F. M. Ipavich
About
In The Last Decade
F. M. Ipavich
176 papers receiving 4.7k citations
Peers
Comparison fields: 5 of 49
- Astronomy and Astrophysics 5.6k
- Molecular Biology 1.1k
- Nuclear and High Energy Physics 949
- Geophysics 840
- Atmospheric Science 241
Countries citing papers authored by F. M. Ipavich
This map shows the geographic impact of F. M. Ipavich'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. M. Ipavich with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites F. M. Ipavich more than expected).
Fields of papers citing papers by F. M. Ipavich
This network shows the impact of papers produced by F. M. Ipavich. 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. M. Ipavich. The network helps show where F. M. Ipavich may publish in the future.
Co-authorship network of co-authors of F. M. Ipavich
This figure shows the co-authorship network connecting the top 25 collaborators of F. M. Ipavich. A scholar is included among the top collaborators of F. M. Ipavich 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. M. Ipavich. F. M. Ipavich is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | Measurement of the Ar/Ca Abundance Ratio From CELIAS/MTOF in Slow and Fast Solar Wind | 1 |
| 2 | On the variability of suprathermal He + ions at 1 AU | 1 |
| 3 | The Influence of Suprathermal Electrons on the Derivation of Coronal Electron Temperatures from Solar Wind Motor Ion Charge States | 4 |
| 4 | The iron, silicon, and oxygen abundance in the solar wind measured with SOHO/CELIAS/MTOF | 3 |
| 5 | A Method for Estimating the Solar Wind H + Contribution to Magnetospheric Plasma | 3 |
| 6 | Origin, transport, and losses of energetic He(+) and He(2+) ions in the magnetosphere of the Earth - AMPTE/CCE observations | 11 |
| 7 | Charge State Distributions of Solar Wind Carbon, Oxygen, and Iron Ions | 0 |
| 8 | Calculation of the Flow Speed of Shock-Accelerated Energetic Particle Distributions, and its Application in Studying the November 12, 1978 Interplanetary Shock Event | 2 |
| 9 | Energetic N + ions in the magnetosphere. | 1 |
| 10 | Magnetospheric ions and electrons in the distant magnetosheath at about 50 and 180 earth radii - ISEE-3 observations | 1 |
| 11 | Energetic (greater than 100 keV) O(+) ions in the plasma sheet | 2 |
| 12 | 27 | |
| 13 | Ionization states of helium in He-3-rich solar energetic particle events | 1 |
| 14 | Suprathermal H(+) and He(2+) in the distant geomagnetic tail ISEE-3 observations | 3 |
| 15 | Direct Determination of the Ionic Charge Distribution of Heavy Ions in Fe-Rich Solar Energetic Particle Events | 1 |
| 16 | Distribution function representation of energy spectra of H, He, C, O and Fe in corotating particle streams | 9 |
| 17 | Temporal variations of the anomalous oxygen /1974-1979/ and disappearance in 1978 | 2 |
| 18 | Composition and energy spectra of low energy ions observed upstream of the earth's bow shock on ISEE-1 | 5 |
| 19 | Analysis of the 31 Oct. 1972 Interplanetary Shock Wave and Associated Unusual Phenomena | 4 |
| 20 | Observations of < 1 MeV/Nuc Protons and Ions During the September 1974 Series of Flares | 2 |
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.