activity
20172021
most citedIncrease in the amplitude of line-of-sight velocities of the small-scale motions in a solar filament before eruption

15 citations · 39 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2021

Small-scale Turbulent Motion of the Plasma in a Solar Filament as the Precursor of Eruption

Daikichi Seki, Kenichi Otsuji, Hiroaki Isobe +5

A filament, a dense cool plasma supported by the magnetic fields in the solar corona, often becomes unstable and erupts. It is empirically known that the filament often demonstrate…

astro-ph.SR202114 cited

Relationship between three-dimensional velocity of filament eruptions and CME association

Daikichi Seki, Kenichi Otsuji, Takako T. Ishii +2

It is widely recognised that filament disappearances or eruptions are frequently associated with Coronal Mass Ejections (CMEs). Since CMEs are a major source of disturbances of the…

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.SR201910 cited

Small-scale motions in solar filaments as the precursors of eruptions

Daikichi Seki, Kenichi Otsuji, Hiroaki Isobe +3

Filaments, the dense cooler plasma floating in the solar corona supported by magnetic fields, generally exhibit certain activations before they erupt. In our previous study (Seki e…

astro-ph.SR2018

Space Weather Prediction from the Ground: Case of CHAIN

Daikichi Seki, Satoru Ueno, Hiroaki Isobe +5

In this article, we insist on the importance and the challenges of the prediction of solar eruptive phenomena including flares, coronal mass ejections (CME), and filament eruptions…

astro-ph.SR201715 cited

Increase in the amplitude of line-of-sight velocities of the small-scale motions in a solar filament before eruption

Daikichi Seki, Kenichi Otsuji, Hiroaki Isobe +3

We present a study on the evolution of the small scale velocity field in a solar filament as it approaches to the eruption. The observation was carried out by the Solar Dynamics Do…