D. S. Draper
About
In The Last Decade
D. S. Draper
68 papers receiving 2.1k citations
Peers
Comparison fields: 5 of 57
- Geophysics 1.5k
- Astronomy and Astrophysics 1.0k
- Atmospheric Science 300
- Artificial Intelligence 239
- Ecology 154
Countries citing papers authored by D. S. Draper
This map shows the geographic impact of D. S. Draper'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. S. Draper with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. S. Draper more than expected).
Fields of papers citing papers by D. S. Draper
This network shows the impact of papers produced by D. S. Draper. 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. S. Draper. The network helps show where D. S. Draper may publish in the future.
Co-authorship network of co-authors of D. S. Draper
This figure shows the co-authorship network connecting the top 25 collaborators of D. S. Draper. A scholar is included among the top collaborators of D. S. Draper 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. S. Draper. D. S. Draper is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 13 | |
| 2 | The Inner SOlar System CHRONology (ISOCHRON) Discovery Mission: Returning Samples of the Youngest Lunar Mare Basalts | 1 |
| 3 | Origin of Olivine-Phyric Shergottites | 1 |
| 4 | 48th Lunar and Planetary Science Conference abstracts | 26 |
| 5 | Constraints on Mantle Plume Melting Conditions in the Martian Mantle Based on Improved Melting Phase Relationships of Olivine-Phyric Shergottite Yamato 980459 | 1 |
| 6 | Moonage Daydream: Reassessing the Simple Model for Lunar Magma Ocean Crystallization | 1 |
| 7 | Lunar and Planetary Science XLVI : abstracts presented at the 46th Lunar and Planetary Science Conference March 16-20, 2015 | 1 |
| 8 | Can Fractional Crystallization of a Lunar Magma Ocean Produce the Lunar Crust | 4 |
| 9 | Experimental Fractional Crystallization of the Lunar Magma Ocean | 4 |
| 10 | High Pressure Experiments Yield Insight into an Early Magma Ocean on Mars | 1 |
| 11 | Core/Mantle Partitioning of Chlorine and a New Estimate for the Hydrogen Abundance of Earth | 1 |
| 12 | Fundamental Importance of Returned Samples to Understanding the Martian Interior | 1 |
| 13 | An updated predictive model for garnet-melt trace element partitioning | 1 |
| 14 | High Pressure Melting of H-Chondrite: A Match for the Martian Basalt Source Mantle | 2 |
| 15 | Effect of Titanium on REE and HFSE Partitioning Between Garnet and Melt | 2 |
| 16 | Preliminary High Pressure Phase Relations of Apollo 15 Green C Glass: Assessment of the Role of Garnet | 3 |
| 17 | Melting in the Deep Lunar Mantle | 2 |
| 18 | A Petrological Model for the Origin of Martian Shergottite Magmas Based on Their Major Element, Trace Element, and Isotopic Compositions | 3 |
| 19 | Melting of Model Martian Mantle at High-Pressure: Implications for the Composition of the Martian Basalt Source Region | 0 |
| 20 | Merits of a Locality Sample for Accomplishing Mars Exploration Goals: The First Sample Return Mission | 0 |
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.