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Yoshiaki Kato

Researcher at University of Oslo

Publications -  12
Citations -  1019

Yoshiaki Kato is an academic researcher from University of Oslo. The author has contributed to research in topics: Chromosphere & Photosphere. The author has an hindex of 11, co-authored 12 publications receiving 955 citations. Previous affiliations of Yoshiaki Kato include Japan Aerospace Exploration Agency & Chiba University.

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The Solar Optical Telescope of Solar-B (Hinode): The Optical Telescope Assembly

TL;DR: The solar optical telescope (SOT) as mentioned in this paper was designed to perform high-precision photometric and polarimetric observations of the Sun in visible light spectra (388 − 668 nm) with a spatial resolution of 0.2 - 0.3 arcsec.
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Solar science with the Atacama Large Millimeter/submillimeter Array - A new view of our Sun

TL;DR: The Atacama Large Millimeter/submillimeter Array (ALMA) as discussed by the authors is a powerful tool for observing the Sun at high spatial, temporal, and spectral resolution, which can address a broad range of fundamental scientific questions in solar physics.
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Solar Science with the Atacama Large Millimeter/Submillimeter Array—A New View of Our Sun

TL;DR: The Atacama Large Millimeter/submillimeter Array (ALMA) as mentioned in this paper is a powerful tool for observing the Sun at high spatial, temporal, and spectral resolution, which can address a broad range of fundamental scientific questions in solar physics.
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Saturation of Stellar Winds from Young Suns

TL;DR: In this article, the authors investigated mass losses via stellar winds from Sun-like main-sequence stars with a wide range of activity levels, and derived a Reimers-type scaling relation that estimates the mass-loss rate from an energetics consideration of their simulations.
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Excitation of slow modes in network magnetic elements through magnetic pumping

TL;DR: In this article, the authors found that the convective downdrafts in the immediate surroundings of magnetic elements are responsible for the excitation of slow modes in the solar atmosphere, and proposed an observational detection of this process.