This study examines the variability of the ionospheric content during the period around the 2015 Saint Patrick magnetic storm and when equatorial plasma bubbles (EPBs) are observed during the quiet time over South America during two other events. It uses the ionospheric scales index map based on the disturbance ionospheric index (DIX). The results are compared to the traces of the ionograms obtained at three different ionospheric stations (Fortaleza, Campo Grande, and Cachoeira Paulista) in Brazil acquired in the same period and at the same time rate. The index is based on the TEC map developed at the "Brazilian Studies and Monitoring of Space Weather" (Embrace/INPE). It covers the whole South America (latitudes from 20°N to 60°S and longitudes from 90°W to 30°W) with 0.5°× 0.5°resolution cells (60 × 60 km 2). Among the results, the DIX map revealed some patches of "Disturbed" and "Weakly Disturbed" ionospheric conditions during the magnetically quiet time before the storm, which were associated with range and frequency Spread-F over the same area as observed in ionograms. Also, the information from the southern portion of the dip equator showed a transition from occurrences of Spread-F prior to sunrise to a condition favorable enough to develop a F3 layer after sunrise. Magnetic storms have also been investigated in a large number of works in several different ways. For instance, the Saint Patrick magnetic storm has been investigated by Astafyeva et al. (2015) using a global multi-instrumental overview of the ionospheric impact of this magnetic storm. Nevertheless, the map present in their Figure 2 has very low resolution. Besides, the maps presented in their Figure 5 have several gaps. In another portion of the study (e.g., Figure 4 that deals with sectoral analysis), they basically used profiles of NmF2 from a single station. In the other study, Venkatesh et al. (2017) did provide quite high-resolution maps, but TEC maps (see their Figures 6 and 9), not disturbances maps. For the disturbance, they used