K. R. Pyle
Impact in
- Astronomy and Astrophysics top 2%
- Solar and Space Plasma Dynamics
- Ionosphere and magnetosphere dynamics
- Astro and Planetary Science
- Gamma-ray bursts and supernovae
- Stellar, planetary, and galactic studies
- Nuclear and High Energy Physics top 10%
- Astrophysics and Cosmic Phenomena
- Dark Matter and Cosmic Phenomena
Papers in
-
- Solar and Space Plasma Dynamics 55
- Ionosphere and magnetosphere dynamics 28
- Astro and Planetary Science 24
-
- Dark Matter and Cosmic Phenomena 14
- Astrophysics and Cosmic Phenomena 10
- Co-authors
- J. A. SimpsonR. B. McKibbenP. A. EvensonD. L. ChenetteP. MeyerM. García-MuñozA. J. TuzzolinoD. C. Hamilton
- Journals
- The Astrophysical Journal (11 papers)Journal of Geophysical Research Atmospheres (10 papers)Science (3 papers)Advances in Space Research (2 papers)IEEE Transactions on Nuclear Science (1 paper)
- Partner nations
- United StatesRussiaJapan
In The Last Decade
K. R. Pyle
63 papers receiving 984 citations
Peers
Comparison fields: 5 of 39
- Astronomy and Astrophysics 1.2k
- Nuclear and High Energy Physics 240
- Atmospheric Science 88
- Radiation 35
- Molecular Biology 222
Countries citing papers authored by K. R. Pyle
This map shows the geographic impact of K. R. Pyle'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 K. R. Pyle with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites K. R. Pyle more than expected).
Fields of papers citing papers by K. R. Pyle
This network shows the impact of papers produced by K. R. Pyle. 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 K. R. Pyle. The network helps show where K. R. Pyle may publish in the future.
Co-authorship network
The 25 scholars most cited alongside K. R. Pyle, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.
All Works
| # | Work | ||
|---|---|---|---|
| 1 | Simultaneous Observations of Solar Neutrons in Association with a Large Solar Flare on June 6, 1991 | 2003 | 1 |
| 2 | Neutron Monitor Sensitivity to Solar Modulation Changes: Altitude vs. Cutoff Rigidity | 1997 | 4 |
| 3 | The Isotopic Composition of Geomagnetically Trapped Helium | 1995 | 3 |
| 4 | 1994 | 16 | |
| 5 | The Haleakala Cosmic Ray Neutron Monitor Station: Intercalibration with the Huancayo Station | 1993 | 10 |
| 6 | Radial Gradients of Galactic Cosmic Rays and Anomalous Components in the Heliosphere Pioneer 10/11, Ulysses and IMP 8 Measurements | 1991 | 3 |
| 7 | The Dependence of Solar Modulation on the Sign of the Cosmic Ray Particle Charge during the 22-year Solar Magnetic Cycle | 1991 | 9 |
| 8 | Observation of a Direct Solar Neutron Event on 22 March 1991 with the Haleakala Hawaii, Neutron Monitor | 1991 | 8 |
| 9 | The Dependence of Solar Modulation on the Sign of the Cosmic Ray Particle Charge : Further Study of a 22 Year Solar Magnetic Cycle | 1987 | 6 |
| 10 | Proton, Helium and Electron Spectra from 1965 Through 1979 AS Tests of Modulation Theory | 1983 | 5 |
| 11 | Radial gradients of galactic cosmic rays measured by Pioneer 10 from 1-29 AU through the period of solar maximum | 1983 | 1 |
| 12 | Gradients of galactic cosmic rays and anomalous helium to more than 23 A.U. during the increase of solar modulation in 1978-80 | 1982 | 2 |
| 13 | The solar modulation of the anomalous helium component from 1965 to 1980 and from 1 to 23 A.U. | 1981 | 2 |
| 14 | Large-Scale Modulation of Galactic Cosmic Rays and Anomalous he Observed at ⩾ 16 AU with Pioneer 10 | 1979 | 11 |
| 15 | The radial intensity gradients for cosmic rays and the anomalous helium from Pioneer 10 and 11 | 1979 | 4 |
| 16 | Variations in the Intensity of Galactic Cosmic Rays and the Anomalous Helium as a Function of Solar Latitude | 1979 | 6 |
| 17 | Large-Scale Modulation of Galactic Cosmic Rays and Anomalous Helium Observed at ≥ 16 AU with Pioneer 10 | 1979 | 2 |
| 18 | Jupiter's Magnetosphere as a 'Point Source' for Electrons Propagating from 1 to 12 AU | 1978 | 2 |
| 19 | Cosmic Ray Intensity Gradients in the Outer Solar System Measured by Pioneer 10 and 11 | 1978 | 11 |
| 20 | Cosmic Ray Radial Intensity Gradients Measured by Pioneer 10 and 11 | 1975 | 2 |
About K. R. Pyle
K. R. Pyle is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics, Radiation, Atmospheric Science and Oceanography, having authored 65 papers that have together received 1.3k indexed citations. Recurring topics across this work include Solar and Space Plasma Dynamics (55 papers), Ionosphere and magnetosphere dynamics (28 papers), Astro and Planetary Science (24 papers), Dark Matter and Cosmic Phenomena (14 papers), Astrophysics and Cosmic Phenomena (10 papers), Atmospheric Ozone and Climate (8 papers), Solar Radiation and Photovoltaics (7 papers) and Nuclear Physics and Applications (6 papers). The work is most often cited by research in Astronomy and Astrophysics (1.2k citations), Nuclear and High Energy Physics (240 citations), Atmospheric Science (88 citations), Radiation (35 citations) and Molecular Biology (222 citations). K. R. Pyle has collaborated with scholars based in United States, Russia and Japan. Frequent co-authors include J. A. Simpson, R. B. McKibben, P. A. Evenson, D. L. Chenette, P. Meyer, M. García-Muñoz, A. J. Tuzzolino, D. C. Hamilton, T. S. Bastian and A. Mogro‐Campero. Their work appears in journals such as The Astrophysical Journal, Journal of Geophysical Research Atmospheres, Science, Advances in Space Research and IEEE Transactions on Nuclear Science.
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.