Fig. 6.

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ADIM data product for the omnidirectional particle flux and anisotropy for a solar electron event observed by SEPT on board STEREO B on 14 August, 2010. From top to bottom: differential directional particle flux including estimated uncertainty ranges as shaded areas that are barely visible because of the large extent of the logarithmic y-axis, nominal μ-value (solid lines) and extent of μ-response (shaded area), omnidirectional particle flux, and anisotropy. In the panels for the omnidirectional flux and anisotropy, the black dots represent the median value of the respective distributions determined by ADIM. The red bars indicate the corresponding uncertainty ranges that are obtained by applying 95% confidence intervals. The green and purple bars mark time-periods where ADIM did not yield a result (we give further details in Sect. 8). The gray shaded areas in the anisotropy panel indicate anisotropy values which cannot be obtained by ADIM.
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