C. Y. Fan
About
In The Last Decade
C. Y. Fan
112 papers receiving 1.8k citations
Peers
Comparison fields: 5 of 71
- Astronomy and Astrophysics 1.9k
- Nuclear and High Energy Physics 461
- Molecular Biology 334
- Atomic and Molecular Physics, and Optics 232
- Atmospheric Science 217
Countries citing papers authored by C. Y. Fan
This map shows the geographic impact of C. Y. Fan'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 C. Y. Fan with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. Y. Fan more than expected).
Fields of papers citing papers by C. Y. Fan
This network shows the impact of papers produced by C. Y. Fan. 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 C. Y. Fan. The network helps show where C. Y. Fan may publish in the future.
Co-authorship network of co-authors of C. Y. Fan
This figure shows the co-authorship network connecting the top 25 collaborators of C. Y. Fan. A scholar is included among the top collaborators of C. Y. Fan 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 C. Y. Fan. C. Y. Fan 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 | Interplanetary Dust Particle Isotopes and Raman Analysis | 0 |
| 3 | Suprathermal H(+) and He(2+) in the distant geomagnetic tail ISEE-3 observations | 3 |
| 4 | 11-year cycle solar modulation of cosmic ray intensity inferred from C-14 content variation in dated tree rings | 1 |
| 5 | Acceleration of particles in the magnetotail | 1 |
| 6 | Temporal variations of the anomalous oxygen /1974-1979/ and disappearance in 1978 | 2 |
| 7 | Composition and energy spectra of low energy ions observed upstream of the earth's bow shock on ISEE-1 | 5 |
| 8 | Recurrent energetic particle events associated with forward/reverse shock pairs near 4 AU in 1978 | 10 |
| 9 | The energy spectra of protons and alpha particles above 300 keV/nucleon during quiet times | 6 |
| 10 | Long Term Modulation of Cosmic-Ray Intensity and Solar Activity Cycle | 8 |
| 11 | Abundances, charge states, and energy spectra of helium and heavy ions during solar particle events | 1 |
| 12 | Heavy Particle Emission of Unusual Composition from the Sun | 2 |
| 13 | The Primary Cosmic Ray Spectrum From 2 x 10 11 eV to 10 15 eV. | 0 |
| 14 | Protons Associated with Centers of Solar Activity and their Propagation in Interplanetary Magnetic Field Regions Co-rotating with the Sun. | 2 |
| 15 | Protons and helium nuclei within interplanetary magnetic regions which co-rotate with the sun. | 20 |
| 16 | Acceleration of particles in the earth's shock transition region and beyond. | 3 |
| 17 | Solar Modulation of the Galactic Helium Spectrum Above 30 Mev Per Nucleon | 2 |
| 18 | DYNAMICS OF THE OUTER RADIATION BELT | 2 |
| 19 | The Equatorial Pitch Angle Distributions of Electrons in the Outer Radiation Belt | 3 |
| 20 | TRAPPED AND COSMIC RADIATION MEASUREMENTS FROM EXPLORER VI | 7 |
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.