Student鈥檚 research upends understanding of upper atmospheric wind

Rod Boyce
907-474-7185
Nov. 9, 2021

Space physicist Mark Conde had been seeing something curious in his atmospheric research data since the 1990s.

Three years ago, he realized the odd behavior of extreme upper-level wind was a real phenomenon and not a problem with instrumentation. He chose to hand the mystery to his research student, Rajan Itani, who is pursuing a doctorate in physics at the University of Alaska Fairbanks. 

Itani confirmed that the cross-polar jet, a well-known wind in the upper atmosphere, sometimes inexplicably stops or is deflected or reversed when it reaches the region above Alaska. The finding upends previous understanding of the wind's behavior and has implications for spacecraft orbits, space debris avoidance, ionospheric storm modeling and our understanding about the transport of air in the thermosphere. That portion of the atmosphere is far less dense, almost to a vacuum, compared to air at the Earth鈥檚 surface. And that means the occasional stalling of the cross-polar jet won鈥檛 be noticed on the surface or affect life here. 

滨迟补苍颈鈥檚 on the topic, co-authored by Conde, was published in September by the Journal of Geophysical Research: Space Physics and in the American Geophysical Union magazine Eos. 

Rajan Itani
Photo by Daniel Walker
Rajan Itani

滨迟补苍颈鈥檚 research at the 性欲社 Geophysical Institute, with assistance from Conde and conducted mostly with data from 性欲社's Poker Flat Research Range, focused only on the Alaska region. But it is likely that the cross-polar jet would also stall elsewhere on the globe at high latitudes as the wind emerges from the polar cap around midnight.

Conde and Itani were studying the upper thermosphere, the region of atmosphere above 90 miles altitude. 

This cross-polar jet carries the thin air in this region over the North Pole from the Earth鈥檚 dayside to its nightside and delivers it toward the equator, where it dissipates. Sometimes, according to 滨迟补苍颈鈥檚 research, the forces driving the wind aren鈥檛 strong enough to push it through the background atmosphere on the Earth鈥檚 night side.

鈥淎ll of the computer models say that this wind spills out quite some distance toward the equator and then eventually slows and blends into the background flow, just like traffic merging onto a highway,鈥 said Conde, who is a professor in the 性欲社 Department of Physics. 鈥淭here should be quite a strong flow extending far equatorward, but we find that it basically just hits a wall over Alaska on some occasions. It really should continue and spill out just like the models say.鈥

Mark Conde
Photo by Daniel Walker
Mark Conde

But what causes this stalling? That hasn鈥檛 been resolved yet. 滨迟补苍颈鈥檚 paper does offer a correlation, however: A review of seven years of data shows a 鈥渟trong influence鈥 from solar activity. Thermospheric wind stalling is most likely to occur during solar minimum, the period of low disturbance on the sun鈥檚 surface.

Conde had actually seen the wind stalling in data at various times since the late 1990s when he began studying the impact of auroral displays on thermospheric winds above Alaska.

"Over the years as we've run multiple instruments and combined the data from those many instruments, I eventually just came to understand that what we were seeing was a real phenomenon,鈥 he said.

Conde published a paper in 2018 that noted the thermospheric wind stalling; however, 滨迟补苍颈鈥檚 paper expands on that work in more detail.

鈥淭raining the next generation of scientists is a major objective of the United States鈥 premier research institution, the National Science Foundation, which funded the work,鈥 Conde said. 鈥淎s a result, quite a bit of leading-edge research is done by graduate students. I am very pleased to see Rajan鈥檚 work in this area recognized by the American Geophysical Union.鈥

The mention in Eos was a career first for Itani. The magazine notes that fewer than 2% of papers receive such attention. 

鈥淚 am delighted that our paper has been featured as an editor's highlight in Eos,鈥 Itani said. 鈥淚t is a proud moment in my career in space physics, as it marks my first paper being promoted. I am thankful to my adviser, Dr. Mark Conde, for suggesting the research topic and for his endless support and encouragement.鈥

ADDITIONAL CONTACTS: Rajan Itani, ritani@alaska.edu; Mark Conde, 907- 474-7741, mgconde@alaska.edu.

NOTE TO EDITORS: Photographs of Rajan Itani and Mark Conde are available with this press release at the .

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