Evidence of Saturn's magnetic field anomaly from Saturnian kilometric radiation high-frequency limit

1991 ◽  
Vol 96 (A8) ◽  
pp. 14129-14140 ◽  
Author(s):  
Patrick Galopeau ◽  
Arturo Ortega -Molina ◽  
Philippe Zarka
1980 ◽  
Vol 3 ◽  
Author(s):  
H. Chang ◽  
I. J. Lowe ◽  
R. J. Karlicek

ABSTRACTMeasurements of T1 (Bo = 0.94T), and T1r as a function of temperature have been carried out on a LaNi5H7 sample at 4 different rotating magnetic field values. The T1 and T1r data are consistent with earlier data by Karlicek and Lowe [3,4], in which an asymmetry in the slopes of the log T1r vs. T−1 plot was found. The new data has been analyzed assuming a spectral density function J(ω,τc) of form J(ω, τc) = A(τc)B(Ω)F(ωτc), with τc = τc∞ exp(Ea/kT). This assumption leads to a spectral density function that fits all our data well, with Ea = 39 KJ/gm-Atom H, and J(ω)∼ Wω−1.35 in the high frequency limit. This Ea agrees well with the Ea obtained from diffusion constant measurements.


Soft Matter ◽  
2017 ◽  
Vol 13 (43) ◽  
pp. 7897-7906 ◽  
Author(s):  
Bram Schroyen ◽  
James W. Swan ◽  
Peter Van Puyvelde ◽  
Jan Vermant

The dispersion quality of colloidal dispersions is quantified by analysing the hydrodynamic stress contributions in the high frequency limit.


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