19 citations as recorded by crossref.

1. Non‐dipolar solar wind structure observed in the cycle 23/24 minimum M. Tokumaru et al. https://doi.org/10.1029/2009GL037461
2. Large-scale structure of solar wind and geomagnetic phenomena M. Olyak https://doi.org/10.1016/j.jastp.2012.06.011
3. Long‐term evolution in the global distribution of solar wind speed and density fluctuations during 1997–2009 M. Tokumaru et al. https://doi.org/10.1029/2011JA017379
4. Coronal Magnetic-Field Configuration Associated with Pseudostreamer and Slow Solar Wind M. Tokumaru & K. Fujiki https://doi.org/10.1007/s11207-024-02398-5
5. Relation Between Coronal Hole Areas and Solar Wind Speeds Derived from Interplanetary Scintillation Measurements M. Tokumaru et al. https://doi.org/10.1007/s11207-017-1066-7
6. Three-dimensional reconstruction of heliospheric structure using iterative tomography: A review B. Jackson et al. https://doi.org/10.1016/j.jastp.2010.10.007
7. Rarefaction of the Very Slow (<350 km/s) Solar Wind in Cycle 24 Compared With Cycle 23 M. Tokumaru et al. https://doi.org/10.1002/2017JA025014
8. BepiColombo Science Investigations During Cruise and Flybys at the Earth, Venus and Mercury V. Mangano et al. https://doi.org/10.1007/s11214-021-00797-9
9. Dynamics of Slow Solar Wind Emerging from an Equatorial Coronal Hole M. Asgari-Targhi & K. Fujiki https://doi.org/10.3847/1538-4357/ae3d99
10. A Study of an Equatorial Coronal Hole Observed at the First Parker Solar Probe Perihelion N. Karna et al. https://doi.org/10.3847/1538-4357/ac3c46
11. North‐south asymmetry in global distribution of the solar wind speed during 1985–2013 M. Tokumaru et al. https://doi.org/10.1002/2014JA020765
12. Optimization of Solar-Wind Speed Models Using Interplanetary Scintillation Observations M. Tokumaru et al. https://doi.org/10.1007/s11207-024-02356-1
13. A newly developed UHF radiotelescope for interplanetary scintillation observations: Solar Wind Imaging Facility M. Tokumaru et al. https://doi.org/10.1029/2011RS004694
14. SPECTRUM OF THE INTERPLANETARY PLASMA TURBULENCE AT A DISTANCE FROM THE SUN GREATER THAN 1 AU M. Olyak et al. https://doi.org/10.15407/rpra21.04.260
15. Solar cycle evolution of the solar wind speed distribution from 1985 to 2008 M. Tokumaru et al. https://doi.org/10.1029/2009JA014628
16. Heliolatitude and Time Variations of Solar Wind Structure from in situ Measurements and Interplanetary Scintillation Observations J. Sokół et al. https://doi.org/10.1007/s11207-012-9993-9
17. Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME B. Jackson et al. https://doi.org/10.1007/s11207-023-02169-8
18. Global Distribution of the Solar Wind Speed Reconstructed from Improved Tomographic Analysis of Interplanetary Scintillation Observations between 1985 and 2019 M. Tokumaru et al. https://doi.org/10.3847/1538-4357/ac1862
19. Comparative Study of Microwave Polar Brightening, Coronal Holes, and Solar Wind over the Solar Poles K. Fujiki et al. https://doi.org/10.1007/s11207-019-1418-6