Zobrazeno 1 - 10
of 387
pro vyhledávání: '"Nozawa Satoshi"'
Publikováno v:
In Advances in Space Research 1 August 2023 72(3):816-829
Autor:
Fujiyama, Masashi, Hayakawa, Hisashi, Iju, Tomoya, Kawai, Toshiki, Toriumi, Shin, Otsuji, Kenichi, Kondo, Katsuya, Watanabe, Yusaku, Nozawa, Satoshi, Imada, Shinsuke
Publikováno v:
Solar Physics, 2019
We revisit the sunspot drawings made by the Japanese astronomer Kunitomo Toubei during 1835-1836 and recount the sunspot group number for each image. There are two series of drawings, preliminary (P, containing 17 days with observations) and summary
Externí odkaz:
http://arxiv.org/abs/1903.03092
Autor:
Anan, Tetsu, Yoneya, Takurou, Ichimoto, Kiyoshi, Ueno, Satoru, Shiota, Daikou, Nozawa, Satoshi, Takasao, Shinsuke, Kawate, Tomoko
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 Solar Telescope at Hida Observatory on August 9th, 2015. Observed Stokes p
Externí odkaz:
http://arxiv.org/abs/1808.06821
Autor:
Tamaoki, Susumu, Saita, Kimiharu, Hoshi, Ryosuke, Arvelius, Sachiko, Fukumi, Yukari, Nozawa, Satoshi, Shibata, Kazunari
Publikováno v:
In The Journal of Space Safety Engineering September 2022 9(3):390-396
Akademický článek
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Autor:
Kato, Koki, Fushimi, Kazunari, Nozawa, Satoshi, Iwai, Chizuo, Masuda, Takahiro, Hioki, Akira, Miyamoto, Kei, Shimokawa, Tetsuya, Akiyama, Haruhiko
Publikováno v:
In Interdisciplinary Neurosurgery: Advanced Techniques and Case Management March 2021 23
We estimated the accuracy of coronal magnetic fields derived from radio observations by comparing them to potential field calculations and the DEM measurements using EUV observations. We derived line of sight component of the coronal magnetic field f
Externí odkaz:
http://arxiv.org/abs/1512.04198
Autor:
Iwai, Kazumasa, Koshiishi, Hideki, Shibasaki, Kiyoto, Nozawa, Satoshi, Miyawaki, Shun, Yoneya, Takuro
We investigate the upper chromosphere and the transition region of the sunspot umbra using the radio brightness temperature at 34 GHz (corresponding to 8.8-mm observations) as observed by the Nobeyama Radioheliograph (NoRH). Radio free-free emission
Externí odkaz:
http://arxiv.org/abs/1511.08991
Autor:
Fushimi, Kazunari, Miyagawa, Takaki, Iwai, Chizuo, Nozawa, Satoshi, Iinuma, Nobuki, Tanaka, Ryo, Shirai, Goshi, Tanahashi, Hiroyuki, Yokoi, Tatsuo, Akiyama, Haruhiko
Publikováno v:
Global Spine Journal; Sep2024, Vol. 14 Issue 7, p2031-2038, 8p
Autor:
Fujishiro, Takashi, Nakano, Atsushi, Yano, Toma, Nakaya, Yoshiharu, Hayama, Sachio, Usami, Yoshitada, Nozawa, Satoshi, Baba, Ichiro, Neo, Masashi
Publikováno v:
In Journal of Clinical Neuroscience June 2020 76:100-106