Comet 67P/Churyumov-Gerasimenko on 26 July 2015 (C)
![](https://cdn.sci.esa.int/documents/34878/35534/1567215217701-ESA_Rosetta_OSIRIS_NAC_20150726_c_625.jpg)
Date: 10 March 2016
Satellite: Rosetta
Depicts: Comet 67P/Churyumov-Gerasimenko
Copyright: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA
This image of Comet 67P/Churyumov–Gerasimenko was captured by Rosetta's OSIRIS narrow-angle camera on 26 July 2015 at 16:54 GMT from a distance of about 170 km.
Shortly before this image was taken, between 15:16 GMT and 15:41 GMT, the RPC-MAG magnetometer on Rosetta detected a sudden drop in the magnetic field, indicating a magnetic-field free region, or diamagnetic cavity. However, the OSIRIS images do not show any appreciable increase of outgassing over this interval of time, ruling out that a change in the comet’s activity might be linked to the formation of the cavity.
Scientists believe that a dynamic perturbation, or instability, that propagates and gets amplified along the boundary between the solar wind and the magnetic field-free cavity, caused the latter to grow in size, allowing Rosetta to detect it.