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Nanocrystallization and High Tensile Strength of Amorphous Zr-Al-Ni-Cu-Ag Alloys
Kim, Y . H .,Kim, S . J .,Yang, Y . S .,Inoue, A .,Han, T . K .,Kim, I . B . 대한금속재료학회(대한금속학회) 2001 METALS AND MATERIALS International Vol.7 No.2
The influence of the addition of Ag to the crystallization and mechanical properties of the amorphous Zr_(65)Al_(7.5)Ni_(10)Cu(17.5-x)Ag_x (x=5, 10 at.%) alloys was investigated. It was found that crystallization takes place through the two-stage process of Am→Am'+icosahedral-phase Zr₂Cu+Zr₂Ni+Zr₂Al₃. The icosahedral particles have a spherical morphology and their sizes range from 10 to 100 ㎚. With the increase in the amount of Ag, thermal instability increases through the simultaneous decrease of T_x and ΔT_x. The σ_f increases significantly from 1560 ㎫ at 0%V_f to 2120 ㎫ at 62%V_f for the 10% Ag alloy.
Evidence of a Rattling Transition in the Caged Compounds LaRu2Zn20 and LaIr2Zn20: 139La NMR Studies
Hideki Tou,Kenji Asaki,Hisashi Kotegawa,Takahiro Onimaru,Keisuke T. Matsumoto,Yukihiro F. Inoue,Toshiro Takabatake 한국물리학회 2013 THE JOURNAL OF THE KOREAN PHYSICAL SOCIETY Vol.63 No.3
We report a study of 139La(I=7/2) nuclear magnetic resonance (NMR) to investigate the structuralphase transition in the two caged compounds LaIr2Zn20 and LaRu2Zn20 from microscopic viewpoints. The former compound shows a second-order structural phase transition around Ts = 200 Kwhereas the latter one shows a first-order structural phase transition at Ts = 150 K. For both compounds,quite narrow La-NMR lines of less that 10 kHz without any electric field gradient (EFG) atthe La site were observed at temperatures above Ts, indicating that the local symmetry at the Lasite holds a cubic symmetry. On the other hand, an EFG at La site appears at temperatures belowTs, evidencing symmetry lowering occurs at the La site at temperatures below Ts. At temperaturesaround Ts, both the nuclear spin-lattice relaxation rate (1/T1) and the nuclear spin-spin relaxationrate (1/T2) show unusual enhancements associated with the slowing down of the EFG fluctuations. However, the temperature dependences of 1/T1T and 1/T2 are different from the typical slowingdownphenomena of the EFG fluctuations due to the classical motional narrowing. The lowering ofthe local symmetry at the La site is ascribed to a freezing of the rattling motion.
Inoue, S.,Hayashi, K.,Magara, T.,Choe, G. S.,Park, Y. D. IOP Publishing 2014 The Astrophysical journal Vol.788 No.2
<P>We performed a magnetohydrodynamic (MHD) simulation using a nonlinear force-free field (NLFFF) in solar active region 11158 to clarify the dynamics of an X2.2-class solar flare. We found that the NLFFF never shows the dramatic dynamics seen in observations, i.e., it is in a stable state against the perturbations. On the other hand, the MHD simulation shows that when the strongly twisted lines are formed at close to the neutral line, which are produced via tether-cutting reconnection in the twisted lines of the NLFFF, they consequently erupt away from the solar surface via the complicated reconnection. This result supports the argument that the strongly twisted lines formed in NLFFF via tether-cutting reconnection are responsible for breaking the force balance condition of the magnetic fields in the lower solar corona. In addition to this, the dynamical evolution of these field lines reveals that at the initial stage the spatial pattern of the footpoints caused by the reconnection of the twisted lines appropriately maps the distribution of the observed two-ribbon flares. Interestingly, after the flare, the reconnected field lines convert into a structure like the post-flare loops, which is analogous to the extreme ultraviolet image taken by the Solar Dynamics Observatory. Eventually, we found that the twisted lines exceed a critical height at which the flux tube becomes unstable to the torus instability. These results illustrate the reliability of our simulation and also provide an important relationship between flare and coronal mass ejection dynamics.</P>
BUILDUP AND RELEASE OF MAGNETIC TWIST DURING THE X3.4 SOLAR FLARE OF 2006 DECEMBER 13
Inoue, S.,Shiota, D.,Yamamoto, T. T.,Pandey, V. S.,Magara, T.,Choe, G. S. IOP Publishing 2012 The Astrophysical journal Vol.760 No.1
