This map shows the geographic impact of Harushi Ueno'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 Harushi Ueno with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Harushi Ueno more than expected).
This network shows the impact of papers produced by Harushi Ueno. 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 Harushi Ueno. The network helps show where Harushi Ueno may publish in the future.
Co-authorship network of co-authors of Harushi Ueno
This figure shows the co-authorship network connecting the top 25 collaborators of Harushi Ueno.
A scholar is included among the top collaborators of Harushi Ueno 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 Harushi Ueno. Harushi Ueno is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Yasue, S., K. Munakata, S. Mori, et al.. (1995). Observation of the First-Three Harmonics of Cosmic-Ray Daily Intensity Variations and the Magnetic Polarity of the Heliosphere. International Cosmic Ray Conference. 4. 615.1 indexed citations
10.
Fujii, Z. & Harushi Ueno. (1990). Long-Term Change in the Cosmic Ray Diurnal Variation. International Cosmic Ray Conference. 6. 314.2 indexed citations
11.
Murakami, K., T. Yamada, S. Sakakibara, et al.. (1990). Sidereal Anisotropy of Cosmic Rays with Median Energy 70 TeV Observed at Liawenee, Tasmania. International Cosmic Ray Conference. 3. 177.2 indexed citations
12.
Fenton, A. G., K. B. Fenton, J. E. Humble, et al.. (1981). Cooperative Observations of Air Showers in Tasmania Looking for Anisotropies in 10(13) - 10(14) EV Primaries ( Coala Project ). International Cosmic Ray Conference. 4. 185.
13.
Ueno, Harushi, Z. Fujii, K. Fujimoto, S. Sakakibara, & K. Nagashima. (1981). Solar and sidereal daily variations observed at Sakashita underground station. International Cosmic Ray Conference. 10. 254–257.4 indexed citations
14.
Sakakibara, S., Harushi Ueno, K. Fujimoto, et al.. (1979). Anisotropy of Small Air Showers in the Galactic Arm. International Cosmic Ray Conference. 4. 216.1 indexed citations
15.
Fujimoto, K., K. Nagashima, Harushi Ueno, & I. Kondò. (1973). Three Dimensional Cosmic Ray Anisotropy in Interplanetary Space Responsible for Solar Semi-Diurnal Variation. International Cosmic Ray Conference. 2. 993.1 indexed citations
16.
Fujii, Z., K. Fujimoto, Harushi Ueno, I. Kondò, & K. Nagashima. (1970). SEMIDIURNAL ANISOTROPY OF COSMIC RADIATION.. International Cosmic Ray Conference. 2. 83.3 indexed citations
17.
Mori, S., et al.. (1963). Development of cosmic ray storms. International Cosmic Ray Conference. 2. 33.1 indexed citations
18.
Ueno, Harushi, et al.. (1963). A 27-day recurrence tendency in cosmic ray diurnal variation with inverse phase. International Cosmic Ray Conference. 2. 322.2 indexed citations
19.
Kamiya, Y., et al.. (1962). SHORT-TERM INCREASES OF THE COSMIC-RAY NUCLEI INTENSITY ASSOCIATED WITH THE SOLAR ACTIVITY. Journal of the Physical Society of Japan. 17. 315.7 indexed citations
20.
Kondò, I., et al.. (1960). OBSERVATION OF THE POINT SOURCE OF COSMIC RAYS. Journal of the Physical Society of Japan. 17. 131.6 indexed citations
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.