M. Tokumaru
About
In The Last Decade
M. Tokumaru
157 papers receiving 2.5k citations
Peers
Comparison fields: 5 of 51
- Astronomy and Astrophysics 2.5k
- Molecular Biology 480
- Atmospheric Science 264
- Oceanography 259
- Nuclear and High Energy Physics 199
Countries citing papers authored by M. Tokumaru
This map shows the geographic impact of M. Tokumaru'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. Tokumaru with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Tokumaru more than expected).
Fields of papers citing papers by M. Tokumaru
This network shows the impact of papers produced by M. Tokumaru. 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. Tokumaru. The network helps show where M. Tokumaru may publish in the future.
Co-authorship network of co-authors of M. Tokumaru
This figure shows the co-authorship network connecting the top 25 collaborators of M. Tokumaru. A scholar is included among the top collaborators of M. Tokumaru 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. Tokumaru. M. Tokumaru is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | A Ground-Based Heliospheric Observatory for Space Weather: The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network | 2 |
| 2 | Observations and Analyses of Heliospheric Faraday Rotation of a Coronal Mass Ejection (CME) Using the LOw Frequency ARray (LOFAR) and Space-Based Imaging Techniques | 1 |
| 3 | The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network October 2016 Observing Campaign: Initial WIPSS Data Analyses | 1 |
| 4 | The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network in support of Space-Weather Science and Forecasting | 1 |
| 5 | Exploration of SOLIS and GONG Data Sets Using the UCSD ISEE IPS Time-Dependent Tomography and the CSSS Magnetic Field Model | 0 |
| 6 | 27 | |
| 7 | 11 | |
| 8 | Solar and interplanetary signatures of declining of solar magnetic fields: Implications to the next solar cycle 25 | 1 |
| 9 | 29 | |
| 10 | Using Interplanetary Scintillation (IPS) For Space-Weather Forecasting | 1 |
| 11 | The 3d Global Forecast of Inner Heliosphere Solar Wind Parameters from Remotely-Sensed IPS Data | 1 |
| 12 | Three-Dimensional Solar Wind Structures Obtained with MHD Simulation Model Using Observation-Based Time-Varying Inner Boundary Map | 5 |
| 13 | Kinematical properties of interplanetary coronal mass ejections detected by interplanetary scintillation observations during the solar cycle 23 | 1 |
| 14 | 3-D Magnetic Field Geometry of the October 28, 2003 ICME: Comparison with SMEI White-Light Observations | 1 |
| 15 | Comparison of Solar Mass Ejection Imager (SMEI) White Light Observations with IPS Velocity | 1 |
| 16 | Three-dimensional structure of compound interplanetary transients associated with 27-28 May 2003 coronal mass ejections | 1 |
| 17 | Geometry of Interplanetary CME Deduced from Cosmic Rays | 1 |
| 18 | The Relation Between the Solar Wind Velocity and the Magnetic Conditions of Coronal Holes | 1 |
| 19 | 11 | |
| 20 | 8 |
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.