Numerical analysis for heat transfer enhancement of a lithium flow under a transverse magnetic field

2000 ◽  
Vol 51-52 ◽  
pp. 899-907 ◽  
Author(s):  
Naotaka Umeda ◽  
Minoru Takahashi
Keyword(s):  
Magnetic Field ◽  
Heat Transfer ◽  
Numerical Analysis ◽  
Heat Transfer Enhancement ◽  
Transverse Magnetic Field ◽  
Transverse Magnetic ◽  
Transfer Enhancement

Heat Transfer in Liquid Metal at an Upward Flow in a Pipe in Transverse Magnetic Field

2020 ◽  
Vol 58 (3) ◽  
pp. 400-409
Author(s):  
N. A. Luchinkin ◽  
N. G. Razuvanov ◽  
I. A. Belyaev ◽  
V. G. Sviridov
Keyword(s):  
Magnetic Field ◽  
Heat Transfer ◽  
Liquid Metal ◽  
Transverse Magnetic Field ◽  
Transverse Magnetic ◽  
Upward Flow

scholarly journals Studies on MHD pressure drop and heat transfer of helium-lithium annular-mist flow in a transverse magnetic field.

1987 ◽  
Vol 30 (269) ◽  
pp. 1768-1775 ◽  
Author(s):  
Akira INOUE ◽  
Masanori ARITOMI ◽  
Minoru TAKAHASHI ◽  
Yosihito NARITA ◽  
Toshikazu YANO ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Heat Transfer ◽  
Pressure Drop ◽  
Transverse Magnetic Field ◽  
Transverse Magnetic ◽  
Mist Flow

scholarly journals NUMERICAL ANALYSIS OF HEAT TRANSFER ENHANCEMENT IN CONICAL-NOZZLE TURBULATORS INSERTED TUBE

2018 ◽  
Vol 13 (1) ◽  
pp. 7-17
Author(s):  
Sibel Güneş ◽  
Toygun Dağdevir ◽  
Orhan Keklikcioğlu ◽  
Veysel Özceyhan
Keyword(s):  
Heat Transfer ◽  
Numerical Analysis ◽  
Heat Transfer Enhancement ◽  
Conical Nozzle ◽  
Transfer Enhancement

scholarly journals New Calibration Parameter for Observations of Transverse Solar Magnetic Fields in the Fe I 5324.19 Å Line

1993 ◽  
Vol 141 ◽  
pp. 196-198
Author(s):  
Weihong Song ◽  
Guoxiang Ai
Keyword(s):  
Magnetic Field ◽  
Numerical Analysis ◽  
Magnetic Fields ◽  
Computational Model ◽  
Transverse Magnetic Field ◽  
Transverse Magnetic ◽  
Square Root ◽  
Solar Magnetic Fields ◽  
Doppler Broadening ◽  
Theoretical And Numerical Analysis

AbstractAdopting the computational model of papers I and II (Song et al. 1990, 1992) we have found that for a better fit of the center of the Fe I 5324.19 Å line, the effect of turbulent Doppler broadening has to be taken into account. Through theoretical and numerical analysis we conclude that the square root of the modulus of Stokes Q and U is an appropiate observational parameter to represent the transverse magnetic field, since it is approximately linearly proportional to the strength of the transverse magnetic field for suitable positions of the filter passband.

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