activity
20092026
most citedCharacteristic Dependence of Umbral Dots on their Magnetic Structure

38 citations · 71 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2026

Magnetic field diagnostics of a solar active region filament

Daiki Yamasaki, Yu Wei Huang, Yuki Hashimoto +2

We performed spectropolarimetric observations of an active region filament in He I 10830 angstrom and Si I 10827 angstrom lines to investigate its magnetic field structure. We carr…

astro-ph.SR2026

Detection of Doppler velocity differences between ions and neutrals in an erupting prominence

Yuwei Huang, Kiyoshi Ichimoto, Tetsu Anan

We performed a spectroscopic observation of an erupting prominence occurred on the solar limb on 2015 May 8th in He I 706.5 nm, O I 777.2 nm triplet and Ca II 849.8 nm lines to inv…

astro-ph.SR2024

A fast-filament eruption observed in the H spectral line. I. Imaging spectroscopy diagnostic

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

Context. Solar filament eruptions usually appear to occur in association with the sudden explosive release of magnetic energy accumulated in long-lived arched magnetic structures.…

astro-ph.SR2016★ 15 cited

Temporal evolution and spatial distribution of white-light flare kernels in a solar flare

Tomoko Kawate, Takako T. Ishii, Yoshikazu Nakatani +4

On 2011 September 6, we observed an X2.1-class flare in continuum and H with a frame rate of about 30~Hz. After processing images of the event by using a speckle-masking image r…

astro-ph.SR2014★ 14 cited

Diagnosis of Magnetic and Electric Fields of Chromospheric Jets through Spectropolarimetric Observations of HI Paschen Lines

Tetsu Anan, Roberto Casini, Kiyoshi Ichimoto

Magnetic fields govern the plasma dynamics in the outer layers of the solar atmosphere, and electric fields acting on neutral atoms that move across the magnetic field enable us to…

astro-ph.SR2011★ 4 cited

Center-to-Limb Variation of Radio Emissions from Thermal-Rich and Thermal-Poor Solar Flares

Tomoko Kawate, Ayumi Asai, Ichimoto Kiyoshi

A statistical analysis of radio flare events was performed by using the event list of Nobeyama Radioheliograph in 1996-2009. We examined center-to-limb variations of 17GHz and 34GH…

astro-ph.SR2009★ 38 cited

Characteristic Dependence of Umbral Dots on their Magnetic Structure

Hiroko Watanabe, Reizaburo Kitai, Kiyoshi Ichimoto

Umbral dots (UDs) were observed in a stable sunspot in NOAA 10944 by the Hinode Solar Optical Telescope on 2007 March 1. The observation program consisted of blue continuum images…