M. A. Shea
About
In The Last Decade
M. A. Shea
273 papers receiving 8.0k citations
Hit Papers
Peers
Comparison fields: 5 of 161
- Molecular Biology 4.0k
- Astronomy and Astrophysics 3.7k
- Pulmonary and Respiratory Medicine 817
- Cardiology and Cardiovascular Medicine 688
- Nuclear and High Energy Physics 682
Countries citing papers authored by M. A. Shea
This map shows the geographic impact of M. A. Shea'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 M. A. Shea with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. A. Shea more than expected).
Fields of papers citing papers by M. A. Shea
This network shows the impact of papers produced by M. A. Shea. 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 M. A. Shea. The network helps show where M. A. Shea may publish in the future.
Co-authorship network of co-authors of M. A. Shea
This figure shows the co-authorship network connecting the top 25 collaborators of M. A. Shea. A scholar is included among the top collaborators of M. A. Shea 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 M. A. Shea. M. A. Shea is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 11 | |
| 2 | GLE and sub-GLE redefinition in the light of high-altitude polar neutron monitors | 78 |
| 3 | A Dynamic Pathway for Calcium-Independent Activation of CaMKII by Methionine Oxidation breakdown → | 881 |
| 4 | Significant Solar Proton Events For Five Solar Cycles (1954-2007) | 6 |
| 5 | Solar proton fluence for 31 solar cycles derived from nitrate enhancements in polar ice | 2 |
| 6 | The Seasonal Dependency of the NO(Y) Impulsive Precipitation Events in Arctic Polar Ice | 1 |
| 7 | Simulation of the solar proton dose observed during the STS-28 flight | 2 |
| 8 | 400 years of large fluence solar proton events | 11 |
| 9 | Cosmic Ray Asymptotic Directions for Chilean Neutron Monitors | 3 |
| 10 | A Relativistic Solar Proton Database for the Ground-level Enhancements of 1956-1984 | 1 |
| 11 | The Effect of Local Time Dependence on the Observation of an Anisotropic Solar Cosmic Ray Flux by Aircraft | 1 |
| 12 | Solar Cosmic Rays on 29 September 1989; An Analysis using the World-Wide Network of Cosmic Ray Stations | 9 |
| 13 | A Quarter of a Century of Relativistic Solar Cosmic Ray Events Recorded by the Oulu Neutron Monitor | 6 |
| 14 | The Evolution of the Anisotropy of Solar Neutron Decay Protons During the 19 October 1989 Solar Cosmic Ray Event | 3 |
| 15 | The Concept of Using the Deep River and Kerguelen Neutron Monitors as 'Flagship' Stations for Ground-Level Solar Cosmic Ray Events | 2 |
| 16 | On the latitude dependence of cosmic ray cutoff rigidity variations during the initial phase of a geomagnetic storm | 5 |
| 17 | Cosmic Ray Access to Satellites from Large Zenith Angles | 1 |
| 18 | Cosmic ray access to earth satellites from below-horizon directions | 3 |
| 19 | PPS76: A computerized event mode solar proton forecasting technique | 15 |
| 20 | Vertical Cutoff Rigidity and the Intensity Distribution of Cosmic Rays Near Cape Town | 1 |
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.