Abstract
Solar flares are strong radiation bursts, whereas large clouds of solar material and magnetic fields thaterupt at high speeds from the Sun are coronal mass ejections. Harmful radiation from a flare does notpass through the atmosphere of the Earth to physically impact humans on the ground, but can disrupt theatmosphere in the layer where GPS and communication signals travel. Flares generate results across theentire electromagnetic spectrum. They emit x-rays and ultraviolet radiation, which means extremely hightemperatures during a flash. Radio waves mean that tiny fractions of particles are accelerated to high levelsof energy. Most of the radiation is synchrotron radiation produced along magnetic field lines by electronstraveling along spiral paths. In this paper was monitored solar flare registered on February 25, 2015. Thisflare, which peaked at 00:49 am EDT from a sunspot called Active Region 1990 (AR1990), is classifiedas an X4.9-class flare. We have performed solar data analysis using the Python/SunPy tool. SunPy waschosen as the principle data analysis environment since it provides easy to use interfaces to the Virtual SolarObservatory (VSO).