'X and C': NASA's GOLD Mission discovers unusual patterns in Earth's ionosphere

Produced by: Tarun Mishra

Credit: NASA

GOLD Mission's  New Findings

NASA's Global-scale Observations of the Limb and Disk (GOLD) mission has discovered unexpected X and C-shaped structures within Earth's ionosphere, a critical layer for radio communication.

Credit: NASA

Role of the Ionosphere

The ionosphere, a layer of charged particles in the upper atmosphere, is influenced by sunlight ionization, which causes its density to fluctuate throughout the day.

Credit: NASA

GOLD's Observations

Launched in 2018, the GOLD geostationary satellite monitors these variations. It recently observed unusual X-shaped patterns in typically smooth plasma regions of the ionosphere.

Credit: NASA

Unexpected Discoveries

Previously, X-shaped patterns were seen during heightened space weather activity, like solar storms or volcanic eruptions. GOLD’s detection during geomagnetically quiet times suggests unknown factors at play.

Credit: NASA

Scientific Insights

Research scientist Fazlul Laskar from the University of Colorado’s Laboratory for Atmospheric and Space Physics noted the unexpected nature of these findings. His paper, published in the Journal of Geophysical Research: Space Physics in April, highlights these observations.

Credit: NASA

Lower Atmosphere Impact

The findings suggest that events in the lower atmosphere may significantly influence the ionosphere, more than extreme solar or volcanic activities.

C-Shaped Bubbles

Besides the X shapes, GOLD also detected C-shaped and reverse C-shaped bubbles in the plasma, positioned unusually close together, which indicates unexpected changes in wind patterns.

Credit: NASA

Ongoing Research

Deepak Karan, a LASP research scientist, emphasized the importance of understanding these phenomena. Meanwhile, NASA continues its efforts to study the ionosphere with projects like the Atmospheric Perturbations Around The Eclipse Path (APEP), which launched sounding rockets during recent solar eclipses to measure changes in the upper atmosphere.

Credit: NASA