First results from 2021 rocket launch shed light on aurora鈥檚 birth

Rod Boyce
907-474-7185
Dec. 19, 2024

Aurora over the 黑料社app
UAF photo by Eric Engman
The northern lights adorn the sky over the UAF Agricultural and Forestry Experiment Station early Sunday morning, April 21, 2024.

Newly published results from a 2021 experiment led by a 黑料社app scientist have begun to reveal the particle-level processes that create the type of auroras that dance rapidly across the sky.

The 鈥 KiNET-X 鈥 lifted off from NASA鈥檚 Wallops Flight Facility in Virginia on May 16, 2021, in the final minutes of the final night of the nine-day launch window.

UAF professor Peter Delamere鈥檚 analysis of the experiment鈥檚 results was published Nov. 19 in .

鈥淭he dazzling lights are extremely complicated,鈥 Delamere said. 鈥淭here鈥檚 a lot happening in there, and there鈥檚 a lot happening in the Earth鈥檚 space environment that gives rise to what we observe.

鈥淯nderstanding causality in the system is extremely difficult, because we don鈥檛 know exactly what鈥檚 happening in space that鈥檚 giving rise to the light that we observe in the aurora,鈥 he said. 鈥淜iNET-X was a highly successful experiment that will reveal more of the aurora鈥檚 secrets.鈥

One of NASA鈥檚 largest sounding rockets soared over the Atlantic Ocean into the ionosphere and released two canisters of barium thermite. The canisters were then detonated, one at about 249 miles high and one 90 seconds later on the downward trajectory at about 186 miles, near Bermuda. The resulting clouds were monitored on the ground at Bermuda and by a NASA research aircraft.

The experiment aimed to replicate, on a minute scale, an environment in which the low energy of the solar wind becomes the high energy that creates the rapidly moving and shimmering curtains known as the discrete aurora. Through KiNET-X, Delamere and colleagues on the experiment are closer to understanding how electrons are accelerated.

鈥淲e generated energized electrons,鈥 Delamere said. 鈥淲e just didn鈥檛 generate enough of them to make an aurora, but the fundamental physics associated with electron energization was present in the experiment.鈥

NASA sounding rocket carrying KiNET-X launches on May 16, 2021
NASA photo by Terry Zaperach
A BlackBrant XII sounding rocket carrying the KiNET-X experiment launches from NASA鈥檚 Wallops Flight Facility in Virginia on May 16, 2021.

The experiment aimed to create an Alfv茅n wave, a type of wave that exists in magnetized plasmas such as those found in the sun鈥檚 outer atmosphere, Earth鈥檚 magnetosphere and elsewhere in the solar system. Plasmas 鈥 a form of matter composed largely of charged particles 鈥 also can be created in laboratories and experiments such as KiNET-X.

Alfv茅n waves originate when disturbances in plasma affect the magnetic field. Plasma disturbances can be caused in a variety of ways, such as through the sudden injection of particles from solar flares or the interaction of two plasmas with different densities.

KiNET-X created an Alfv茅n wave by disturbing the ambient plasma with the injection of barium into the far upper atmosphere.

Sunlight converted the barium into an ionized plasma. The two plasma clouds interacted, creating the Alfv茅n wave.

That Alfv茅n wave instantly created electric field lines parallel to the planet鈥檚 magnetic field lines. And, as theorized, that electric field significantly accelerated the electrons on the magnetic field lines.

鈥淚t showed that the barium plasma cloud coupled with, and transferred energy and momentum to, the ambient plasma for a brief moment,鈥 Delamere said. 

The transfer manifested as a small beam of accelerated barium electrons heading toward Earth along the magnetic field line. The beam is visible only in the experiment鈥檚 magnetic field line data.

鈥淭hat鈥檚 analogous to an auroral beam of electrons,鈥 Delamere said.

He calls it the experiment鈥檚 鈥済olden data point.鈥

Barium clouds in the KiNET-X experiment
Photo courtesy Don Hampton
Ionization by the sun turns the green barium cloud of the KiNET-X experiment to purple over the Atlantic Ocean on May 16, 2021.

Analysis of the beam, visible only as a varying shades of green, blue and yellow pixels in Delamere鈥檚 data imagery, can help scientists learn what is happening to the particles to create the dancing northern lights.

The results so far show a successful project, one that can even allow more information to be gleaned from its predecessor experiments.

鈥淚t鈥檚 a question of trying to piece together the whole picture using all of the data products and numerical simulations,鈥 Delamere said.

Three UAF students doing their doctoral research at the UAF Geophysical Institute also participated. Matthew Blandin supported optical operations at Wallops Flight Facility, Kylee Branning operated cameras on a NASA Gulfstream III aircraft out of Langley Research Center, also in Virginia, and Nathan Barnes assisted with computer modeling in Fairbanks..

The experiment also included researchers and equipment from Dartmouth College, the University of New Hampshire and Clemson University.

ADDITIONAL CONTACT: Peter Delamere, padelamere@alaska.edu

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