  Brightenings observed in the solar extreme-ultraviolet (EUV) images are
generally interpreted as signatures of micro- or nanoflares occurring at the
transition region or coronal temperatures. Recent observations with the Extreme
Ultraviolet Imager (EUI) on board Solar Orbiter have revealed the smallest of
such brightenings (termed campfires) in the quiet-Sun corona. Analyzing EUI 174
{\AA} data at a resolution of about 400 km on the Sun with a cadence of 5 s
from 30-May-2020, we report here a number of cases where these campfires
exhibit propagating signatures along their apparent small (3-5 Mm) loop-like
structures. Measured propagation speeds are generally between 25 km s$^{-1}$
and 60 km s$^{-1}$. These apparent motions would be slower than the local sound
speed if the loop plasma is assumed to be at a million Kelvin. Furthermore,
these brightenings exhibit non-trivial propagation characteristics such as
bifurcation, merging, reflection and repeated plasma ejections. We suggest that
these features are manifestations of the internal dynamics of these small-scale
magnetic structures and could provide important insights into the dynamic
response ($\sim$40 s) of the loop plasma to the heating events as well as into
the locations of the heating events themselves.
