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Sunquakes Reveal The Solar Furnace
Dublin - Apr 01, 2003 Most people are familiar with the fact that sensitive instruments known as seismographs can detect earthquakes taking place many hundreds or thousands of miles away. By studying the waves from these tremors, scientists can find out about the conditions deep inside our rocky planet. In the same way, astronomers are now able to measure millions of sound waves that propagate throughout the Sun, causing it to vibrate or ring like a bell. This technique, known as helioseismology, is the solar equivalent of terrestrial seismology. On Monday 7 April, Dr. John Leibacher (U.S. National Solar Observatory) will highlight recent results from helioseismology studies during a presentation to the UK/Ireland Solar Physics Meeting in Dublin. These will include new views of the rapidly changing "sub-surface solar weather" and the far side of the Sun, as well as prospects for seeing finer and deeper details within the Sun and other stars. "Unimaginable 25 years ago, helioseismology today allows us to 'see' into the otherwise invisible interior of the Sun," said Dr. Leibacher. "This has enabled us to overthrow some theories, corroborate others, and pose many more new questions as we finally get a glimpse of how things work. "We are now testing fundamental theories of physics and astrophysics, substantially advancing our knowledge of the Sun's structure and dynamics," he added. "We are also beginning to measure significant temporal variations ranging from the scale of the eleven-year solar sunspot cycle right down to 'solar weather' variations on the scale of a day. "Recent observations have been producing some remarkable results on flows of gas that we can image below the surface of the Sun. For example, we are now seeing strong subsurface winds flowing into groups of sunspots, which change from day to day. "These sunspots are the sources of the strong magnetic fields which give rise to explosions on the surface. These, in turn, produce all sorts of terrestrial effects, from the aurora borealis, to fluctuations in navigational satellite signals, to power outages, and in the longer term they may influence Earth's climate. "With the discovery of these flows, we may be getting close to understanding the real nature of sunspots, with the tantalising prospect of being able to predict their occurrence. We can already utilise helioseismic imaging to detect sunspot groups on the far side of the Sun, before they rotate onto the visible hemisphere. "It has been an exhilarating ride and we are excited to see what the next turn will reveal," he said. Community Email This Article Comment On This Article Related Links Solar Subsurface Weather Solar Farside Imaging Transit Of Mercury Across The Sun In May 2003 Global Oscillation Network Group Royal Astronomical Society SpaceDaily Search SpaceDaily Subscribe To SpaceDaily Express Solar Science News at SpaceDaily
From 'Macro' To 'Micro' � Turbulence Seen By Cluster
Paris (ESA) Aug 11, 2005Thanks to measurements by ESA's Cluster mission, a team of European scientists have identified 'micro'-vortices in Earth's magnetosphere. |
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