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The influence of solar wind and geomagnetic indices on lower band chorus emissions in the inner magnetosphere

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Figure

Table 1
Figure 2. The figure depicts the legend for the solar wind parameters with the time lags selected by the error reductionratio algorithm
Figure 3. The figure follows the same format as Figure 1 but with the errorreduction ratio algorithm including second degree nonlinear terms.
Figure 6. The figure depicts the legend for the solar wind parameters and geomagnetic indices with the time lagsselected by the error reduction ratio algorithm

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