activity
20062008
most citedEmergence of a Helical Flux Rope Under an Active Region Prominence

171 citations · 344 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph20084 cited

Numerical Study of a Propagating Non-Thermal Microwave Feature in a Solar Flare Loop

T. Minoshima, T. Yokoyama

We analytically and numerically study the motion of electrons along a magnetic loop, to compare with the observation of the propagating feature of the non-thermal microwave source…

astro-ph2008171 cited

Emergence of a Helical Flux Rope Under an Active Region Prominence

Takenori J. Okamoto, Saku Tsuneta, Bruce W. Lites +12

Continuous observations were obtained of active region 10953 with the Solar Optical Telescope (SOT) on board the \emph{Hinode} satellite during 2007 April 28 to May 9. A prominence…

astro-ph200739 cited

Comparative Analysis of Non-thermal Emissions and Study of Electron Transport in a Solar Flare

T. Minoshima, T. Yokoyama, N. Mitani

We study the non-thermal emissions in a solar flare occurring on 2003 May 29 by using RHESSI hard X-ray (HXR) and Nobeyama microwave observations. This flare shows several typical…

astro-ph200735 cited

Triggering Mechanism for the Filament Eruption on 2005 September 13 in Active Region NOAA 10808

Kaori Nagashima, Hiroaki Isobe, Takaaki Yokoyama +3

On 2005 September 13 a filament eruption accompanied by a halo CME occurred in the most flare-productive active region NOAA 10808 in Solar Cycle 23. Using multi-wavelength observat…

astro-ph200710 cited

The Origin of Ripples in Cool Cores of Galaxy Clusters: Heating by MHD Waves?

Yutaka Fujita, Takeru K. Suzuki, Takahiro Kudoh +1

We consider MHD waves as a heating source of cool cores of galaxy clusters. In particular, we focus on transverse waves (Alfven waves), because they can propagate a longer distance…

astro-ph200661 cited

Two-dimensional MHD simulations of relativistic magnetic reconnection

Naoyuki Watanabe, Takaaki Yokoyama

It has been recognized that magnetic reconnection process is of great importance in high-energy astrophysics. We develop a new two-dimensional relativistic resistive magnetohydrody…