Science Success Story

Total Solar Eclipse

XSEDE Allocations on Expanse Supercomputer Provided Sneak Peek of Extended Solar Corona

By Kimberly Mann Bruch, SDSC Communications


This set of images shows a special visualization of the three-dimensional (3D) magnetic field. By tracing magnetic field lines at extremely high resolution, astrophysicists can calculate a 3D map of the so-called squashing factor – a scientific measure designed to indicate the presence of complex structures in the magnetic field. They then integrate the map along the line-of-sight, with special weightings to create a composite that resembles solar eclipse images. This is intended to highlight the inherent complexity of the sun's magnetic field and its intimate connection to visible emission from the solar corona. Credit: Cooper Downs, Predictive Science, Inc.

On Saturday, December 4, a total eclipse of the sun occured at 07:33 (Universal Time) over Antarctica and parts of the South Pacific near the southern tip of Chile. The solar corona – visible to the naked eye only during a total eclipse – was viewable for just over one minute. Thanks to the handiwork of Predictive Science Inc. researchers, who ran simulations using Extreme Science and Engineering Discovery Environment (XSEDE) allocations on the Expanse supercomputer at the San Diego Supercomputer Center (SDSC) at UC San Diego, we had a preview of the spectacle before it even occurred.

 

Why It's Important

The researchers' prediction, posted November 27 – one week before totality, was based on a state-of-the-art computer simulation of the tenuous, magnetized outer atmosphere of the sun known as the solar corona. In addition to providing a sneak peek for eclipse chasers, such predictions aid scientists who are planning eclipse observations from the ground, sea and air. Eclipses also provide a unique opportunity for researchers to test the accuracy and predictive capability of physical models of the solar corona. Such models are essential for understanding how the corona is heated and how it drives the structure and dynamics of the inner-heliosphere, including Earth-affecting disturbances known as space weather.

"Because of the large core and memory count on Expanse nodes, we have the ability to run several cases of various degrees of complexity and size – some quite large – with rapid turnaround, which was essential for getting the final prediction together." – Cooper Downs, astrophysicist at Predictive Science, Inc.

How XSEDE Helped

"Expanse was an essential resource – especially because of its unique hardware architecture and rapid turnaround for mid-scale simulations," said Cooper Downs, an astrophysicist at Predictive Science, Inc. "Although we have allocations on other supercomputers, without Expanse we would have had to start everything several days earlier to make sure all the runs and renders could be completed on time. This would mean the solar observations used to drive the model would be even more out of date, risking the accuracy of the prediction."

Downs, whose research focuses on understanding thermodynamic and magnetic processes in the solar corona is particularly interested in the improvement and validation of numerical models through direct comparisons to observational data. He said that Expanse allows him to run larger simulations and create more accurate diagnostics. 

"Because of the large core and memory count on Expanse nodes, we have the ability to run several cases of various degrees of complexity and size – some quite large – with rapid turnaround, which was essential for getting the final prediction together," Downs said.

XSEDE allocation TG-MCA03T014 was utilized for the work on Expanse.

At a Glance:

  • Predictive Science Inc. researchers ran solar corona simulations using XSEDE allocations on the Expanse supercomputer at the San Diego Supercomputer Center at UC San Diego.

  • The simulations provided a sneak peek of the eclipse and helped scientists plan observations from the ground, sea and air. 

  • These models aid in understanding how the corona is heated and how it drives the structure and dynamics of the inner-heliosphere, including Earth-affecting disturbances known as space weather.