TRACERS heliophysics mission enters Phase B

SwRI-managed TRACERS heliophysics mission enters Phase B
Two NASA sounding rockets carrying SwRI-developed ion instruments studied the electrodynamics of the polar cusp. The instruments will fly on TRACERS, a heliophysics mission to study how the Earth's and Sun's magnetic fields interact, set to launch in 2023. Credit: NASA/Jamie Adkins
NASA has approved the Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) mission to proceed to Phase B, which marks the transition from concept study to preliminary flight design. The satellites, led by the University of Iowa (UI) and managed by Southwest Research Institute, are set to launch in late 2023.

In addition to providing management and science services to UI, SwRI is developing the Analyzer for Cusp Ions (ACI) instrument, which will study how the magnetic fields of the Sun and the Earth interact through novel measurements in the polar cusps. Under a subcontract to Millennium Space Systems, SwRI is also managing the development of its two bus platforms, supporting instrument integration and testing, and conducting mission operations.

TRACERS will use two satellites to observe particles and fields at the Earth's northern magnetic cusp region—the region encircling the Earth's poles where our planet's magnetic field lines curve down toward Earth. Here, the magnetic field allows particles from the boundary between Earth's and interplanetary space to access the atmosphere.

"TRACERS is an exciting mission," said SwRI's Dr. Stephen Fuselier, a mission co-investigator leading the development of the ACI instrument. "We had the opportunity to do a test run of the mission and ACI when we flew NASA's TRICE-2 rockets in 2018 as a part of the international, multi-mission "Grand Challenge Initiative—Cusp" observational campaign. The data returned from that single pass through the cusp were amazing. We can't wait to get the data from thousands of cusp passes."

SwRI-managed TRACERS heliophysics mission enters Phase B
This false-color image of the Earth's magnetosphere illustrates the depression in magnetic field strength in the northern and southern cusps. SwRI has designed an ion instrument for the TRACERS mission to investigate the variability of magnetic reconnection by obtaining measurements in the cusps. Credit: NASA/GSFC/N. A. Tsyganenko/C. T. Russell

The cusp provides easy access to the Earth's boundary with interplanetary space allowing a unique perspective on how magnetic fields all around Earth interact with those from the Sun. In a process known as , the field lines explosively reconfigure, accelerating particles to velocities reaching a significant fraction of the speed of light.

Magnetic reconnection is responsible for explosive solar events, such as and , and drives disturbances in Earth's space environment. Such disturbances produce spectacular auroras, while the high-energy electromagnetic radiation they send toward Earth can also shut down electrical power grids and disrupt satellite-based communication and navigation systems.

TRACERS will be the first space mission to explore this process in the cusp with two satellites, providing observations of how processes change over both space and time. The cusp vantage point also permits simultaneous observations of reconnection throughout near-Earth . TRACERS will provide important context for the SwRI-led Magnetospheric Multiscale mission, which has been in Earth orbit for over five years gathering the first detailed, high-speed observations of reconnection events.

"Over the planned one-year mission, the identical satellites will be outfitted with a combined total of 10 instruments to measure the plasma and fields in over 3,000 cusp crossings," said SwRI's Ron Black, who is serving as the TRACERS mission manager. "This will allow us to determine variability over a wide range of solar wind conditions."


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Citation: TRACERS heliophysics mission enters Phase B (2020, June 22) retrieved 10 May 2021 from https://phys.org/news/2020-06-tracers-heliophysics-mission-phase.html
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