M. Kojima

How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation (2008)

Fujiki, K., Kojima, M., Tokumaru, M., Ohmi, T., Yokobe, A., Hayashi, K., ...

Observations from the second Ulysses fast latitude scan show that the global structure of solar wind near solar maximum is much more complex than at solar minimum. Soon after solar maximum, Ulysses...

How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation (2008)

Fujiki, K., Kojima, M., Tokumaru, M., Ohmi, T., Yokobe, A., Hayashi, K., ...

Observations from the second Ulysses fast latitude scan show that the global structure of solar wind near solar maximum is much more complex than at solar minimum. Soon after solar maximum, Ulysses...

Tracking heliospheric disturbances by interplanetary scintillation (2008)

Tokumaru, M., Kojima, M., Fujiki, K., Yamashita, M.

Coronal mass ejections are known as a solar cause of significant geospace disturbances, and a fuller elucidation of their physical properties and propagation dynamics is needed for space weather...

Nanoviridae (2005)

Vetten, H. J., Chu, P. W. G., Dale, J. L., Harding, R., Hu, J., Katul, L., ...