Experiment hurtled into aurora above Norway by NASA rocket

Funded by the National Aeronautics and Space Administration (NASA), the Rocket Experiment for Neutral Upwelling, or RENU, aimed to measure the complex, underlying physics behind the phenomena of "satellite drag. The launch required conditions that enhance the transfer of solar wind energy to Earth's magnetic field and, eventually, into our atmosphere to create the stunning northern lights or aurora. With the Sun becoming increasingly active after an unusually long quiet cycle, the researchers were banking that aurora would occur to allow a launch during the November 28 – December 12 window.

Neutral upwelling has been known to exist since the earliest days of the space program when observers noted increased "drag" on Earth-orbiting satellites during periods of solar activity. At the time, the effect was largely attributed to a complex heating process that causes the upper part of the Earth's atmosphere, or thermosphere, to swell up horizontally on a scale of hundreds of kilometers.

More recent observations have shown that neutral upwelling can also occur on much smaller scales and more localized in the cusp region – two "funnels" of magnetic field lines that allow a small amount of solar wind to reach the top of the atmosphere and produce the auroral glow. This upwelling process is more vertical in nature and appears to be associated with auroral processes.

The RENU instrument payload was designed to take an array of measurements, including those for neutral gas, electric and magnetic fields, and precipitating particles, and the new data acquired during the flight will provide information essential for the advancement of understanding the process. The launch location in the far northern polar region was chosen so that the experiment could take place in total darkness.

Although the effect of satellite drag can negatively impact a spacecraft's orbit over time, which is a concern for certain low-orbit, strategic satellites, Lessard stresses this was not the primary motivation for the experiment.

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Pictured is a portion of the Kjell Henriksen Observatory (KHO), which is operated by the University Center of Svalbard and provides downrange support for many sounding rocket missions launched from the Andøya Rocket Range. KHO is near Longyearbyen on the island of Svalbard about 435 miles north of Andøya Rocket Range in Andenes, Norway. The rocket's trajectory puts it precisely over KHO on Svalbard when the rocket is at apogee or its highest point. Photo by Njľl Gulbrandsen.

"From NASA's point of view this is a mission of pure science, we're trying to understand the processes behind neutral upwelling and how it is associated with visible aurora phenomena," says Lessard, associate professor at the UNH Institute for the Study of Earth, Oceans, and Space (EOS) and department of physics. He adds that RENU is taking a new scientific approach and is attempting to test, measure, and quantify "electron precipitation" that brings energetic particles down from high above the Earth and delivers energy into the upper atmosphere via Earth's magnetic field lines.

"This is the first time anyone has tried to measure these neutral particle enhancements at these altitudes and with this combination of instruments," Lessard says. He adds that it appears the team was successful in getting the rocket to transit a region of neutral density enhancement but because so much data is gathered during rocket launches (unlike satellites, vast amounts of data can be transmitted quickly back to Earth) it could take months to analyze the results.

The team of investigators also includes colleagues from the Aerospace Corporation, Dartmouth College, Cornell University, the U.S. Air Force Academy, NASA's Goddard Space Flight Center, and other collaborators, including those at the Kjell Henriksen Observatory (KHO), which is operated by the University Center of Svalbard.

An array of ground-based instrumentation located at KHO in the northernmost part of Norway complemented the rocket measurements. The data will be used to quantify neutral density enhancement, or regions of higher neutral atom density, and will also be used by theorists on the team to run mathematical models to gain insight into the heating and precipitation processes. Notes Lessard, "The instrumentation and science support provided from our colleagues at KHO has been invaluable."

Provided by University of New Hampshire