TY - GEN
T1 - Measurement of surface tension for molten silicon by electromagnetic levitation combined with static magnetic field
AU - Takenaga, Noriaki
AU - Hibiya, Taketoshi
AU - Fukuyama, Hiroyuki
AU - Watanabe, Masahito
AU - Ozawa, Shumpei
AU - Kobatake, Hidekazu
AU - Awaji, Satoshi
PY - 2006
Y1 - 2006
N2 - We have attempted to superimpose a static magnetic field to electromagnetic levitation, so as to investigate the possibility, whether application of a magnetic field can improve a surface tension measurement technique using an oscillating drop method. Movement of gravitational center of a droplet, which causes measurement error, was suppressed by applying a magnetic field. Amplitude of oscillation of the "Area" and "Sum" modes were attenuated vanishingly above 0.5T, whereas oscillation of the "Diff" mode exclusively remained although the amplitude became small in the magnetic field. Using frequencies of these three modes, frequency of surface oscillation of m = 0, m = ±1 and m = ±2 modes were derived. This suggests that oscillation of the m = 0 and m = ±1 modes are damped by applying a static magnetic filed. However, there still remains an argument, whether remained oscillation really corresponds to that of m = ±2 or that of axial rotation in the static magnetic field.
AB - We have attempted to superimpose a static magnetic field to electromagnetic levitation, so as to investigate the possibility, whether application of a magnetic field can improve a surface tension measurement technique using an oscillating drop method. Movement of gravitational center of a droplet, which causes measurement error, was suppressed by applying a magnetic field. Amplitude of oscillation of the "Area" and "Sum" modes were attenuated vanishingly above 0.5T, whereas oscillation of the "Diff" mode exclusively remained although the amplitude became small in the magnetic field. Using frequencies of these three modes, frequency of surface oscillation of m = 0, m = ±1 and m = ±2 modes were derived. This suggests that oscillation of the m = 0 and m = ±1 modes are damped by applying a static magnetic filed. However, there still remains an argument, whether remained oscillation really corresponds to that of m = ±2 or that of axial rotation in the static magnetic field.
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U2 - 10.2514/6.iac-06-a2.2.09
DO - 10.2514/6.iac-06-a2.2.09
M3 - Conference contribution
AN - SCOPUS:41149157976
SN - 9781605600390
T3 - AIAA 57th International Astronautical Congress, IAC 2006
SP - 627
EP - 632
BT - AIAA 57th International Astronautical Congress, IAC 2006
PB - American Institute of Aeronautics and Astronautics Inc.
T2 - AIAA 57th International Astronautical Congress, IAC 2006
Y2 - 2 October 2006 through 6 October 2006
ER -