CMEs are huge bursts of coronal plasma threaded with intense magnetic fields ejected from the Sun over the course of several hours. CMEs arriving at Earth can generate geomagnetic storms, which can cause anomalies in and disruptions to modern conveniences such as electronic grids and GPS systems. Coronagraphs are instruments that block out light emitted by the Sun's surface so that its outer atmosphere, or corona, can be observed.
"SwSCOR is a short, externally occulted coronagraph with a novel 1.5-stage occultation scheme that enables darker, wider-field imaging than a single multi-disk occulter alone," said SwRI's Dr. Craig DeForest, who is leading the study. "Its Arago spot suppressor redirects the major source of diffracted stray light - the Arago spot - formed by the occulter itself. This design enables imaging closer to and/or farther from the Sun than comparably sized instruments with conventional occultation."
Stray light is the largest challenge of coronagraph design. Coronal structures a few degrees away from the Sun are a billion times fainter than the Sun itself. Diffraction injects stray light into the optics as sunlight scatters around the occulter in front of the instrument. Multi-disk occulters cut stray light by many orders of magnitude in the current generation of single-stage coronagraphs. Adding more disks yields more occultation but tightens the machining or assembly tolerances.
"SwRI is investigating several novel occulter designs," DeForest said. "Preliminary laboratory experiments with our latest prototype indicate a more than 10-fold improvement over similar-geometry multi-disk designs in use today, while improving manufacturability and alignment tolerances."
SwRI designed SwSCOR using internal funding, incorporating heritage processes and facilities from the development of the Polarimeter to Unify the Corona and Heliosphere mission's Wide-Field Imager (PUNCH/WFI). DeForest is the principal investigator of PUNCH, a NASA Small Explorer (SMEX) mission set to launch in 2025, which is designed to better understand how the mass and energy of the Sun's corona become the solar wind that fills the solar system.
"We prototyped and tested key elements of SwSCOR in SwRI's stray light cleanroom facility," DeForest said. "It will directly measure the 3D trajectory of halo CMEs, eliminating the strongest ambiguity in arrival time forecasting: confusion between wide, slow CMEs and narrow, fast CMEs."
Related Links
Solar Science at SwRI
Solar Science News at SpaceDaily
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