Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Naoki Kohara"'
Autor:
Yoshitaka Saito, M. Kubo, Naoki Kohara, K. Kobayashi, Kazuyoshi Kumagai, Takamasa Yamagami, K. Mori, T. Tamura, Yasushi Sakamoto, Saku Tsuneta, Yukio Katsukawa
Publikováno v:
Solar Physics. 250:431-441
Spectroscopic observation of solar flares in the hard X-ray energy range, particularly the 20 ∼ 100 keV region, is an invaluable tool for investigating the flare mechanism. This paper describes the design and performance of a balloon-borne hard X-r
Autor:
Naoki Kohara, Katsuhiro Mouri, Takami Yasuda, Mayu Urata, Chiaki Kudo, Takumi Hamatani, Mamoru Endo
Publikováno v:
GCCE
Astronomy education needs flexible education programs in accordance with various seasonal phenomena. However, panels or exhibits in science museums are often too static to behave dynamically to serve the purpose. In this paper, we represent a method
Autor:
Saku Tsuneta, M. Kubo, Tomonori Tamura, Takamasa Yamagami, Ken Kobayashi, Yasushi Sakamoto, Kazuyoshi Kumagai, Yukio Katsukawa, Naoki Kohara, Yoshitaka Saito
Publikováno v:
The Astrophysical Journal. 648:1239-1246
We report on the analysis of a thermal flare observed by a newly developed balloon-borne hard X-ray spectrometer. This instrument uses CdTe detectors and can observe the 20-120 keV hard X-ray range, with 3.0 keV energy resolution at 60 keV. During th
Autor:
K. Mori, Takamasa Yamagami, Yoshitaka Saito, Yukio Katsukawa, Kazuyoshi Kumagai, M. Kubo, Yasushi Sakamoto, Saku Tsuneta, T. Tamura, K. Kobayashi, Naoki Kohara
Publikováno v:
Advances in Space Research. 33(10):1786-1789
著者人数: 11名
Accepted: 2003-05-02
資料番号: SA1003991000
Accepted: 2003-05-02
資料番号: SA1003991000
Autor:
Yoshinori Ichikawa, Seima Kato, Chidane Ouchi, Katsuhiko Murakami, Naoki Kohara, Tokuyuki Honda, Katsumi Sugisaki, Yucong Zhu, Katsura Otaki, Masanobu Hasegawa, Mitsuo Takeda
Publikováno v:
Fringe 2013 ISBN: 9783642363580
Extreme ultraviolet (EUV, λ=13.5 nm) lithography is expected as the next generation lithography to the ArF immersion lithograph (λ =193 nm ). Projection optics is composed of several aspheric mirrors and its aberration should be about 1/30λ rms (0
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8428d011a7f04f7f13399d87760e2477
https://doi.org/10.1007/978-3-642-36359-7_70
https://doi.org/10.1007/978-3-642-36359-7_70
Publikováno v:
JSAP-OSA Joint Symposia 2014 Abstracts.
Stimulated Raman scattering (SRS) microscope has enabled label-free rapid Raman spectral imaging. Recent studies have reported video-rate imaging with a pixel clock of over 10 MHz [1, 2]. However, these systems require expensive and bulky devices suc
Publikováno v:
JSAP-OSA Joint Symposia 2014 Abstracts.
Stimulated Raman scattering (SRS) microscope is a powerful tool for label-free rapid imaging [1-3]. As a fiber-laser-based SRS (FL-SRS) microscope is promising in terms of compactness, robustness and cost efficiency, several types of FL-SRS microscop
Publikováno v:
Solar Energy Materials and Solar Cells. 67:209-215
We investigated the electrical properties of the Cu(In,Ga)Se 2 /MoSe 2 /Mo structure. CIGS/Mo heterocontact including the MoSe 2 layer is not Schottky-type but a favorable ohmic-type contact by the evaluation of dark I – V measurement at low temper
Publikováno v:
Solar Energy Materials and Solar Cells. 50:63-70
Cell performances of Cu(In,Ga)Se 2 (CIGS) thin-film solar cells were measured and analyzed as a function of temperature and illumination. The J sc and V oc were linearly changed with the temperature in the range of 10°C–70°C, and the J sc was pro
Publikováno v:
Journal of Applied Physics. 82:3572-3575
A transient photocurrent measurement with a zero-field time-of-flight configuration was carried out on ITO/ZnO/CdS(n-type)/Cu(In,Ga)Se2(p-type, Eg=1.15 eV)/Mo/glass solar cell to get the information about the minority carrier transport on the Cu(In,G