12 results on '"Mase H"'
Search Results
2. The JEM-EUSO Mission.
- Author
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Ebisuzaki, T., Mase, H., Takizawa, Y., Kawasaki, Y., Miyamoto, H., Shinozaki, K., Ohmori, H., Hachisu, Wada, S., Ogawa, T., Kajino, F., Inoue, N., Sakaki, N., Adams, J., Christl, M., Young, R., Bonamente, M., Santangelo, A., Teshima, M., and Parizot, E.
- Subjects
- *
ASTRONOMICAL observations , *COSMIC rays , *PARTICLES (Nuclear physics) , *TELESCOPES , *CHERENKOV radiation , *ULTRAVIOLET radiation , *PHOTONS , *PARTICLE acceleration , *NEUTRINO astrophysics , *SYMMETRY (Physics) - Abstract
The JEM-EUSO mission explores the origin of the extreme energy cosmic rays (EECRs) above 100 EeV and explores the limits of the fundamental physics, through the observations of their arrival directions and energies. It is designed to achieve an exposure larger than 1 million km2 sr year at the highest energies to open a new particle astronomy channel. This super-wide-field of view (60 degrees) telescope with a diameter of about 2.5 m looks down from space onto the night sky to detect near UV photons (330-400 nm, both fluorescent and Cherenkov photons) emitted from the giant air showers produced by EECRs. The arrival direction map with more than five hundred events after just the three years will tell us the origin of the EECRs, allow us to identify the nearest EECR sources with known astronomical objects, which can afterwards be examined in other astronomical channels. This is likely to lead to an understanding of the acceleration mechanisms perhaps producing discoveries in astrophysics and fundamental physics. The comparison of the energy spectra among the spatially resolved individual sources will help to clarify the acceleration/emission mechanism, and also finally confirm the Greisen-Zatsepin-Kuz'min process for the validation of Lorentz invariance up to γ∼1011. Neutral components (neutrinos and gamma rays) can be detected as well, if their fluxes are high enough. The JEM-EUSO mission is planned to be launched by a H2B rocket about JFY 2016 and transferred to ISS by H2 Transfer Vehicle (HTV). It will be attached to the Exposed Facility external experiment platform of 'KIBO.' JEM-EUSO is being developed by an international collaboration of institutions from 13 countries. [ABSTRACT FROM AUTHOR]
- Published
- 2011
- Full Text
- View/download PDF
3. Modified Hunt’s Equation Incorporating Wave Setup.
- Author
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Hedges, T. S. and Mase, H.
- Subjects
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WAVES (Physics) , *VIBRATION (Mechanics) , *HYDRODYNAMICS , *ATMOSPHERIC waves , *ACCELERATION waves - Abstract
Hunt’s equation provides a simple means of estimating the runup of breaking waves. However, breaking waves also induce setup on a slope. A modification to Hunt’s equation is advocated which accounts for the presence of wave setup. Support for the modification is provided by data from model tests involving random waves approaching smooth, impermeable slopes of 1:5, 1:10, 1:20, and 1:30. Coefficients to be used in the modified equation are given which allow the significant runup and other characteristic values to be estimated. [ABSTRACT FROM AUTHOR]
- Published
- 2004
- Full Text
- View/download PDF
4. Microcrystalline silicon solar cells fabricated on polymer substrate
- Author
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Mase, H., Kondo, M., and Matsuda, A.
- Subjects
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SOLAR cells , *SILICON crystals - Abstract
Low temperature fabrication of microcrystalline silicon solar cells was studied. It was found that reasonable performance is available even limiting substrate temperature at 100°C. Applying this technique to thermoplastic polymer substrates, a conversion efficiency of 6% was achieved. [Copyright &y& Elsevier]
- Published
- 2002
- Full Text
- View/download PDF
5. Simple line-sampling apparatus for line frequency stroboscopic observation of periodic phenomena using scanning electron microscopy.
- Author
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Ikuta, T., Mase, H., and Shimizu, R.
- Subjects
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PHYSICS instruments , *SCANNING electron microscopy - Abstract
Detailed operations of the apparatus for the stroboscopic observation of periodic phenomena at the region of line frequencies, such as the magnetic domain response, under the scanning electron microscopy are described in this paper. To achieve the stroboscopic observation at such low frequencies, a new line-sampling technique has been introduced instead of the conventional point-sampling method. In addition to the line-sampling stroboscopy, a multiframe operation is also introduced to display the stroboscopic images of different phase values simultaneously. These operations are simply realized by applying the raster separation and the blanking on the display monitor scope under the multiple line-sampling during the one-drive period. To demonstrate the ability of this simple apparatus, some results of the stroboscopic observation of magnetic domains in an Fe–Si sample under a 60-Hz drive field are also presented in this paper. [ABSTRACT FROM AUTHOR]
- Published
- 1987
- Full Text
- View/download PDF
6. Dynamic observation of magnetic domains in amorphous ferromagnetic ribbons driven at line frequencies.
- Author
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Mase, H., Shimizu, R., and Ikuta, T.
