http://chineseinput.net/에서 pinyin(병음)방식으로 중국어를 변환할 수 있습니다.
변환된 중국어를 복사하여 사용하시면 됩니다.
M. Shimizu,Y. Ohsawa,H. Yoda,S. Shirotori,B. Altansargai,N. Shimomura,Y. Kato,S. Oikawa,H. Sugiyama,T. Inokuchi,K. Koi,M. Ishikawa,K. Ikegami,A. Kurobe Korean Magnetics Society 2018 Journal of Magnetics Vol.23 No.4
A voltage-control spintronics memory (VoCSM) which has a potential of low energy consumption uses the spin-Hall effect (SHE) and the voltage-controlled magnetic anisotropy (VCMA) effect for its write operation. In this work, the relationship between the critical switching current (Icsw) and the SHE electrode thickness (tN) is investigated in the range of 5 nm < tN < 8 nm. In the fabrication process, we develop highly-selective patterning process to stop MTJ etching precisely on the surface of the SHE electrode. Using the technique, Icsw is reduced by half as tN is varied from 8 nm to 5 nm, and Icsw of 112 mA at 20 ns write current pulse is obtained for MTJ size of 50 × 150 nm2 on Ta(2 nm)/TaB (3 nm) electrode. The results indicate that the decrease in the SHE electrode thickness is a promised method to reduce Icsw, which leads VoCSM to a low-energy-consumption device.
H. Yoda,Y. Ohsawa,Y. Kato,N. Shimomura,M. Shimizu,K. Koi,S. Shirotori,T. Inokuchi,H. Sugiyama,S. Oikawa,B. Altansargai,M. Ishikawa,A. Kurobe 한국자기학회 2019 Journal of Magnetics Vol.24 No.1
We designed a voltage-control spintronics memory unit-cell, VoCSM, with high write-efficiency to prove a potential to reduce writing energy per bit. By optimizing a self-aligned structure, the cell has the critical switching current (Icsw) smaller than 50 μA at 20 nsec. for designed MTJ size of about 50 × 150 ㎚². The value is much smaller than that for mature STT-MRAM with the similar dimension. VoCSM also was proved to have unlimited endurance. Finally, with an empirical equation of Icsw further reduction of Icsw is estimated to clarify that VoCSM has a potential to reduce Icsw down to several μA.
AKARI MID- TO FAR-INFRARED OBSERVATIONS OF DIFFUSE GALACTIC EMISSION
Sakon, I.,Onaka, T.,Mori, T.I.,Ohsawa, R.,Doi, Y.,Okada, Y.,Kaneda, H.,Ootsubo, T. The Korean Astronomical Society 2012 天文學論叢 Vol.27 No.4
We have collected dozens of mid-infrared spectra showing UIR bands from diffuse Galactic emitting regions with the AKARI's Infrared Camera (IRC) onboard AKARI, as part of the ISMGN Mission Program. The datasets cover various directions in the inner Galactic Plane ($|l|$ < 70 deg), in the outer Galactic Plane ($|l|$ > 70 deg), and in the off-Plane ($|b|$ > 2 deg). The variations in the UIR band ratios are examined in terms of the radiation environments judged from the far-infrared ($50-170{\mu}m$) spectral energy distribution (SED) made with AKARI/FIS All Sky Survey data at each slit position where mid-IR spectra were obtained. We have found that the band ratios of $6.2{\mu}m/11.2{\mu}m$ and $7.7{\mu}m/11.2{\mu}m$ toward the inner Galaxy are systematically higher than those toward the outer Galaxy and off the Galactic plane. Likely causes of the variations in properties of UIR bands in diffuse emission on a Galactic scale are discussed in this paper.
Planck Collaboration, Planck Collaboration,Giard, M.,Berne, O.,Doi, Y.,Ishihara, D.,Joblin, Ch.,Kaneda, I.,Marshall, D.,Nakagawa, T.,Ohsawa, R.,Onaka, T.,Sakon, I.,Shibai, H.,Ysard, N. The Korean Astronomical Society 2012 天文學論叢 Vol.27 No.4
We show how the rotation emission from isolated interstellar Polycyclic Aromatic Hydrocarbons (PAHs) can explain the so-called anomalous microwave emission (AME). AME has been discovered in the last decade as microwave interstellar emission (10 to 70 GHz) that is in excess compared to the classical emission processes: thermal dust, free-free and synchrotron. The PAHs are the interstellar planar nano-carbons responsible for the near infrared emission bands in the 3 to 15 micron range. Theoretical studies show that under the physical conditions of the interstellar medium (radiation and density) the PAHs adopt supra-thermal rotation velocities, and consequently they are responsible for emission in the microwave range. The first results from the PLANCK mission unexpectedly showed that the AME is not only emitted by specific galactic interstellar clouds, but it is present throughout the galactic plane, and is particularly strong in the cold molecular gas. The comparison of theory and observations shows that the measured emission is fully consistent with rotation emission from interstellar PAHs. We draw the main lines of our PLANCK-AKARI collaborative program which intends to progress on this question by direct comparison of the near infrared (AKARI) and microwave (PLANCK) emissions of the galactic plane.