Sheet-Type Flow Process Using Magnetic-Field-Induced Heating with Single-Mode Microwaves Applied to a Continuous Metal Nanoparticle Synthesis

2020 ◽  
Vol 59 (46) ◽  
pp. 20447-20454
Author(s):  
Masato Miyakawa ◽  
Takashi Nakamura ◽  
Ryoko Iwabuchi ◽  
Masateru Nishioka
RSC Advances ◽  
2015 ◽  
Vol 5 (19) ◽  
pp. 14637-14645 ◽  
Author(s):  
Takuya Sumi ◽  
Ralf Dillert ◽  
Satoshi Horikoshi

On preparation of bimetal nanoparticles by using a single-mode microwave resonator, Ag–Ni and Pd–Ag nanocomposites were synthesized under microwave irradiation at 80 centigrade, which was a lower temperature than that for reduction of Ag ion.


1994 ◽  
Vol 08 (26) ◽  
pp. 1661-1665
Author(s):  
WANG ZHIHE ◽  
HAN HANMIN ◽  
HAN GUCHANG ◽  
WANG SHUNXI

The magnetoresistance curves of Bi(2223) thick film were measured near T c with applied magnetic field parallel and perpendicular to the c axis ranging up to 0.12 T. The results show that thermally activated flux flow region does not exist very close to T c and magnetoresistive transition can be well described by a thermally activated flux flow process below 108.5 K and at lower magnetic field. The relation between applied magnetic field H and temperature T was found to fit with “irreversibility line.”


2015 ◽  
Vol 44 (12) ◽  
pp. 1206002
Author(s):  
PU Sheng-li ◽  
TANG Jia-li ◽  
LIU Zhi-heng ◽  
LUO Long-feng

2020 ◽  
Vol 493 (1) ◽  
pp. 1249-1260
Author(s):  
G Rüdiger ◽  
M Schultz

ABSTRACT A conducting Taylor–Couette flow with quasi-Keplerian rotation law containing a toroidal magnetic field serves as a mean-field dynamo model of the Tayler–Spruit type. The flows are unstable against non-axisymmetric perturbations which form electromotive forces defining α effect and eddy diffusivity. If both degenerated modes with m = ±1 are excited with the same power then the global α effect vanishes and a dynamo cannot work. It is shown, however, that the Tayler instability produces finite α effects if only an isolated mode is considered but this intrinsic helicity of the single-mode is too low for an α2 dynamo. Moreover, an αΩ dynamo model with quasi-Keplerian rotation requires a minimum magnetic Reynolds number of rotation of Rm ≃ 2000 to work. Whether it really works depends on assumptions about the turbulence energy. For a steeper-than-quadratic dependence of the turbulence intensity on the magnetic field, however, dynamos are only excited if the resulting magnetic eddy diffusivity approximates its microscopic value, ηT ≃ η. By basically lower or larger eddy diffusivities the dynamo instability is suppressed.


2019 ◽  
Vol 37 (13) ◽  
pp. 3208-3213
Author(s):  
Cui Liang ◽  
Dengwei Zhang ◽  
Yilan Zhou ◽  
Xiaowu Shu ◽  
Shuangliang Che ◽  
...  

Langmuir ◽  
2013 ◽  
Vol 29 (31) ◽  
pp. 9863-9873 ◽  
Author(s):  
Siva Rama Krishna Perala ◽  
Sanjeev Kumar

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