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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 ofthis movement is still unknown. Areas with high mass densities such as galacticsuperclusters seem to be one of the causes of this flow. There are severalmethods for simulating the motion of local clusters, one of which is the bulkflow. The bulk current can be seen as a mass movement of a large part of theuniverse. This anisotropy at the local scale seems to have the same origin asthe anisotropy at the larger scale. In this paper, anisotropies on both smalland large scales were investigated using chameleon fields. The data used areType Ia supernovae (Pantheon catalog for a total of 1,048 supernovae inredshift (0.15<z<2.3)). The results showed that on a smaller scale (less than150 MPa) the direction of motion of the local group galaxies is the same as thedirection of the bulk, and on larger scales, the direction of the bulk currentis the same as the direction of the current of dark energy dipole.

Can Chameleon fields be the source of both the dark energy dipole and the CMB dipole?