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Hiromitsu Ishibashi

Researcher at National Institute of Information and Communications Technology

Publications -  8
Citations -  68

Hiromitsu Ishibashi is an academic researcher from National Institute of Information and Communications Technology. The author has contributed to research in topics: Coronal mass ejection & Signal processing. The author has an hindex of 5, co-authored 8 publications receiving 56 citations.

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The 17 March 2015 storm: the associated magnetic flux rope structure and the storm development

TL;DR: In this paper, the authors determined the magnetic cloud (MC) structure associated with the 17 March 2015 storm and gained an insight into how the storm developed responding to the solar wind conditions by fitting to both cylindrical and toroidal flux rope models.
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Interplanetary Magnetic Flux Ropes as Agents Connecting Solar Eruptions and Geomagnetic Activities

TL;DR: In this article, the authors investigated the solar wind structure for 11 cases that were selected for the campaign study promoted by the International Study of Earth-affecting Solar Transients (ISEST) MiniMax24 Working Group 4.
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OCTAD-S: digital fast Fourier transform spectrometers by FPGA

TL;DR: In this article, the authors have developed a digital fast Fourier transform spectrometer made of an analog-to-digital converter (ADC) and a field-programmable gate array (FPGA).
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OCTAD-S: Digital Fast Fourier Transform Spectrometers by FPGA

TL;DR: In this paper, the authors have developed a digital fast Fourier transform (FFT) spectrometer made of an analog-to-digital converter (ADC) and a field-programmable gate array (FPGA).
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Structure of interplanetary magnetic cloud on April 16, 1999 and its origin estimated by fitting the torus‐shaped flux rope model

TL;DR: In this article, the authors examined the relationship between interplanetary magnetic cloud observed by the ACE satellite on April 16, 1999 and its solar origin, which is consistent with previous studies about magnetic clouds and their solar origins, although corresponding solar surface phenomena occurred near the central meridian.