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Therefore an index based on ULF wave power could better characterize solar wind magnetosphere interaction than KP, Dst, AE, etc. indices which described mainly quasi-study state condition of the system.
Until recently, subsequent studies neglected ionospheric Hall current effects on ULF waves.
Kato and Tamao (1956) examined the effect of the ionosphere Hall conductivity on ULF waves.
In this paper we highlight the effects of ionospheric Hall conductance on ULF wave interaction with the magnetosphere-ionosphere-atmosphere-ground system, an important factor recognised by Kato and Tamao (1956).
Caution in extrapolating the abundant data on ULF composition confirmed in sheep [ 36] to the bovine model is required.
iTRAQ analysis was carried out on ULF recovered from pregnant heifers on Days 13, 16 and 19 (n=4 per day) to identify quantitative changes in the protein content (Proteome factory, Berlin, Germany).
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Recent thought on the origin of ULF waves (Kivelson, 2006) has mainly focused on field-line resonances or origin through excitation on the flanks of the magnetosphere and usually under more active solar wind conditions, notably of higher speed.
It is expected to shed light on the propagation of ULF waves from the outer magnetosphere, through the ionosphere and down to Earth.
The recently revived interest in Hall current effects on the transition of ULF waves from the magnetosphere through to the ground have been investigated using one-dimensional model approximations.
Of the 12 candidate genes which encode for putatively secreted proteins and whose expression was modulated in the endometrium during the estrous cycle and early pregnancy, 5 were detected by either iTraq or nano LC MS/MS analysis of ULF collected on either Days 13, 16 or 19 of pregnancy.
This is one of the key physics of ULF waves in the terrestrial magnetosphere.
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