Total power uGMRT (550−850 MHz) images of Abell 2744 at different resolutions (5″, top left; 10″, top right; 15″, bottom left; 25″, bottom right). The known diffuse emission sources, namely the main relic (R1), the fainter relics (R2, R3, and R4), and the extended halo are recovered in our new uGMRT observations. The radio emission at the center of the halo apparently shows a cone-like morphology. The image properties are given in Table 2. Here, panel top left, top right, bottom left and bottom right correspond to IM9, IM10, IM12, and IM15, respectively. Contour levels are drawn at [1, 2, 4, 8, …] × 3.5 σ_rms. In these images there is no region below −3 σ_rms. The beam size is indicated in the bottom left corner of the each image.