F. Capaccioni
About
In The Last Decade
F. Capaccioni
204 papers receiving 2.4k citations
Peers
Comparison fields: 5 of 70
- Astronomy and Astrophysics 2.3k
- Ecology 579
- Atmospheric Science 474
- Aerospace Engineering 306
- Geophysics 303
Countries citing papers authored by F. Capaccioni
This map shows the geographic impact of F. Capaccioni'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 F. Capaccioni with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites F. Capaccioni more than expected).
Fields of papers citing papers by F. Capaccioni
This network shows the impact of papers produced by F. Capaccioni. 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 F. Capaccioni. The network helps show where F. Capaccioni may publish in the future.
Co-authorship network of co-authors of F. Capaccioni
This figure shows the co-authorship network connecting the top 25 collaborators of F. Capaccioni. A scholar is included among the top collaborators of F. Capaccioni 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 F. Capaccioni. F. Capaccioni is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 29 | |
| 2 | 11 | |
| 3 | The outburst sequence of 67/P on 2015 September 13 as seen by VIRTIS/Rosetta | 1 |
| 4 | SIMBIO-SYS for BepiColombo: status and issues. | 2 |
| 5 | Comet 67P: Thermal Maps and Local Properties as Derived from Rosetta/VIRTIS data | 1 |
| 6 | Investigations of 67/P-CG surfaces thermal properties at Southern latitudes and variations with heliocentric distances with VIRTIS/Rosetta | 1 |
| 7 | Global Resolved Temperature Maps of Vesta | 2 |
| 8 | Retrieval of Disk-Resolved Phase Functions of Vesta and Comparison with Other Asteroids | 1 |
| 9 | Testing the Hapke model by means of Montecarlo ray-tracing | 1 |
| 10 | Calibration of Spectral Indexes Suitable for Olivine Detection on Vesta | 3 |
| 11 | Olivine on Vesta: clues for the interior | 1 |
| 12 | Mineralogical Composition of the Different Types of Bright Deposits on Vesta | 1 |
| 13 | A Montecarlo routine to simulate scattering in particulate media | 1 |
| 14 | Dawn Observations of Marcia Crater, Vesta | 1 |
| 15 | VIMS Observations of Saturn’s Rings Investigated by means of Montecarlo Ray Tracing | 1 |
| 16 | VIS-IR spectrograms of Saturn's rings retrieved from Cassini-VIMS radial mosaics | 2 |
| 17 | Performances of the Data Compression and Binning Algorithms adopted on the VIRTIS-M Spectrometer onboard Rosetta | 1 |
| 18 | Spectrophotometric analysis of Rhea surface scattering properties | 1 |
| 19 | The Martian Atmosphere as Observed by VIRTIS-M on Rosetta Spacecraft | 1 |
| 20 | Laboratory simulation of asteroid lightcurves from fragments obtained from hypervelocity impacts | 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.