September 06, 2008 22:18:05 UT - Mission Day: 4663 - DOY: 250
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Solar flares set the Sun quaking

 

Data from SOHO's VIRGO instrument show clearly that powerful starquakes ripple around the Sun in the wake of the mighty solar flares that explode above its surface. The observations give solar physicists a new insight into a long running solar mystery, and may even provide a way of studying other stars, too.

The outermost quarter of the Sun's interior is a constantly churning maelstrom of hot gas. Turbulence in this region causes ripples that criss-cross the solar surface, making it heave up and down in a patchwork pattern of peaks and troughs.

SOHO has proved to be an exceptional spacecraft for studying this phenomenon. Discovering how the ripples move around the Sun has provided valuable information about the Sun's interior conditions. A class of oscillations called the 5-minute oscillations with a frequency of around 3 millihertz have proven particularly useful.

According to conventional thinking, the 5-minute oscillations can be thought of as the sound you would get from a bell sitting in the middle of the desert and constantly being touched by random sand grains, blown on the wind. What Christopher Karoff and Hans Kjeldsen, both at the University of Århus, Denmark, saw in the data, however, was very different. "The signal we saw was like someone occasionally walking up to the bell and striking it, which told us that there was something missing from our understanding of how the Sun works," Karoff says.

So they began looking for the culprit and discovered an unexpected correlation with solar flares. It seemed that when the number of solar flares went up, so did the strength of the the 5-minute oscillations. "The strength of the correlation was so strong that there can be no doubt about it," says Karoff. A similar phenomenon is known on Earth in the aftermath of large earthquakes. For example, after the 2004 Sumatra-Andaman Earthquake, the whole Earth rang with seismic waves like a vibrating bell for several weeks.

The correlation is not the end of the story. Now the researchers have to work to understand the mechanism by which the flares cause the oscillations. "We are not completely sure how the solar flares excite the global oscillations," says Karoff. In a broader context the correlation suggests that, by looking for similar oscillations within other stars, astronomers can monitor them for flares. Already, Karoff has used high-technology instruments at major ground-based telescopes to look at other Sun-like stars. In several cases, he detected the tell-tale signs of oscillations that might originate from flares.

"Now we need to monitor these stars for hundreds of days," he says. That will require dedicated spacecraft, such as the recently launched COROT mission. The hard work, it seems, is just starting.

 

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Last modification: Friday, 09-Jul-2004 14:44:29 EDT

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3D view of a CME heading towards Earth


A CME similar to the one on the previous page, heading almost directly towards Earth, observed by LASCO C2. The size of the Sun is indicated by a circle, and the x-marked circle on the Sun shows the origin of the CME. Panel a shows the total intensity (darker means more intensity) as imaged directly by LASCO. Only the narrow lower end of the "lightbulb" shape is visible - the widest portion has expanded beyond the field of view, whereas the front part and the core are too dim to be seen or hidden behind the occulter. Panel d is a topographic map of the material shown in panel a. The distance from the plane of the Sun to the material is colour coded - the scale in units of solar radii is shown on the side. Panels b and c show the intensity as it would have appeared to an observer positioned to the side of the Sun or directly above it, respectively.

Picture credits: SOHO/LASCO (ESA & NASA) and Thomas Moran
Instrument: LASCO (Large Angle and Spectrometric Coronagraph)


Last modification: Friday, 09-Jul-2004 14:44:29 EDT
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