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Table 3.

Correlation of SRT time differences with heliocentric distance for impulsive events, filtered for different additional parameters.

Filtering STIX main HXR peak RPW type III onset


criteria no. C p no. C p
all impulsive 85 0.30 ± 0.09 0.008 86 0.34 ± 0.10 0.0023

single peak/burst 49 0.29 ± 0.13 0.065 29 0.30 ± 0.16 0.13
multiple peaks/bursts 36 0.29 ± 0.15 0.092 57 0.37 ± 0.13 0.01

high anisotropy 45 0.17 ± 0.13 0.31 44 0.44 ± 0.13 0.004
medium anisotropy 21 0.48 ± 0.20 0.03 22 0.41 ± 0.26 0.062

well-connected 47 0.23 ± 0.14 0.15 42 0.19 ± 0.15 0.24
poorly connected 19 0.42 ± 0.16 0.088 17 0.57 ± 0.20 0.039

ambient SW 42 0.52 ± 0.10 0.0005 44 0.46 ± 0.14 0.002
IP structure 15 0.27 ± 0.17 0.39 13 0.46 ± 0.16 0.13

Notes. The time differences refer to VDA SRTs with respect to the main STIX HXR peak and the RPW type III onset. Shown are the numbers of events, the Pearson correlation coefficients C, and the p-values p.

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