D. O. Muhleman
About
In The Last Decade
D. O. Muhleman
130 papers receiving 3.5k citations
Hit Papers
Peers
Comparison fields: 5 of 92
- Astronomy and Astrophysics 3.5k
- Atmospheric Science 1.3k
- Aerospace Engineering 626
- Global and Planetary Change 347
- Statistical and Nonlinear Physics 185
Countries citing papers authored by D. O. Muhleman
This map shows the geographic impact of D. O. Muhleman'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. O. Muhleman with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. O. Muhleman more than expected).
Fields of papers citing papers by D. O. Muhleman
This network shows the impact of papers produced by D. O. Muhleman. 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. O. Muhleman. The network helps show where D. O. Muhleman may publish in the future.
Co-authorship network of co-authors of D. O. Muhleman
This figure shows the co-authorship network connecting the top 25 collaborators of D. O. Muhleman. A scholar is included among the top collaborators of D. O. Muhleman 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. O. Muhleman. D. O. Muhleman is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | Reflected Signal Analysis and Surface Albedo in the Mars Orbiter Laser Altimeter (MOLA) Investigation | 1 |
| 2 | MOLA: The Future of Mars Global Cartography | 3 |
| 3 | Martian Polar Regions: 3.5-cm Radar Images | 1 |
| 4 | Microwave Imaging of Jupiter's Troposphere During Impact with Comet P/Shoemaker-Levy 9 | 4 |
| 5 | VLA/Goldstone 3.5-cm Radar Observations of Mercury in 1994: South Polar and Other Results | 3 |
| 6 | Titan's Radar Reflectivity and Rotation | 4 |
| 7 | A Cold, Dry, Cloudy, Dust-free Mars Atmosphere in the 1990's | 1 |
| 8 | The Surface of Titan and Titan's Rotation: What is Radar Telling Us? | 9 |
| 9 | Observations of Titan's Radio Light-Curve at 3. 5 cm | 5 |
| 10 | VLA/Goldstone Planetary Radar results. | 1 |
| 11 | Radar and Radio Observations of Titan | 2 |
| 12 | High Spatial and Spectral Resolution of the 115 GHz CO Line on Venus | 2 |
| 13 | VLA Polarization Measurements of Ganymede and Callisto | 1 |
| 14 | Spatial Resolution of the CO J=0-->1 Line on Venus | 1 |
| 15 | Microwave spectroscopy and radiometry of Saturn and Titan. | 1 |
| 16 | Microwave Emission from Titan and the Galilean Satellites | 1 |
| 17 | The Longitudinal Variation of the Thermal Inertia and of the 2. 8 cm Brightness Temperature of Mars. | 3 |
| 18 | The CO Distribution in the Atmosphere of Venus from 230 Ghz Spectral Measurements. | 3 |
| 19 | A Radio Synthesis Map of the Saturn System at a Wavelength of 3.71 cm | 6 |
| 20 | Orientation-Dependence of the Evolution of Long-Period Comet Orbits | 1 |
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.