Zobrazeno 1 - 10
of 4 945
pro vyhledávání: '"Takata M"'
Autor:
Ohkura N, Tanaka R, Watanabe S, Hara J, Abo M, Nakade Y, Horii J, Matsuura Y, Inoue D, Takata M, Tamura M, Matsumoto I, Sanada S, Kasahara K
Publikováno v:
International Journal of COPD, Vol Volume 16, Pp 1393-1399 (2021)
Noriyuki Ohkura,1 Rie Tanaka,2 Satoshi Watanabe,1 Johsuke Hara,1 Miki Abo,1 Yusuke Nakade,3 Junsei Horii,4 Yukihiro Matsuura,4 Dai Inoue,5 Munehisa Takata,6 Masaya Tamura,6 Isao Matsumoto,6 Shigeru Sanada,7 Kazuo Kasahara1 1Kanazawa University Hospit
Externí odkaz:
https://doaj.org/article/22db3662ce9c49aba93c0c7d0f62efee
Autor:
Takata, M., Gough, D. O.
Analysis of f-mode frequencies has provided a measure of the radius of the Sun which is lower, by a few hundredths per cent, than the photospheric radius determined by direct optical measurement. Part of this difference can be understood by recognizi
Externí odkaz:
http://arxiv.org/abs/2310.11299
Autor:
Harada T, Yamasaki A, Fukushima T, Hashimoto K, Takata M, Kodani M, Okazaki R, Takeda K, Watanabe M, Kurai J, Shimizu E
Publikováno v:
International Journal of COPD, Vol 2015, Iss Issue 1, Pp 595-602 (2015)
Tomoya Harada, Akira Yamasaki, Takehito Fukushima, Kiyoshi Hashimoto, Miki Takata, Masahiro Kodani, Ryota Okazaki, Kenichi Takeda, Masanari Watanabe, Jun Kurai, Eiji Shimizu Division of Medical Oncology and Molecular Respirology, Department of Multid
Externí odkaz:
https://doaj.org/article/c4e5bc1b7d3e40dd8c9ec5b57c2ddde1
Autor:
Yamasaki A, Kawasaki Y, Takeda K, Harada T, Fukushima T, Takata M, Hashimoto K, Watanabe M, Kurai J, Nishimura K, Shimizu E
Publikováno v:
International Journal of General Medicine, Vol 2014, Iss default, Pp 505-512 (2014)
Akira Yamasaki,1 Yuji Kawasaki,2 Kenichi Takeda,1 Tomoya Harada,1 Takehito Fukushima,1 Miki Takata,1 Kiyoshi Hashimoto,1 Masanari Watanabe,1 Jun Kurai,1 Koichi Nishimura,3 Eiji Shimizu1 1Division of Medical Oncology and Molecular Respirology, Departm
Externí odkaz:
https://doaj.org/article/510473fa3ea5480f8577337c52e9ca27
Autor:
Pinçon, C., Takata, M.
Publikováno v:
A&A 661, A139 (2022)
Asteroseismology has proven to be a powerful method for probing stellar interiors. Analytical descriptions of the global oscillation modes, in combination with pulsation codes, have provided valuable help in processing and interpreting the large amou
Externí odkaz:
http://arxiv.org/abs/2203.03402
Autor:
Nagai T., Arikawa Y., Hosoda H., Ioka Y., Hasegawa A., Wada K., Takaoku S., Takata M., Noritake K., Minami Y., Watanabe K., Yamanoi K., Nakamura H., Watari T., Cadatal-Raduban M., Shimizu T., Sarukura N., Nakai M., Norimatsu T., Azechi H.
Publikováno v:
EPJ Web of Conferences, Vol 59, p 13012 (2013)
A fast-decay and low-afterglow liquid scintillator was developed for the fast ignition experiment at the Institute of Laser Engineering (ILE). The liquid scintillator was coupled to a gated photomultiplier (PMT), and the gating performance under high
Externí odkaz:
https://doaj.org/article/56edd3e5380348278f3be9e81fd10cab
Autor:
Ouazzani, R-M., Lignières, F., Dupret, M-A., Salmon, S. J. A. J., Ballot, J., Christophe, S., Takata, M.
Publikováno v:
A&A 640, A49 (2020)
Gamma Doradus stars present an incredibly rich pulsation spectra, with gravito-inertial modes, in some cases supplemented with delta Scuti-like pressure modes and in numerous cases with Rossby modes. The present paper aims at showing that, in additio
Externí odkaz:
http://arxiv.org/abs/2006.09404
Publikováno v:
A&A 626, A125 (2019)
Observations of mixed modes in evolved low-mass stars enable us to probe the properties of not only the outer envelope of these stars, but also their deep layers. Among the seismic parameters associated with mixed modes, the gravity offset, denoted w
Externí odkaz:
http://arxiv.org/abs/1905.05691
Autor:
Benomar, O., Bazot, M., Nielsen, M. B., Gizon, L., Sekii, T., Takata, M., Hotta, H., Hanasoge, S., Sreenivasan, K. R., Christensen-Dalsgaard, J.
Publikováno v:
Science, Vol. 361, Issue 6408, pp. 1231-1234, 21 Sep 2018
The differentially rotating outer layers of stars are thought to play a role in driving their magnetic activity, but the underlying mechanisms that generate and sustain differential rotation are poorly understood. We report the measurement of latitud
Externí odkaz:
http://arxiv.org/abs/1809.07938
Autor:
Saio, H., Bedding, T. R., Kurtz, D. W., Murphy, S. J., Antoci, V. L., Shibahashi, H., Li, Gang, Takata, M.
The Fourier spectrum of the $\gamma$-Dor variable KIC 5608334 shows remarkable frequency groups at $\sim$3, $\sim$6, $\sim$9, and 11--12\,d$^{-1}$. We explain the four frequency groups as prograde sectoral g modes in a rapidly rotating star. Frequenc
Externí odkaz:
http://arxiv.org/abs/1803.08677