NASA Measures Pulsating Aurora

This all-sky movie shows a time lapse of a pulsating aurora on Jan. 3, 2012. Scientists compared the video, taken in Poker Flat, Alaska, over the course of three minutes, with satellite measurements of the numbers and energies of electrons raining down from the magnetosphere to better understand how electrons transfer energy to the upper atmosphere and create the auroras. The black mark traces the satellite foot point—the place where the satellite is magnetically connected to the aurora—of the Defense Meteorological Satellite Program satellite.

Credits: NASA

In this study, published in the Journal of Geophysical Research, scientists compared ground-based videos of pulsating auroras–a certain type of aurora that appears as patches of brightness regularly flickering on and off–with satellite measurements of the numbers and energies of electrons raining down towards the surface from inside Earth’s magnetic bubble, the magnetosphere. The team found something unexpected: A drop in the number of low-energy electrons, long thought to have little or no effect, corresponds with especially fast changes in the shape and structure of pulsating auroras.

“Without the combination of ground and satellite measurements, we would not have been able to confirm that these events are connected,” said Marilia Samara, a space physicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and lead author on the study.

Pulsating auroras are so-called because their features shift and brighten in distinct patches, rather than elongated arcs across the sky like active auroras. However, their appearance isn’t the only difference. Though all auroras are caused by energetic particles–typically electrons–speeding down into Earth’s atmosphere and colliding brilliantly with the atoms and molecules in the air, the source of these electrons is different for pulsating auroras and active auroras.

 

This image of a colorful aurora was taken in Delta Junction, Alaska, on April 10, 2015. All auroras are created by energetic electrons, which rain down from Earth’s magnetic bubble and interact with particles in the upper atmosphere to create glowing lights that stretch across the sky.

 Image courtesy of Sebastian Saarloos

 

Active auroras happen when a dense wave of solar material–such as a high-speed stream of solar wind or a large cloud that exploded off the sun called a coronal mass ejection–hits Earth’s magnetic field, causing it to rattle. This rattling releases electrons that have been trapped in the tail of that magnetic field, which stretches out away from the sun. Once released, these electrons go racing down towards the poles, then they interact with particles in Earth’s upper atmosphere to create glowing lights that stretch across the sky in long ropes.

On the other hand, the electrons that set off pulsating auroras are sent spinning to the surface by complicated wave motions in the magnetosphere. These wave motions can happen at any time, not just when a wave of solar material rattles the magnetic field.

“The hemispheres are magnetically connected, meaning that any time there is pulsating aurora near the north pole, there is also pulsating aurora near the south pole,” said Robert Michell, a space physicist at NASA Goddard and one of the study’s authors. “Electrons are constantly pinging back and forth along this magnetic field line during an aurora event.”

The electrons that travel between the hemispheres are not the original higher-energy electrons rocketing in from the magnetosphere. Instead, these are what’s called low-energy secondary electrons, meaning that they are slower particles that have been kicked up out in all directions only after a collision from the first set of higher-energy electrons. When this happens, some of the secondary electrons shoot back upwards along the magnetic field line, zipping towards the opposite hemisphere.

When studying their pulsating aurora videos, researchers found that the most distinct change in the structure and shape of the aurora happened during times when far fewer of these secondary electrons were shooting in along hemispheric magnetic field lines.

“It turns out that secondary electrons could very well be a big piece of the puzzle to how, why, and when the energy that creates auroras is transferred to the upper atmosphere,” said Samara.

However, most current simulations of how the aurora form don’t take secondary electrons into account. This is because the energy of the individual particles is so much lower than the electrons coming directly from the magnetosphere, leading many to assume that their contribution to the glowing northern lights is negligible. However, their cumulative effect is likely much larger.

“We need targeted observations to figure out exactly how to incorporate these low-energy secondary electrons into our models,” said Samara. “But it seems clear that they may very well end up playing a more important role than previously thought.”

Measurements of the number and energies of electrons were made by two satellites that happened to be passing overhead during these pulsating aurora events: Reimei, a JAXA satellite tasked with studying auroras, and a satellite from the U.S. Department of Defense’s Defense Meteorological Satellite Program. The ground-based all-sky cameras–used to study both auroras and meteors–are operated at Poker Flat Research Range in Fairbanks, Alaska and the European Incoherent Scatter Scientific Association Radar Facility in Tromsø, Norway.

 

 

Susan Hendrix
NASA Goddard Space Flight Center