Search Results - "Kawate, Tomoko"
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Validation of computed extreme ultraviolet emission spectra during solar flares
Published in Earth, planets, and space (25-03-2021)“…X-rays and extreme ultraviolet (EUV) emissions from solar flares rapidly change the physical composition of the Earth’s thermosphere and ionosphere, thereby…”
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Study of Time Evolution of Thermal and Nonthermal Emission from an M-class Solar Flare
Published in The Astrophysical journal (01-07-2022)“…Abstract 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,…”
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Statistical and Observational Research on Solar Flare EUV Spectra and Geometrical Features
Published in The Astrophysical journal (01-11-2020)“…Abstract We performed statistical analysis on the flare emission data to examine parameters related to the flare extreme-ultraviolet (EUV) spectra. This study…”
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Nowcast of an EUV dynamic spectrum during solar flares
Published in Journal of atmospheric and solar-terrestrial physics (01-09-2020)“…In addition to X-rays, extreme ultraviolet (EUV) rays radiated from solar flares can cause serious problems, such as communication failures and satellite drag…”
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Blue-wing enhancement of the chromospheric Mg ii h and k lines in a solar flare
Published in Publications of the Astronomical Society of Japan (01-12-2018)“…Abstract We performed coordinated observations of AR 12205, which showed a C-class flare on 2014 November 11, with the Interface Region Imaging Spectrograph…”
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Observation of tungsten emission spectra up to W46+ ions in the Large Helical Device and contribution to the study of high-Z impurity transport in fusion plasmas
Published in Nuclear fusion (01-10-2024)“…Spectroscopic studies of emissions released from tungsten ions combined with a pellet injection technique have been conducted in Large Helical Device for…”
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Statistical analysis for EUV dynamic spectra and their impact on the ionosphere during solar flares
Published in Earth, planets, and space (01-12-2023)“…The X-rays and extreme ultraviolet (EUV) emitted during solar flares can rapidly change the physical composition of Earth’s ionosphere, causing space weather…”
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Model-based reproduction and validation of the total spectra of a solar flare and their impact on the global environment at the X9.3 event of September 6, 2017
Published in Earth, planets, and space (20-04-2021)“…We attempted to reproduce the total electron content (TEC) variation in the Earth's atmosphere from the temporal variation of the solar flare spectrum of the…”
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Chromospheric Anemone Jets as Evidence of Ubiquitous Reconnection
Published in Science (American Association for the Advancement of Science) (07-12-2007)“…The heating of the solar chromosphere and corona is a long-standing puzzle in solar physics. Hinode observations show the ubiquitous presence of chromospheric…”
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Better Understanding of Hydrogen Pellet Ablation Cloud Spectra through the Occupation Probability Formalism in LHD
Published in Atoms (01-01-2024)“…We have recently incorporated the occupation probability formalism (OPF) in the simulation model [C. Stehlé and S. Jacquemot, Astron. Astrophys. 271, 348…”
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EUV/VUV Spectroscopy for the Study of Carbon Impurity Transport in Hydrogen and Deuterium Plasmas in the Edge Stochastic Magnetic Field Layer of Large Helical Device
Published in Plasma (01-06-2023)“…The ergodic layer in the Large Helical Device (LHD) consists of stochastic magnetic fields exhibiting a three-dimensional structure that is intrinsically…”
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Infrared spectro-polarimeter on the Solar Flare Telescope at NAOJ/Mitaka
Published in Publications of the Astronomical Society of Japan (01-08-2018)“…Abstract An infrared spectro-polarimeter installed on the Solar Flare Telescope at the Mitaka headquarters of the National Astronomical Observatory of Japan is…”
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Simultaneous Observation of Tungsten Spectra of W0 to W46+ Ions in Visible, VUV and EUV Wavelength Ranges in the Large Helical Device
Published in Atoms (17-09-2021)“…Spectroscopic studies for emissions released from tungsten ions have been conducted in the Large Helical Device (LHD) for contribution to the tungsten…”
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14
NIFS Atomic and Molecular Numerical Database for Collision Processes
Published in Atoms (09-10-2020)“…The National Institute for Fusion Science (NIFS) has compiled and developed atomic and molecular numerical databases for various collision processes and makes…”
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Evaluation of Fe XIV Intensity Ratio for Electron Density Diagnostics by Laboratory Measurements
Published in Atoms (30-08-2021)“…The intensity ratio of Fe XIV 264.765A/274.203A is useful to determine the electron density of solar corona, and the relationship between the electron density…”
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Center-to-Limb Variation of Radio Emissions from Thermal-Rich and Thermal-Poor Solar Flares
Published in Publications of the Astronomical Society of Japan (25-12-2011)“…A statistical analysis of radio flare events was conducted by using the event list of Nobeyama Radioheliograph in the years 1996–2009. We examined…”
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Internal Fine Structure of Ellerman Bombs
Published in Publications of the Astronomical Society of Japan (25-08-2010)“…We conducted coordinated observations of Ellerman bombs (EBs) between Hinode Satellite and Hida Observatory (HOP12). Ca II H broad-band filter images of NOAA…”
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Spicule Dynamics over a Plage Region
Published in Publications of the Astronomical Society of Japan (25-08-2010)“…We studied spicular jets over a plage area and derived their dynamic characteristics using Hinode Solar Optical Telescope (SOT) high-resolution images. A…”
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Infrequent Occurrence of Significant Linear Polarization in H Solar Flares
Published in The Astrophysical journal (12-02-2019)“…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…”
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High-Speed Imaging System for Solar-Flare Research at Hida Observatory
Published in Publications of the Astronomical Society of Japan (25-04-2013)“…A high-speed imaging system for observing solar flares in the continuum and H $ \alpha$ wavelengths was installed on a $ \phi$ 25 cm telescope of the Solar…”
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