P. Bochsler
About
In The Last Decade
P. Bochsler
179 papers receiving 3.3k citations
Peers
Comparison fields: 5 of 77
- Astronomy and Astrophysics 3.1k
- Atmospheric Science 393
- Atomic and Molecular Physics, and Optics 256
- Ecology 232
- Molecular Biology 226
Countries citing papers authored by P. Bochsler
This map shows the geographic impact of P. Bochsler'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. Bochsler with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites P. Bochsler more than expected).
Fields of papers citing papers by P. Bochsler
This network shows the impact of papers produced by P. Bochsler. 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. Bochsler. The network helps show where P. Bochsler may publish in the future.
Co-authorship network of co-authors of P. Bochsler
This figure shows the co-authorship network connecting the top 25 collaborators of P. Bochsler. A scholar is included among the top collaborators of P. Bochsler 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. Bochsler. P. Bochsler is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | A Possible Contribution from the Ancient Terrestrial Atmosphere to the Trapped Xenon Inventory of Lunar Soils | 1 |
| 2 | The Elemental Composition of Solar Wind with Implications for Fractionation Processes During Solar Wind Formation | 1 |
| 3 | Comparison of Solar Wind Noble Gas Data from Genesis with Apollo/SWC - New Results from Implantation Experiments | 4 |
| 4 | In Search of Solar Wind Nitrogen in Genesis Material: Further Analysis of a Gold Cross Arm of the Concentrator | 4 |
| 5 | Fractionation Processes in the Solar Wind Revealed by Noble Gases Collected by Genesis Regime Targets | 4 |
| 6 | Solar Wind Helium and Neon from Metallic Glass Flown on Genesis - Preliminary Bulk and Velocity-Dependent Data | 2 |
| 7 | Depth-dependant Fractionation of Light Solar Wind Noble Gases in a Genesis Target | 1 |
| 8 | Trapping and Release Data of Artificially Implanted Noble Gases into Metals -- Tests for Genesis Targets | 1 |
| 9 | Solar and Solar-Wind Oxygen Isotopes and the Genesis Mission | 1 |
| 10 | 14 | |
| 11 | Measurement of The Ion-induced Electron Yields From Thin Carbon Foils For Low-energy Ions | 0 |
| 12 | Measurement of the Ar/Ca Abundance Ratio From CELIAS/MTOF in Slow and Fast Solar Wind | 1 |
| 13 | Solar and Galactic Composition | 3 |
| 14 | 20 | |
| 15 | Solar Orbiter --- A High Resolution Mission to the Sun and Inner Heliosphere | 3 |
| 16 | The Influence of Suprathermal Electrons on the Derivation of Coronal Electron Temperatures from Solar Wind Motor Ion Charge States | 4 |
| 17 | The iron, silicon, and oxygen abundance in the solar wind measured with SOHO/CELIAS/MTOF | 3 |
| 18 | Modeling the evolution of N and 15 N/ 14 N in the lunar regolith: mixing models involving two components. | 1 |
| 19 | Interaction of solar wind ions with thin carbon foils - calibration of time-of-flight spectrometers. | 3 |
| 20 | Tritium in lunar material | 3 |
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.