1980
DOI: 10.1016/0141-6359(80)90006-9
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Ultra stable magnetic suspensions for rotors in gravity experiments

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Cited by 12 publications
(1 citation statement)
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“…[la] the power loss to eddy currents goes as as. But since the kinetic energy is E = Iw2/2, and since the decay time is r* = E/E, (13) the decay-time spectra would be expected to go as w3' ', i.e., the effect would be most pronounced at low w . However, the skin depth of aluminium in all of our experiments exceeds the disc thickness so another w-dependence is presentone which we have not attempted to evaluate.…”
Section: A Fluctuations In Rotor Periodmentioning
confidence: 99%
“…[la] the power loss to eddy currents goes as as. But since the kinetic energy is E = Iw2/2, and since the decay time is r* = E/E, (13) the decay-time spectra would be expected to go as w3' ', i.e., the effect would be most pronounced at low w . However, the skin depth of aluminium in all of our experiments exceeds the disc thickness so another w-dependence is presentone which we have not attempted to evaluate.…”
Section: A Fluctuations In Rotor Periodmentioning
confidence: 99%