B. V. Jackson
About
In The Last Decade
B. V. Jackson
170 papers receiving 2.7k citations
Peers
Comparison fields: 5 of 55
- Astronomy and Astrophysics 2.8k
- Molecular Biology 581
- Oceanography 204
- Artificial Intelligence 127
- Atmospheric Science 110
Countries citing papers authored by B. V. Jackson
This map shows the geographic impact of B. V. Jackson'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 B. V. Jackson with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. V. Jackson more than expected).
Fields of papers citing papers by B. V. Jackson
This network shows the impact of papers produced by B. V. Jackson. 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 B. V. Jackson. The network helps show where B. V. Jackson may publish in the future.
Co-authorship network of co-authors of B. V. Jackson
This figure shows the co-authorship network connecting the top 25 collaborators of B. V. Jackson. A scholar is included among the top collaborators of B. V. Jackson 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 B. V. Jackson. B. V. Jackson is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 44 | |
| 2 | Bz Determinations and Forecasts Using UCSD Analysis Techniques | 1 |
| 3 | 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 |
| 4 | 40 | |
| 5 | The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network in support of Space-Weather Science and Forecasting | 1 |
| 6 | Exploration of SOLIS and GONG Data Sets Using the UCSD ISEE IPS Time-Dependent Tomography and the CSSS Magnetic Field Model | 0 |
| 7 | Incorporation of MEXART Interplanetary Scintillation (IPS) Data into the UCSD 3-D Tomography as Part of the Worldwide IPS Stations (WIPSS) Initiative: Enhancing Space Weather Science and Forecasting | 1 |
| 8 | How Reliable Is the Prediction of Solar Wind Background | 2 |
| 9 | Using Interplanetary Scintillation (IPS) For Space-Weather Forecasting | 1 |
| 10 | The 3d Global Forecast of Inner Heliosphere Solar Wind Parameters from Remotely-Sensed IPS Data | 1 |
| 11 | CMEs In The Heliosphere Observed With Combined Imaging And In-situ Data From LASCO, Stereo And SMEI | 1 |
| 12 | Numerical Simulations of Solar Wind Disturbances by Coupled Models | 3 |
| 13 | 3-D Magnetic Field Geometry of the October 28, 2003 ICME: Comparison with SMEI White-Light Observations | 1 |
| 14 | An Empirical Description of Zodiacal Light as Measured by SMEI | 4 |
| 15 | The Evolution of Comets in the Heliosphere as Observed by SMEI | 2 |
| 16 | Power System for the Herschel & Planck Spacecraft | 1 |
| 17 | Heliospheric Photometric Images and 3D Reconstruction from the Solar Mass Ejection Imager (SMEI) Data | 1 |
| 18 | Three-dimensional structure of compound interplanetary transients associated with 27-28 May 2003 coronal mass ejections | 1 |
| 19 | Space Weather Using Remote Sensing Data | 1 |
| 20 | A Space-Borne Near-Earth Asteroid Detection System | 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.