activity
20072020
most citedMultiple Plasmoid Ejections and Associated Hard X-ray Bursts in the 2000 November 24 Flare

60 citations · 309 across the 10 of their papers we have counts for

collaborators

13 papers

astro-ph.SR202018 cited

Statistical Analysis of the Relation between Coronal Mass Ejections and Solar Energetic Particles

Kosuke Kihara, Yuwei Huang, Nobuhiko Nishimura +4

To improve the forecasting capability of impactful solar energetic particle (SEP) events, the relation between coronal mass ejections (CMEs) and SEP events needs to be better under…

astro-ph.SR2020

SMART/SDDI Filament Disappearance Catalogue

Daikichi Seki, Kenichi Otsuji, Takako T. Ishii +8

This paper describes a new SMART/SDDI Filament Disappearance Catalogue, in which we listed almost all the filament disappearance events that the Solar Dynamics Doppler Imager (SDDI…

astro-ph.SR2019

Dynamic Processes of the Moreton Wave on 2014 March 29

Denis P. Cabezas, Ayumi Asai, Kiyoshi Ichimoto +4

On 2014 March 29, an intense solar flare classified as X1.0 occurred in the active region 12017. Several associated phenomena accompanied this event, among them a fast-filament eru…

astro-ph.SR20171 cited

Statistical Studies of Solar White-Light Flares and Comparisons with Superflares on Solar-type Stars

Kosuke Namekata, Takahito Sakaue, Kyoko Watanabe +9

Recently, many superflares on solar-type stars have been discovered as white-light flares (WLFs). The statistical study found a correlation between their energies () and duratio…

astro-ph.SR201712 cited

Observational Study on the Fine Structure and Dynamics of a Solar Jet. II. Energy Release Process Revealed by Spectral Analysis

Takahito Sakaue, Akiko Tei, Ayumi Asai +3

We report a solar jet phenomenon associated with the C5.4 class flare on 2014 November 11. The data of jet was provided by Solar Dynamics Observatory (SDO), X-Ray Telescope (XRT) a…

astro-ph.SR201716 cited

Variation of Solar Microwave Spectrum in the Last Half Century

M. Shimojo, K. Iwai, A. Asai +3

The total solar fluxes at 1, 2, 3.75, and 9.4 GHz were observed continuously from 1957 to 1994 at Toyokawa, and from 1994 until now at Nobeyama, Japan with the current Nobeyama Rad…