Overview of the C2-class flare observed at 08:46 UT on May 6, 2019. Panel a: continuum map showing the sunspot and the pores. Panel b: line-of-sight magnetic field as inferred from a Milne-Eddington inversion of the Fe I 6173.34 Å line. The color scale extends in the ±0.8 kG range, where black and white represent the negative and positive polarity, respectively. Panels c and d: chromospheric intensity maps, observed with the CRISP and CHROMIS instruments at the SST, showing bright flare ribbons at the flare footpoints. Panels e–i: AIA images observed in different channels, in logarithmic scale. The green and magenta contours represent the negative and positive polarity in the photosphere, respectively. A dashed white line and the “P1”, “P2”, and “P3” in panel c highlight the location of the pixels analyzed in the paper. Solar north, solar east, and the direction of the disk center are indicated by “N”, “E”, and “DC”, respectively.