Hsiu-Shan Yu
About
In The Last Decade
Hsiu-Shan Yu
26 papers receiving 368 citations
Peers
Comparison fields: 5 of 20
- Astronomy and Astrophysics 385
- Molecular Biology 117
- Artificial Intelligence 40
- Oceanography 27
- Atmospheric Science 18
Countries citing papers authored by Hsiu-Shan Yu
This map shows the geographic impact of Hsiu-Shan Yu'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 Hsiu-Shan Yu with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Hsiu-Shan Yu more than expected).
Fields of papers citing papers by Hsiu-Shan Yu
This network shows the impact of papers produced by Hsiu-Shan Yu. 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 Hsiu-Shan Yu. The network helps show where Hsiu-Shan Yu may publish in the future.
Co-authorship network of co-authors of Hsiu-Shan Yu
This figure shows the co-authorship network connecting the top 25 collaborators of Hsiu-Shan Yu. A scholar is included among the top collaborators of Hsiu-Shan Yu 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 Hsiu-Shan Yu. Hsiu-Shan Yu is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 15 | |
| 2 | 52 | |
| 3 | Bz Determinations and Forecasts Using UCSD Analysis Techniques | 1 |
| 4 | 14 | |
| 5 | 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 |
| 6 | The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network: Initial Results from the October 2016 Space-Weather Campaign | 1 |
| 7 | 40 | |
| 8 | Exploration of SOLIS and GONG Data Sets Using the UCSD ISEE IPS Time-Dependent Tomography and the CSSS Magnetic Field Model | 0 |
| 9 | 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 |
| 10 | A Statistical Study of the Radial and North-South Component Values of Heliospheric Magnetic Field | 1 |
| 11 | 6 | |
| 12 | 8 | |
| 13 | How Reliable Is the Prediction of Solar Wind Background | 2 |
| 14 | The first super geomagnetic storm of solar cycle 24: "The St. Patrick day (17 March 2015)" event | 2 |
| 15 | 84 | |
| 16 | 14 | |
| 17 | 3 | |
| 18 | 7 | |
| 19 | 1 | |
| 20 | The 3d Global Forecast of Inner Heliosphere Solar Wind Parameters from Remotely-Sensed IPS Data | 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.