- Subjects
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MAGNETS , *PHYSICS - Abstract
The recently developed dynamic observation technique of R. Shimizu and T. Ikuta [Appl. Phys. Lett. 44, 811 (1984)] for scanning electron microscopy, ‘‘line-sampling stroboscopy,’’ was used for the observation of magnetic domains in an amorphous ferromagnetic ribbon. The image-processing technique introduced turned out to be very useful, allowing the behavior of domain walls, which is often obscured by topological contrast, to be clearly observed. [ABSTRACT FROM AUTHOR]
- Published
- 1987
- Full Text
- View/download PDF
7. Overall View of the JEM-EUSO Instruments.
- Author
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Kajino, F., Ebisuzaki, T., Mase, H., Tsuno, K., Takizawa, Y., Kawasaki, Y., Shinozaki, K., Ohmori, H., Wada, S., Inoue, N., Sakaki, N., Adams, J., Christl, M., Young, R., Ferguson, C., Bonamente, M., Santangelo, A., Teshima, M., Parizot, E., and Gorodetzky, P.
- Subjects
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ASTRONOMICAL observatories , *WIDE-angle lenses , *TELESCOPES , *CHERENKOV radiation , *COSMIC ray showers , *PHOTONS , *ATMOSPHERE , *EARTH (Planet) - Abstract
JEM-EUSO mission with a large and wide-angle telescope mounted on ISS has been planned to open up 'particle astronomy' through the investigation of extreme-energy cosmic rays by detecting fluorescent and Cherenkov photons by air showers developed in the earth's atmosphere. The JEM-EUSO telescope consists of optical Fresnel lenses with a diameter of about 2.5 m, 300 k channels of MAPMT, frontend readout electronics, trigger electronics, and system electronics. An infrared camera and a LIDAR system will be used to monitor the earth's atmosphere. [ABSTRACT FROM AUTHOR]
- Published
- 2011
- Full Text
- View/download PDF
8. The JEM-EUSO Mission to Explore the Extreme Universe.
- Author
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Ebisuzaki, Toshikazu, Takahashi, Y., Kajino, F., Mase, H., Santangelo, A., Teshima, M., Parizot, E., Gorodetzky, P., Catalano, O., Picozza, P., Casolino, M., Panasyuk, M., Khrenov, B. A., Park, I. H., Peter, T., Medina-Tanco, G., Rodriguez-Frias, D., Szabelski, J., and Bobik, P.
- Subjects
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COSMIC rays , *EXTREME environments , *CHERENKOV radiation , *NEUTRINOS , *GAMMA rays , *PARTICLE acceleration - Abstract
The JEM-EUSO mission explores the origin of the extreme energy comic-rays (EECRs) above 1020 eV and challenges to the limit of the basic physics, through the observations, of their arrival directions and energies. It is designed to observe more than 1,000 events of EECRs above 7×1019 eV in its five-year operation with an exposure larger than 1 million km2·sr·year. The super-wide-field (60 degrees) telescope with a diameter of about 2.5 m looks down the atmosphere of the night-side of the earth to detect near UV photons (330–400 nm, both fluorescent and Cherenkov photons) emitted from the giant air-shower produced by an EECR. The arrival direction map with 1,000 events naturally tells us the origin of the EECRs and allows us to identify the EECR sources to known astronomical objects. The comparison among the energy spectra of the spatially resolved individual sources will clarify the acceleration/emission mechanism, and also finally confirm the Greisen-Zatse′pin-Kuzmin process for the validation of Lorentz invariance up to γ∼1011. Neutral components (neutrinos and gamma rays) can also be detected as well, if their fluxes are high enough. The JEM-EUSO mission is planned to be launched by a H2B rocket about 2015 and transferred to ISS by H2 Transfer Vehicle (HTV). It will be attached to the external experiment platform of “KIBO” which completed July 2009 by STS-127 mission of the space shuttle. The first flight of HTV by H2B rocket was successfully done in September and October 2009. [ABSTRACT FROM AUTHOR]
- Published
- 2010
- Full Text
- View/download PDF
9. Sandy Beach Profile Response to Sloping Seawalls: An Experimental Study.
- Author
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Zheng, J.-H., Jeng, D.-S., and Mase, H.
