Medical Imaging Skills Harnessed to Understand the Sun

NCAR solar physicist Scott McIntosh busy at work in his lab, headphones at the ready.
(Image credit: NCAR)

Solar physicist Scott McIntosh studies the inner — and outer — workings of the sun, including oscillations in the Sun's corona known as Alfvén waves. Such waves transport energy outward from the surface of the sun, and by studying them, McIntosh and others are gaining more insight into the fundamental behavior of solar magnetic fields. The knowledge is helping scientists achieve a fuller understanding of how the Sun affects the Earth and the solar system. His work made headlines in 2007 and continues to break new ground with new findings. Below, McIntosh answers the ScienceLives 10 Questions. Name: Scott McIntosh Age: 35 Institution: NSF's National Center for Atmospheric Research (NCAR), High Altitude Observatory (HAO) Field of Study: Solar Physics

What inspired you to choose this field of study? I got into it by accident. I planned to get a Ph.D. in medical imaging, studying pre-stroke conditions. Knowing that I specialized in medical imaging techniques, a solar physics professor asked me to use those skills to help interpret ultraviolet (UV) light from the solar atmosphere. Deciphering this UV light provides information that’s useful for understanding the solar plasma — its temperature, density, and chemical makeup, among other characteristics, which in turn tells a lot about the sun as a system. I fell in love with the challenge of putting disparate pieces of information together to understand how the sun behaves. Due to its close connection to conditions on Earth, a solid understanding of the complex solar atmosphere and its output is critical.

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