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Scientists Find Elusive Waves in Sun's Corona;
Discovery Can Help Unlock Secrets of Corona's Heat, Solar Storms

August 30, 2007

Steve TomczykSteve Tomczyk. [ENLARGE] (Photo by Carlye Calvin, ©UCAR. News media terms of use*)BOULDER—Scientists for the first time have observed elusive oscillations in the Sun's corona, known as Alfvén waves, that transport energy outward from the surface of the Sun. The discovery is expected to give researchers more insight into the fundamental behavior of solar magnetic fields, eventually leading to a fuller understanding of how the Sun affects Earth and the solar system.

The research, led by Steve Tomczyk of the National Center for Atmospheric Research (NCAR), is being published this week in Science.

"Alfvén waves can provide us with a window into processes that are fundamental to the workings of the Sun and its impacts on Earth," says Tomczyk, a scientist with NCAR's High Altitude Observatory.

Alfvén waves are fast-moving perturbations that emanate outward from the Sun along magnetic field lines, transporting energy. Although they have been detected in the heliosphere outside the Sun, they have never before been viewed within the corona, which is the outer layer of the Sun's atmosphere. Alfvén waves are difficult to detect partly because, unlike other waves, they do not lead to large-intensity fluctuations in the corona. In addition, their velocity shifts are small and not easily spotted.

Alfvén waves
Coronal Waves - Visuals & Multimedia Gallery
Scientists for the first time have observed elusive oscillations in the Sun's corona, known as Alfvén waves, by tracking the motions of coronal plasma (charged particles and gas) around the entire edge of the Sun. In this series of images and animations, NCAR's Coronal Multi-channel Polarimeter instrument, or CoMP, has captured the intensity of the light emitted from the solar corona (upper left), the line width or spectral extent over which the light is emitted (upper right), and the velocity (lower left). The oscillations of the plasma velocity are made clearer by filtering the velocity data to show only oscillations that recur periodically every five minutes. (lower right and still image, below). These motions are caused by the Alfvén waves. [View animation, QuickTime, 9.5MB] (Image courtesy

CoMP DopplerSee caption, above, for description. [ENLARGE]

"Our observations allowed us to unambiguously identify these oscillations as Alfvén waves," says coauthor Scott McIntosh of the Southwest Research Institute in Boulder. "The waves are visible all the time and they occur all over the corona, which was initially surprising to us."

Insights into the Sun

By tracking the speed and direction of the waves, researchers will be able to infer basic properties of the solar atmosphere, such as the density and direction of magnetic fields. The waves may provide answers to questions that have puzzled physicists for generations, such as why the Sun's corona is hundreds of times hotter than its surface.

The research also can help scientists better predict solar storms that spew thousands of tons of magnetized matter into space, sometimes causing geomagnetic storms on Earth that disrupt sensitive telecommunications and power systems. By learning more about solar disruptions, scientists may be able to better protect astronauts from potentially dangerous levels of radiation in space.

"If we want to go to the moon and Mars, people need to know what's going to happen on the Sun," Tomczyk says.

A powerful instrument

To observe the waves, Tomczyk and his coauthors turned to an instrument developed at NCAR over the last few years. The Coronal Multichannel Polarimeter, or CoMP, uses a telescope at the National Solar Observatory in Sacramento Peak, New Mexico, to gather and analyze light from the corona, which is much dimmer than the Sun itself. It tracks magnetic activity around the entire edge of the Sun and collects data with unusual speed, making a measurement as frequently as every 15 seconds.

The instrument enabled the research team to simultaneously capture intensity, velocity, and polarization images of the solar corona. Those images revealed propagating oscillations that moved in trajectories aligned with magnetic fields, and traveled as fast as nearly 2,500 miles per second.

In addition to Tomczyk and McIntosh, the research team included scientists from the National Solar Observatory, University of Notre Dame, Framingham High School in Massachusetts, University of Michigan, and NCAR.

About the article

Title: "Alfvén Waves in the Solar Corona"

Authors: S. Tomczyk, S.W. McIntosh, S.L. Keil, P.G. Judge, T. Schad, D.H. Seeley, J. Edmondson

Publication: Science, August 31, 2007

Alfvén wavesScientists for the first time have observed elusive oscillations in the Sun's corona, known as Alfvén waves, by tracking the motions of coronal plasma (charged particles and gas) around the entire edge of the Sun. In this series of images and animations, NCAR's Coronal Multi-channel Polarimeter instrument, or CoMP, has captured the intensity of the light emitted from the solar corona (upper left), the line width or spectral extent over which the light is emitted (upper right), and the velocity (lower left). The oscillations of the plasma velocity are made clearer by filtering the velocity data to show only oscillations that recur periodically every five minutes. (lower right and next image to the right). These motions are caused by the Alfvén waves. (Image courtesy Steve Tomczyk and Scott McIntosh, NCAR.)

CoMP Doppler

 

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The National Center for Atmospheric Research and UCAR Office of Programs are operated by UCAR under the sponsorship of the National Science Foundation and other agencies. Opinions, findings, conclusions, or recommendations expressed in this publication do not necessarily reflect the views of any of UCAR's sponsors.

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