Processes in Earth’s upper atmosphere create bright swaths of color known as airglow, as seen here in an image taken from the International Space Station. Credit: NASA
New research using data from 
NASA’s GOLD mission – short for Global-scale Observations of the Limb and Disk – saw a surprising asymmetric motion in one of the twin bands of charged particles that form in Earth’s atmosphere at night. GOLD’s unique perspective (right) made this observation possible, as other types of measurements made from ground-based instruments (left) can’t see changes that happen over open waters. The red dots show the peak of the electron band as measured by ground-based sensors that measure total electron content, while the black dots show the peak of the electron band measured by GOLD. Towards the end of the visualization, the measured peaks appear in different places. Credit: NASA’s Scientific Visualization Studio
This means the ionosphere and upper atmosphere are shaped by a host of complex factors, including space weather conditions – such as geomagnetic storms, driven by the Sun – and terrestrial weather. These regions also act as a highway for many of our communications and navigation signals. Changes in the ionosphere’s density and composition can muddle the signals passing through, like radio and GPS.
From its vantage point on a commercial communications satellite in geostationary orbit, GOLD makes hemisphere-wide observations of the ionosphere about every 30 minutes. This unprecedented birds-eye view is giving scientists new insights into how this region changes.
Mysterious movement
One of the nighttime ionosphere’s most distinctive features are twin bands of dense charged particles on either side of Earth’s magnetic equator. These bands – called the Equatorial Ionization Anomaly, or EIA – can change in size, shape, and intensity, depending on the conditions in the ionosphere.
The bands can also move position. Until now, scientists have relied on data captured by satellites passing through the region, averaging measurements over months to see just how the bands might be shifting in the long term. But short-term changes were more difficult to track.
Before GOLD, scientists suspected that any quick changes that happen in the bands would be symmetrical. If the northern band moves north, the southern band makes a mirror motion south. One night in November 2018, though, GOLD saw something that challenged this idea: the southern band of particles drifted southward, while the northern band remained steady – all in less than two hours.
The shape of Earth’s magnetic field (represented by orange lines in this data visualization) near the equator drive charged particles (blue) away from the equator, creating two dense bands just north and south of the equator known as the equatorial ionization anomaly. Credit: NASA’s Scientific Visualization Studio
This isn’t the first time scientists have seen the bands move like this, but this shorter event – only about two hours, compared to a more typical six to eight hours seen prior – was seen for the first time, and could only have been observed by GOLD. The observations are outlined in a paper published on December 29, 2020, in the Journal of Geophysical Research: Space Physics.
The symmetrical drifting of these bands is caused by rising air that drags charged particles along with it. As night falls and temperatures cool, warmer pockets of air surge upwards. The charged particles carried within these warmer air pockets are bound by magnetic field lines, and for those pockets near Earth’s magnetic equator the shape of Earth’s magnetic field means that upward motion also pushes the charged particles horizontally. This creates the symmetrical northward and southward drift of the two charged particle bands.
The exact cause of the asymmetric drift observed by GOLD is still a mystery – though Cai suspects the answer lies in some combination of the many factors that shape the motion of electrons in the ionosphere: ongoing chemical reactions, electric fields, and high-altitude winds blowing through the region.
Though surprising, these findings can help scientists peer behind the curtain of the ionosphere and better understand what drives its changes. Because it’s impossible to observe every process with a satellite or ground-based sensor, scientists rely heavily on computer models to study the ionosphere, much like models that help meteorologists predict weather on the ground. To create these simulations, scientists code in what they suspect are the underlying physics at work and compare the model’s prediction to observed data.
Before GOLD, scientists got that data from occasional passing satellites and limited ground-based observations. Now, GOLD gives scientists a bird’s-eye view.
Reference: “Observation of Postsunset OI 135.6 nm Radiance Enhancement Over South America by the GOLD Mission” by Xuguang Cai, Alan G. Burns, Wenbin Wang, Liying Qian, Jing Liu, Stanley C. Solomon, Richard W. Eastes, Robert E. Daniell, Carlos R. Martinis, William E. McClintock and Inez S. Batista, 29 December 202, Journal of Geophysical Research: Space Physics.
DOI: 10.1029/2020JA028108