Zobrazeno 1 - 10
of 1 594
pro vyhledávání: '"Oba T"'
Publikováno v:
Therapeutics and Clinical Risk Management, Vol Volume 16, Pp 17-20 (2020)
Shinkichi Takamori, 1 Takashi Seto, 1 Mikako Jinnouchi, 2 Taro Oba, 1 Masafumi Yamaguchi, 1 Mitsuhiro Takenoyama 1 1Department of Thoracic Oncology, National Hospital Organization Kyushu Cancer Center, Fukuoka 811-1395, Japan; 2Department of Radiolog
Externí odkaz:
https://doaj.org/article/5647ec1218e14921a67367425c4bdbce
Autor:
Oba T, Ono M, Iesato A, Hanamura T, Watanabe T, Ito T, Kanai T, Maeno K, Ito KI, Tateishi A, Yoshizawa A, Takayama F
Publikováno v:
OncoTargets and Therapy, Vol 2016, Iss Issue 1, Pp 1641-1646 (2016)
Takaaki Oba,1 Mayu Ono,1 Asumi Iesato,1 Toru Hanamura,1 Takayuki Watanabe,1 Tokiko Ito,1 Toshiharu Kanai,1 Kazuma Maeno,1 Ken-ichi Ito,1 Ayako Tateishi,2 Akihiko Yoshizawa,2 Fumiyoshi Takayama31Division of Breast, Endocrine and Respiratory Surgery, D
Externí odkaz:
https://doaj.org/article/883bf6ebf0cc49549a6e381dfe0046c8
Autor:
Iesato A, Oba T, Ono M, Hanamura T, Watanabe T, Ito T, Kanai T, Maeno K, Ishizaka K, Kitabatake H, Takeuchi D, Suzuki A, Nakayama J, Ito K
Publikováno v:
OncoTargets and Therapy, Vol 2015, Iss default, Pp 91-97 (2014)
Asumi Iesato,1 Takaaki Oba,1 Mayu Ono,1 Toru Hanamura,1 Takayuki Watanabe,1 Tokiko Ito,1 Toshiharu Kanai,1 Kazuma Maeno,1 Katsuhiko Ishizaka,2 Hiroyuki Kitabatake,3 Daisuke Takeuchi,4 Akira Suzuki,4 Jun Nakayama,5 Ken-ichi Ito11Division of Breast and
Externí odkaz:
https://doaj.org/article/8e1a74d0218b4c9691cf9fcae66ea981
We perform radiative magnetohydrodynamic calculations for the solar quiet region to investigate the dependence of statistical flow on magnetic properties and the three-dimensional (3D) structure of magnetic patches in the presence of large-scale flow
Externí odkaz:
http://arxiv.org/abs/2103.03789
Publikováno v:
EPJ Web of Conferences, Vol 59, p 19004 (2013)
We have demonstrated frequency upshift in the terahertz region by flash ionization. The magnitude of upshift frequency is tuned by the laser intensity. A proof of principle experiment has been performed with a plasma creation time scale much shorter
Externí odkaz:
https://doaj.org/article/606c5a64bbab4265a2c99486e5151c83
Gas convection is observed in the solar photosphere as the granulation, i.e., having highly time-dependent cellular patterns, consisting of numerous bright cells called granules and dark surrounding-channels called intergranular lanes. Many efforts h
Externí odkaz:
http://arxiv.org/abs/2001.03575
Autor:
Noda, C. Quintero, Iijima, H., Katsukawa, Y., Shimizu, T., Carlsson, M., Rodríguez, J. de la Cruz, Cobo, B. Ruiz, Suárez, D. Orozco, Oba, T., Anan, T., Kubo, M., Kawabata, Y., Ichimoto, K., Suematsu, Y.
We investigate the diagnostic potential of the spectral lines at 850 nm for understanding the magnetism of the lower atmosphere. For that purpose, we use a newly developed 3D simulation of a chromospheric jet to check the sensitivity of the spectral
Externí odkaz:
http://arxiv.org/abs/1904.09151
Autor:
Noda, C. Quintero, Uitenbroek, H., Carlsson, M., Suárez, D. Orozco, Katsukawa, Y., Shimizu, T., Cobo, B. Ruiz, Kubo, M., Oba, T., Kawabata, Y., Hasegawa, T., Ichimoto, K., Anan, T., Suematsu, Y.
The next generation of solar observatories aim to understand the magnetism of the solar chromosphere. Therefore, it is crucial to understand the polarimetric signatures of chromospheric spectral lines. For this purpose, we here examine the suitabilit
Externí odkaz:
http://arxiv.org/abs/1810.01067
Autor:
Noda, C. Quintero, Villanueva, G. L., Katsukawa, Y., Solanki, S. K., Suárez, D. Orozco, Cobo, B. Ruiz, Shimizu, T., Oba, T., Kubo, M., Anan, T., Ichimoto, K., Suematsu, Y.
Publikováno v:
A&A 610, A79 (2018)
Of the two solar lines, K I $D_1$ and $D_2$, almost all attention so far has been devoted to the $D_1$ line, as $D_2$ is severely affected by an O$_2$ atmospheric band. This, however, makes the latter appealing for balloon and space observations from
Externí odkaz:
http://arxiv.org/abs/1801.01655
Solar granules are bright patterns surrounded by dark channels called intergranular lanes in the solar photosphere and are a manifestation of overshooting convection. Observational studies generally find stronger upflows in granules and weaker downfl
Externí odkaz:
http://arxiv.org/abs/1709.06933