Fig. C.1
VMDB (top), VMN (middle), and CMOR 38 MHz (bottom) intensity maps of the Orionids (left) and η-Aquariids (right). For each apparition of the shower presented in Appendices A and B, the activity profile is normalized by the corresponding maximum ZHR determined in Sect. 6.3.1 (reminded by the black curve at the right of the map).
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