- Subjects
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SEA-walls , *BEACHES , *BEACH erosion , *STORM surges , *FIELD research , *ENERGY dissipation , *SHORELINE monitoring - Abstract
Zheng, J.-H., Jeng, D.-S. and Mase, H., 2007. Sandy beach profile response to sloping seawalls: an experimental study. Journal of Coastal Research, SI 50 (Proceedings of the 9th International Coastal Symposium), 334 – 337. Gold Coast, Australia, ISSN 0749.0208. Seawalls are commonly used as a tool for coastal defence worldwide. Most previous studies have considered the case of vertical seawalls and descriptions of existing seawalls, rather than the influence of different designs of sloping seawalls on beach erosion. In this study, laboratory investigations of an undistorted moveable bed model were conducted to determine the resulting beach profile of artificial sandy beaches. In the experiments, three different sloping seawalls were considered under erosive wave conditions with a 50-year return period. The coast of Northern Jiangsu Province, China, is used as a case study. To simulate natural conditions, similarity criteria are developed assuming that the energy dissipation per unit volume along the beach profile is uniform and that the wave properties can be properly scaled by Froude criteria. Field surveys of beach profile changes due to the storm surge induced by Typhoon 9711 were taken to validate the experimental model and good agreements were attained. Spatial profile configurations were studied by examining dominant profile features such as the break point bar and the scour trough on the seawall-backed profiles. Experimental results provided a reference for the maintenance of artificial sandy beaches and the design of seawalls on the coast of Northern Jiangsu Province, China. [ABSTRACT FROM AUTHOR]
- Published
- 2007
- Full Text
- View/download PDF
10. Positive pulse bias method in plasma-based ion implantation
- Author
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Ikehata, T., Shimatsu, K., Sato, N.Y., and Mase, H.
- Subjects
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ION implantation , *X-rays - Abstract
A novel scheme of the plasma-based ion implantation (PBII), the positive pulse bias (PPB) method has been proposed, in which a workpiece to be treated is at the ground potential while the plasma surrounding it is biased to a positive high voltage; thus the ion sheath same as the one in the conventional negative pulse bias (NPB) method is formed on the workpiece. Principal merit of the PPB method over the NPB method is that it possesses a mechanism of suppressing X-rays from the wall by impact of secondary electrons and it enables to manipulate the workpiece during PBII processing. The latter merit will serve to realize an efficient continuous processing system. The principle of the PPB method is discussed based on the asymmetric double probe theory and results of the proof-of-principle experiment are presented. [Copyright &y& Elsevier]
- Published
- 2003
- Full Text
- View/download PDF
11. Sheath formation and ion flux distribution inside the trench in plasma-based ion implantation
- Author
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Ikehata, T., Shioya, K., Araki, T., Sato, N.Y., Mase, H., and Yukimura, K.
- Subjects
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ION implantation , *ELECTRON emission - Abstract
Geometrical effects of a three-dimensional workpiece on the plasma-based ion implantation have been studied using trench-shape and L-shape workpieces. Temporal and spatial evolution of the sheath and the ion flux on the workpiece are measured for a negative voltage pulse of −1.8 to −7.0 kV, 40 μs: (1) The trench is occupied by the ion sheath quickly due to the sheath overlapping from both side walls; this effect is not seen in the L-shape workpiece with only one side wall. (2) Electrons are detected inside the trench even after the ion sheath fills the trench, which is attributed to secondary electrons emitted from the surface of the workpiece by ion impact and trapped electrostatically between the side walls. (3) The ion flux incident upon the inner surface of the trench is strongly enhanced because trapped secondary electrons ionize the filling gas as in the hollow-cathode discharge. The enhanced ionization is therefore not seen in L-shape and planar workpieces. [Copyright &y& Elsevier]
- Published
- 2003
- Full Text
- View/download PDF
12. Centrifugal mass separation in rotating plasmas produced by a coaxial plasma gun.
- Author
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Ikehata, T., Suzuki, M., Tanabe, T., and Mase, H.
- Subjects
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CENTRIFUGES , *PLASMA gases , *COPPER , *ZINC - Abstract
Rotating Cu/Zn plasmas produced by a coaxial plasma gun have been applied to plasma centrifuge. A separation factor of up to 10 is measured over a radius of 4 cm when a current of 13 kA and an axial magnetic field of 2.5 kG are applied. Plasma parameters are: rotation frequency ω=1.1×106 rad/s, density n∼1015 cm-3, and ion temperature Ti=10 eV. The separation factor of 2 is attained even in the plasma core where the density is higher than one-half of the peak value. This is attributed to the fact that a strong centrifugal force forms a hollow density profile which gives the density peak at a radius of 2 cm. [ABSTRACT FROM AUTHOR]
- Published
- 1989
- Full Text
- View/download PDF
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