activity
20062022
most citedDevelopment of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations

33 citations · 72 across the 6 of their papers we have counts for

collaborators

5 papers

astro-ph.SR202028 cited

Validation of Coronal Mass Ejection Arrival-Time Forecasts by Magnetohydrodynamic Simulations based on Interplanetary Scintillation Observations

Kazumasa Iwai, Daikou Shiota, Munetoshi Tokumaru +3

Coronal mass ejections (CMEs) cause various disturbances of the space environment; therefore, forecasting their arrival time is very important. However, forecasting accuracy is hin…

astro-ph.SR201933 cited

Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations

Kazumasa Iwai, Daikou Shiota, Munetoshi Tokumaru +3

Coronal mass ejections (CMEs) cause disturbances in the environment of the Earth when they arrive at the Earth. However, the prediction of the arrival of CMEs still remains a chall…

astro-ph.SR20194 cited

Comparative Study of Microwave Polar Brightening, Coronal Holes, and Solar Wind Over the Solar Poles

Ken'ichi Fujiki, Kiyoto Shibasaki, Seiji Yashiro +3

We comparatively studied the long-term variation (1992-2017) in polar brightening observed with the Nobeyama Radioheliograph, the polar solar wind velocity with interplanetary scin…

physics.space-ph2017

The response of the terrestrial bow shock and magnetopause of the long term decline in solar polar fields

Madhusudan Ingale, P. Janardhan, K. Fujiki +2

The location of the terrestrial magnetopause (MP) and it's subsolar stand-off distance depends not only on the solar wind dynamic pressure and the interplanetary magnetic field (IM…

astro-ph2006

International Colloquium "Scattering and Scintillation in Radio Astronomy" was held on June 19-23, 2006 in Pushchino, Moscow region, Russia

V. I. Shishov, W. A. Coles, B. J. Rickett +52

Topics of the Colloquium: a) Interplanetary scintillation b) Interstellar scintillation c) Modeling and physical origin of the interplanetary and the interstellar plasma turbulence…