cloud Shadows and Anti-Shadows on Saturn | 1 |
| 7 | Using HST bandpass filter images from the OPAL program to test the ability of candidate chromophores to model spatial and temporal variations on Jupiter | 1 |
| 8 | Vertical Wind Shear in Neptune's Atmosphere Explained with a Modified Thermal Wind Equation | 0 |
| 9 | A New Dark Vortex | 0 |
| 10 | Computation of Concentric Shell Particle Scattering Effects in Jovian Clouds | 1 |
| 11 | Evidence for Ammonia and Water Ices as the Primary Components of Cloud Particles in Saturn's Great Storm of 2010-2011 | 2 |
| 12 | First Views of North Polar Clouds and Circulation on Uranus | 1 |
| 13 | Uranus High Signal-to-noise Ratio Near-IR Imaging: Recent Results | 1 |
| 14 | Implications of New Methane Absorption Coefficients on Uranus Vertical Structure Derived from Near-IR Spectra | 1 |
| 15 | Evidence for Widely Distributed Ammonia Ice on Jupiter | 1 |
| 16 | Uranus Cloud Layers As Constrained By HST STIS Spectra | 2 |
| 17 | Cloud structure on Uranus as constrained by near IR 1.1-1.8 micron spectra. | 1 |
| 18 | Keck 2 AO Observations of Neptune in 2003 and 2004. | 3 |
| 19 | HST Observations of Neptune in 2002 | 1 |
| 20 | The Phase Variation of Titan's Brightness Contrast: Implied Constraints on Properties of Haze Particles | 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.