activity
20082023
most citedChromospheric Anemone Jets as Evidence of Ubiquitous Reconnection

436 citations · 628 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.IM2023★ 3 cited

Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release

Amir Caspi, Daniel B. Seaton, Roberto Casini +12

The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poo…

astro-ph.SR2023★ 7 cited

Magnetic Field of Solar Dark Filaments Obtained from He I 10830 Angstrom Spectro-polarimetric Observation

Daiki Yamasaki, Yu Wei Huang, Yuki Hashimoto +4

Solar filaments are dense and cool plasma clouds in the solar corona. They are supposed to be supported in a dip of coronal magnetic field. However, the models are still under argu…

astro-ph.SR2022★ 14 cited

Study of Time Evolution of Thermal and Non-Thermal Emission from an M-Class Solar Flare

Shunsaku Nagasawa, Tomoko Kawate, Noriyuki Narukage +3

We conduct a wide-band X-ray spectral analysis in the energy range of 1.5-100 keV to study the time evolution of the M7.6 class flare of 2016 July 23, with the Miniature X-ray Sola…

astro-ph.SR2020★ 11 cited

Nowcast of an EUV dynamic spectrum during solar flares

Toshiki Kawai, Shinsuke Imada, Shohei Nishimoto +2

In addition to X-rays, extreme ultraviolet (EUV) rays radiated from solar flares can cause serious problems, such as communication failures and satellite drag. Therefore, methods f…

astro-ph.SR2019★ 21 cited

Estimating the temperature and density of a spicule from 100 GHz data obtained with ALMA

Masumi Shimojo, Tomoko Kawate, Takenori J. Okamoto +6

We succeeded in observing two large spicules simultaneously with the Atacama Large Millimeter/submillimeter Array (ALMA), the Interface Region Imaging Spectrograph (IRIS), and the…

astro-ph.SR2019★ 4 cited

Infrequent Occurrence of Significant Linear Polarization in H Solar Flares

Tomoko Kawate, Yoichiro Hanaoka

We performed statistical and event studies of linear polarization in the H line during solar flares. The statistical study revealed that, among 71 H flares analyzed, includin…

astro-ph.SR2018★ 9 cited

Measurement of Vector Magnetic Field in a Flare kernel with a Spectropolarimetric Observation in He I 10830 A

Tetsu Anan, Takurou Yoneya, Kiyoshi Ichimoto +5

A flare kernel associated with a C4 class flare was observed in a spectral window including the He I triplet 10830 A and Si I 10827 A with a spectropolarimeter on the Domeless Sola…

astro-ph.SR2018★ 52 cited

Blue wing enhancement of the chromospheric Mg II h and k lines in a solar flare

Akiko Tei, Takahito Sakaue, Takenori J. Okamoto +6

We performed coordinated observations of AR 12205, which produced a C-class flare on 2014 November 11, with the Interface Region Imaging Spectrograph (IRIS) and the Domeless Solar…

astro-ph.SR2017★ 1 cited

White paper of the "soft X-ray imaging spectroscopy"

Noriyuki Narukage, Shin-nosuke Ishikawa, Tomoko Kawate +2

The solar corona is full of dynamic phenomena, e.g., solar flares, micro flares in active regions, jets in coronal holes and in the polar regions, X-ray bright points in quiet regi…

astro-ph.SR2017★ 1 cited

UV/EUV High-Throughput Spectroscopic Telescope: A Next Generation Solar Physics Mission white paper

S. Imada, T. Shimizu, T. Kawate +2

The origin of the activity in the solar corona is a long-standing problem in solar physics. Recent satellite observations, such as Hinode, Solar Dynamics Observatory (SDO), Interfa…

astro-ph.SR2016★ 23 cited

Observations and simulations of the Na I D1 line profiles in an M-class solar flare

D. Kuridze, M. Mathioudakis, D. J. Christian +7

We study the temporal evolution of the Na I D1 line profiles in the M3.9 flare SOL2014-06-11T21:03 UT, using high spectral resolution observations obtained with the IBIS instrument…

astro-ph.SR2013★ 2 cited

The Relationship Between EUV Nonthermal Line Broadening and High-energy Particle During Solar Flare

Tomoko Kawate, Shinsuke Imada

We have studied the relationship between the location of EUV nonthermal broadening and high-energy particles during the large flares by using EUV imaging spectrometer onboard {\it…

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.SR2010★ 26 cited

Spicule Dynamics over Plage Region

Tetsu Anan, Reizaburo Kitai, Tomoko Kawate +14

We studied spicular jets over a plage area and derived their dynamic characteristics using Hinode Solar Optical Telescope (SOT) high-resolution images. The target plage region was…

astro-ph.SR2009★ 14 cited

Multi-Wavelength Observation of Electron Acceleration in the 2006 December 13 Flare

T. Minoshima, S. Imada, T. Morimoto +8

We present a multi-wavelength observation of a solar flare occurring on 2006 December 13 with Hinode, RHESSI, and the Nobeyama Radio Observatory, to study the electron acceleration…

astro-ph2008★ 436 cited

Chromospheric Anemone Jets as Evidence of Ubiquitous Reconnection

Kazunari Shibata, Tahei Nakamura, Takuma Matsumoto +19

The heating of the solar chromosphere and corona is a long-standing puzzle in solar physics. Hinode observations show the ubiquitous presence of chromospheric anemone jets outside…