Fig. 5.


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Same as Figure 4, but comparison of rotational variation from the TIM TSI (black), SOLSTICE UV (red), and SIM UV (blue dot) at 240 nm during 2003–2013. The normalized amplitudes are estimated with an intrinsic mode function I, by removing the mean of I over the analysis time and by dividing with its standard deviation, for TSI and UV, respectively. Numbers in right and left axes indicate the normalized amplitude of the rotational variations of TSI and UV.

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