<P>We analyze the temporal evolution of the three-dimensional magnetic structure of the flaring active region (AR) NOAA 10930 by using the nonlinear force-free fields extrapolated from the photospheric vector magnetic fields observed by the Solar Optical Telescope on board Hinode. This AR consisted mainly of two types of twisted magnetic field lines: one has a strong negative (left-handed) twist due to the counterclockwise motion of the positive sunspot and is rooted in the regions of both polarities in the sunspot at a considerable distance from the polarity inversion line (PIL). In the flare phase, dramatic magnetic reconnection occurs in those negatively twisted lines in which the absolute value of the twist is greater than a half-turn. The other type consists of both positively and negatively twisted field lines formed relatively close to the PIL between two sunspots. A strong Ca II image began to brighten in this region of mixed polarity, in which the positively twisted field lines were found to be injected within one day across the pre-existing negatively twisted region, along which strong currents were embedded. Consequently, the central region near the PIL contains a mix of differently twisted field lines and the strong currents may play a prominent role in flare onset.</P>
Fabrication of Nano-Structures on NiFe Film by Anodization with Atomic Force Microscope
T. Okada,H. Uchida,M. Inoue 한국자기학회 2006 Journal of Magnetics Vol.11 No.3
We studied local anodization on permalloy (Ni??Fe₂?) thin film with an atomic force microscope (AFM), which was performed by applying a voltage between the permalloy sample and conductive AFM tip. Comparing with anodization on Si (100) substrate, nano-structures on the permalloy thin film was fabricated with low processability. In order to improve the processability on the permalloy thin film, we used dot-fabrication method, that is, a conductive AFM probe was kept at a position on the film during the anodization process.
Changes in Serum Biochemical Markers of Bone Cell Activity in Growing Thoroughbred Horses
Inoue, Yoshinobu,Asai, Y.,Ohmori, H.,Fujii, H.,Matsui, T.,Yano, H. Asian Australasian Association of Animal Productio 2006 Animal Bioscience Vol.19 No.11
We studied the changes in biochemical markers of bone metabolism in growing Thoroughbred horses. Serum osteocalcin (OC), as a marker for bone formation, and carboxy-terminal propeptide of type-I collagen (PICP), as a marker for bone formation, carboxy-terminal telopeptide of type-I collagen (ICTP), as a marker for bone resorption, were determined in nine clinically healthy horses from 3 d to 17 mo of age. The BW and withers height (WH) increased during the study. On the other hand, a rapid reduction in body weight gain (BWG) was observed between 1 mo and 9 mo of age and a rapid reduction in withers height gain was observed between 1 mo and 5 mo of age. The serum markers decreased significantly with increasing age. In particular, dramatic changes in serum markers occurred between 3 d to 1 wk and 5 to 7 mo of age in these horses, which suggests that bone turnover rapidly decreased after birth. On the other hand, the ratio of PICP to ICTP decreased through the experiment. This result suggests that the reduction in bone formation exceeded that of bone resorption. There was a significant correlation between markers and growth parameters, except for the correlation between PICP and BWG on single linear regression analysis. Serum OC and ICTP were affected by the WH in multiple linear regression analysis. These results indicated that the age-related variation in serum biochemical markers of bone metabolism reflected bone growth, but neither BW nor BWG. Therefore, we consider that changes in bone modeling are the major factor affecting the levels of serum biochemical markers by 17 mo of age in horses.
Inoue, Y.,Kuramoto, Y.,Hattori, M.,Adachi, M.,Kimura, M.,Akahane, T. The Korean Infomation Display Society 2011 Journal of information display Vol.12 No.3
Alignment failure sometimes occurs during the rubbing process because the rubbing cloth comes in direct contacts with the surface of the alignment film. A number of researches observed and evaluated the surface of the alignment film after the rubbing process had been reported. The real-time rubbing process has not been observed directly yet, though. In this study, the movement of the piles of the rubbing cloth during the rubbing process was observed with a high-speed camera. Furthermore, the relationship between the rubbing scratch on the alignment films and the movement of the pile was investigated. It was found that the movement of the pile affected the rubbing scratches.