Suggested Searches

6 min read

Discovering Bonus Science With NASA’s Magnetospheric Multiscale Spacecraft

The four Magnetospheric Multiscale spacecraft are flying out of their element. The spacecraft have just completed a short detour from their routine science — looking at processes within Earth’s magnetic environment — and instead ventured outside it, studying something they were not originally designed for.

For three weeks, MMS studied the solar wind — the stream of supersonic charged particles flung around the solar system by the Sun — to better understand what’s known as turbulence in plasmas, the heated, electrified gases that make up 99 percent of ordinary matter in the universe. Turbulence is the chaotic motion of a fluid. It shows up in daily life everywhere from eddies in a river to smoke from a chimney, but it is incredibly hard to study because it’s so unpredictable and it remains one of the least well understood disciplines in all of physics. The mini-campaign will provide scientists with an up close and in-situ view to push the frontiers of the field.

But to take these groundbreaking measurements, MMS had to operate in an entirely new way — and MMS scientists and engineers designed a clever way to allow the spacecraft to study the solar wind with unprecedented accuracy, testing the limits and versatilities of MMS’ capabilities.

Opening New Doors

The Magnetospheric Multiscale mission, MMS, was launched in 2015 to study magnetic reconnection — the explosive snapping and forging of magnetic field lines, which flings high-energy particles around Earth. MMS was built with state-of-the-art instruments that take measurements with nearly 100 times better resolution than previous instruments. After two years of studying magnetic reconnection in Earth’s magnetic environment — the magnetosphere — on the dayside, MMS elongated its orbit to begin looking at reconnection behind Earth, away from the Sun, where it’s thought to spark the auroras.

Since MMS has completed its original mission goals, it’s now taking time in its extended mission to tackle some new science objectives. Understanding turbulence, which is one of NASA’s prime science objectives, is the first mini-campaign MMS plans to undertake.

“We would like to make a lot of these mini-campaigns in the future if this one is successful, which it’s already shaping up to be,” said Bob Ergun, researcher at the Laboratory for Atmospheric and Space Physics in Boulder, Colorado, who heads the new campaign. “MMS is a very, very powerful observatory with incredibly sensitive instruments on it and we’re trying to maximize their use to study these other priority sciences.”

Thinking Outside of the Magnetosphere

Studying the solar wind is best done from in the solar wind, but most of the time, the four MMS spacecraft orbit within or on the edge of Earth’s magnetosphere — where the magnetic field creates a buffer that protects the spacecraft from the solar wind. Occasionally, however, routine orbital adjustments, used to maintain MMS’ elongated orbit, take it well outside. This year, a boost to the spacecraft orbit is taking MMS entirely out of Earth’s magnetic environment and past the bow shock — a region where the supersonic solar wind slams into Earth’s magnetosphere. At such a distance, MMS passes through the solar wind itself, which allows a window of time to study the region’s turbulence.

Studying the solar wind is nothing like studying magnetic reconnection, but can be done with the same instruments that measure magnetic and electric fields. MMS is equipped with some of the most precise instruments ever flown in space, but in order to use them to study the solar wind, some adjustments first need to be made.

Infographic describing changes in MMS formation for first mini-campaign. MMS is shown in its original position, with its four antenna pointed parallel ad perpendicular to the edges of the graphic. Then it shows them in the campaign position, tilted 15 degrees to the right. It also shows the fleet of satellites in their original formation, forming a triangular pyramid. Then it shows them in their campaign formation, in a straight line.
This infographic compares the four MMS spacecraft’s normal orientation and formation to the orientation and formation for the mission’s first mini-campaign to study turbulence in the solar wind.
Credits: NASA’s Goddard Space Flight Center/Mary Pat Hrybyk-Keith

Download MMS’ mini-campaign infographic as pdf

Normally MMS flies in a pyramid-shaped formation called a tetrahedron, which allows all four spacecraft to be equally separated. As they flew through the solar wind, the spacecraft were instead arranged in what scientists call a “string of pearls.”  Flying perpendicular to the wind, the spacecraft followed one after another, each offset at distances of 25 to 100 kilometers (about 15.5 to 62 miles) from their neighbor. This allows scientists to see how much the solar wind varies over different distances.

However, as the spacecraft travel through the supersonic solar wind they create a wake behind them, just like a boat. This wake is not a natural feature in the solar wind, so the MMS scientists want to avoid having their instruments, which spin at the end of long booms, dragged through it. To make precise measurements unencumbered by the wake, the spacecraft were each tilted up 15 degrees. The tilt lifts the spinning booms up from travelling behind the spacecraft through the wake.

This angle allows scientists to get better data, but it comes with a cost. As a result of the tilt, the solar array doesn’t get as much light, meaning the spacecraft’s power is reduced by a few watts each. The tilt also puts thermal stress on the spacecraft, since the top of each gets hotter than the bottom. For a short campaign however, these effects won’t permanently affect the spacecraft.

Old Spacecraft, New Tricks

The data MMS gathered in this campaign will be some of the most accurate measurements of turbulence in the solar wind ever made. The research will also complement the work being done by NASA’s Parker Solar Probe, which flies through the Sun’s atmosphere studying the origins of the solar wind. While Parker Solar Probe measures the initial turbulence in the solar wind, MMS measured the aftermath when it reaches Earth.

“Almost all of the astrophysical plasmas we look at around the Sun, stars, black holes, accretion disks, jets, are all extremely turbulent, so by understanding it around Earth we understand it elsewhere,” Ergun said.

Ultimately this mini-campaign will also serve as a test case for what MMS is capable of doing in the future. Learning the nuances of MMS’ formations and tilt angles will allow the scientists to better understand MMS’s range of abilities, which may open the door up for other types of scientific campaigns as well.

Related Links

By Mara Johnson-Groh
NASA’s Goddard Space Flight Center, Greenbelt, Md.