Fig. 7
Schematic of the near-nucleus region obstructed by the bigger lobe. The solar EUV are unable to reach the region close to the neck when this configuration occurs. Credits for nucleus model: A. Beth, Imperial College London, CDPP, VESPA, NAVCAM/ESA, and dimensions: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/ INTA/UPM/DASP/IDA.
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