  Recent research shows that the local group is moving toward (l,b)=(276,30)
relative to the cosmic background radiation at a speed of about $600 kms^{-1}$
which is known as the cosmic background radiation dipole. The exact cause of
this movement is still unknown. Areas with high mass densities such as galactic
superclusters seem to be one of the causes of this flow. There are several
methods for simulating the motion of local clusters, one of which is the bulk
flow. The bulk current can be seen as a mass movement of a large part of the
universe. This anisotropy at the local scale seems to have the same origin as
the anisotropy at the larger scale. In this paper, anisotropies on both small
and large scales were investigated using chameleon fields. The data used are
Type Ia supernovae (Pantheon catalog for a total of 1,048 supernovae in
redshift (0.15<z<2.3)). The results showed that on a smaller scale (less than
150 MPa) the direction of motion of the local group galaxies is the same as the
direction of the bulk, and on larger scales, the direction of the bulk current
is the same as the direction of the current of dark energy dipole.
