What is a solar flare?
A solar flare is a sudden release of energy from the Sun, often associated with sunspots, that emits radiation across the electromagnetic spectrum.
Science / Space
Recent solar flares, including the strongest of 2025, have caused radio blackouts across multiple continents and sparked vibrant auroras. This increased solar activity signals the Sun is entering a more active phase of its 11-year cycle.
The recent surge in solar activity is part of the Sun’s natural 11-year cycle, which is now approaching its solar maximum. This period is characterized by increased sunspot activity and more frequent solar flares and coronal mass ejections (CMEs). The X2.7-class flare, the strongest of the year so far, caused immediate radio blackouts due to the burst of X-rays and extreme ultraviolet radiation ionizing Earth’s upper atmosphere.
While the immediate impact was short-lived, lasting about 10 minutes, the potential for further disruptions remains as the active sunspot region AR4087 rotates to face Earth directly. CMEs, if associated with these flares, could trigger geomagnetic storms, leading to more prolonged communication and navigation system disturbances, as well as enhanced auroras.
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A solar flare is a sudden release of energy from the Sun, often associated with sunspots, that emits radiation across the electromagnetic spectrum.
Solar flares are classified as A, B, C, M, and X, with each class representing a tenfold increase in energy.
A CME is a large expulsion of plasma and magnetic field from the Sun’s corona.
They can cause radio blackouts, geomagnetic storms, auroras, and disruptions to power grids and satellite communications.
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