  We investigate the asymmetric propagation of 100 TeV electrons (whose
radiation mainly concentrates on 20--30 TeV) in turbulent magnetic fields
around pulsars, using GPU-accelerated simulations to explore their trajectories
and interactions within pulsar wind nebulae and the interstellar medium. Key
results include the identification of ``mirage'' sources indicating significant
offsets in high-energy emissions from their originating pulsars, challenging
the results of traditional symmetric diffusion models. By varying parameters
like source distance, magnetic field strength, and electron injection spectral
index, the study delineates their effects on observable phenomena such as the
probability that a source has at least one mirage around it, as well as the
source separation. Our results offer insights into some puzzling sources
observed recently by the Large High Altitude Air Shower Observatory (LHAASO),
and shed light on the cosmic-ray transport mechanism in the interstellar
medium.
