What is a Solar Flare?

Aug. 11, 2023

A powerful solar flare disrupted radio and navigation signals across North America recently.

About Solar Flare:

  • A solar flare is an intense burst of radiation coming from the release of magnetic energy associated with sunspots.
  • Flares are our solar system’s largest explosive events. 
  • They are seen as bright areas on the sun, and they can last from minutes to hours.
  • In a matter of just a few minutes, they heat the material to many millions of degrees and produce a burst of radiation across the electromagnetic spectrum, including from radio waves to x-rays and gamma rays.
  • Although solar flares can be visible in white light, they are often more readily noticed via their bright X-ray and ultraviolet emissions.
  • Effect on Earth:
    • The intense radiation emitted during a solar flare can affect satellite communications, disrupt radio signals, and even pose a risk to astronauts in space.
    • Additionally, the increased solar radiation can lead to geomagnetic storms, which may impact power grids and cause auroras (northern and southern lights) at lower latitudes.

What is a Geomagnetic Storm?

  • A geomagnetic storm is a major disturbance of Earth's magnetosphere.
  • These storms result from variations in the solar wind  that produces significant changes in the currents, plasmas, and fields in Earth’s magnetosphere.
  • The solar wind conditions that are effective for creating geomagnetic storms are sustained (for several hours) periods of the high-speed solar wind and a southward-directed solar wind magnetic field (opposite the direction of Earth’s field) at the dayside of the magnetosphere.
  • The largest such storms are associated with solar coronal mass ejections (CMEs), where a billion tons or so of plasma from the sun, with its embedded magnetic field, arrives at Earth. 

Key Facts about Coronal Mass Ejections (CMEs):

  • Solar flares are different to 'coronal mass ejections' (CMEs), which were once thought to be initiated by solar flares.
  • CMEs are large expulsions of plasma and magnetic field from the Sun’s corona that propagates outward into interplanetary space.
  • Although some are accompanied by flares, it is now known that most CMEs are not associated with flares.
  • The blast of a CME carries about a billion tons of material out from the Sun at very high speeds of hundreds of kilometers per second.