A team led by Southwest Research Institute (SwRI) has made the first direct detection of the source of magnetic reconnection. Analyzing data from NASA's Magnetospheric Multiscale (MMS) mission, scientists have observed how this explosive physical process converts stored magnetic energy into kinetic energy and heat.

"Just as in astronomy a new telescope like Hubble opens a new window on the universe, with MMS a new 'microscope' has opened a new window to clearly see reconnection," said Dr. James L. Burch, vice president of SwRI's Space Science and Engineering Division and MMS principal investigator.

"The four MMS satellites hone in on the role of electrons in magnetic reconnection, which allows two magnetic fields to interconnect. MMS measures the process 100 times faster than previously possible to clearly visualize the rapidly evolving process."

In late summer 2015, the four identically instrumented MMS spacecraft began to survey the magnetopause. In this boundary between the solar wind and Earth's magnetosphere, the scientists are searching for locations where the solar wind magnetic field and the terrestrial magnetic field reconnect.

In half of the over 4,000 magnetopause encounters, MMS has seen evidence of reconnection, but most often the spacecraft did not pass through the reconnection sites themselves. Then on October 16, 2015, MMS flew through the heart of a reconnection region.

"We hit the jackpot," says Dr. Roy Torbert, MMS deputy principal investigator and director of SwRI's Earth, Oceans, and Space office at the University of New Hampshire. "The spacecraft passed directly through the electron dissipation region, and we were able to perform the first-ever physics experiment in this environment."

MMS measures plasmas, hot ionized gases consisting of approximately equal numbers of positively charged ions and negatively charged electrons. The solar wind and Earth's magnetospheric plasmas are both magnetized.

For reconnection to occur, the plasmas become "demagnetized" - that is, the plasma and the magnetic field become decoupled. The critical and final stage in this process occurs in a relatively small region in space known as the "electron dissipation region." As the electrons become demagnetized, the magnetic fields of the Sun and the Earth interconnect and the solar wind and magnetospheric plasmas mix.

Magnetic reconnection - which occurs in both natural plasma environments and laboratory plasma and fusion experiments - is at the heart of space weather.

Reconnection is responsible for explosive solar events, such as solar flares and coronal mass ejections, and drives disturbances in Earth's space environment. Such disturbances produce spectacular auroras, but can also shut down electrical power grids and disrupt satellite-based communication and navigation systems.

"We've studied it theoretically, and we've simulated it with supercomputers. But up to now we haven't known what controls the conversion of magnetic energy into particle energy," said Burch. "We designed the MMS mission to use Earth's magnetosphere as a giant laboratory to perform the definitive experiment on reconnection."

Examining the data from the encounter, the MMS team saw a drop in the magnetic field to near zero, oppositely directed ion flows, accelerated electrons, an enhanced electric field, and a strong electrical current - all indications that the spacecraft had entered the dissipation region.

The telltale signature of reconnection, however, was a spike observed in the electric power generated by the electrons. "This was the 'smoking gun' for reconnection," explains Burch. "It was theoretically predicted but never seen until MMS."

Another feature observed for the first time by MMS as it traversed the dissipation region was a rapid change in the electrons as they streamed into the dissipation region and were accelerated outward along field lines opened during reconnection. This observation was the first definitive measurement of the interconnection of the solar and terrestrial magnetic fields.