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The relationship between the flare power and the changes in the H' and β during solar flares of varying intensities has been presented by Thomson et al. (2005).
The degradation by high laser intensities has been observed in polycrystalline MAPbI3 films [28, 29], which is mainly due to the low thermal conductivity of MAPbI3 [30].
Considering that the standardization of 67Ga does not depend on the decay scheme parameters (except for the half-life), the measurement of the γ-emission intensities has been performed.
The relationship between the changes in the D-region, H′ and β, and the flare power during solar flares of varying intensities has been reported by a number of researchers (e.g., Thomson and Clilverd 2001; McRae and Thomson 2004; Thomson et al. 2005; Tan et al. 2014).
Due to unspecific binding, the global background adjustment method robust multi-array average (RMA) expression measure, which ignores the MM intensities, has been developed [ 19].
Moreover, micro stimulation at low current intensities has been shown to yield saccades with smaller-than-optimal amplitudes (Van Opstal et al. 1990), which cannot be explained by an ideal center-of-gravity computation.
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The intensities have been shifted for clarity.
Applying this new methodology, resource intensities have been assessed and quantified for 22 major copper mines.
The peak intensities have been obtained by fitting the peaks assuming Lorentzian distribution.
Rainfall intensities have been measured by means of a heated siphon rain gauge.
The emission intensities have been normalized by the blue emission peak of the feather-like samples.
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