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The Solar Dynamics Observatory, or "SDO" for short, will gather data on the sun. From a geosynchronous orbit over a specially-constructed communications center in New Mexico, SDO will capture detailed images of the surface of the sun and take accurate measurements of changes in the sun's magnetic field and the solar wind.
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What mechanisms drive the quasi-periodic 11-year cycle of solar activity?
- How is active region magnetic flux synthesized, concentrated, and dispersed across the solar surface?
- How does magnetic reconnection on small scales reorganize the large-scale field topology and current systems and how significant is it in heating the corona and accelerating the solar wind?
- Where do the observed variations in the Sun's EUV spectral irradiance arise, and how do they relate to the magnetic activity cycles?
- What magnetic field configurations lead to the coronal mass ejections, filament eruptions, and flares that produce energetic particles and radiation?
- Can the structure and dynamics of the solar wind near Earth be determined from the magnetic field configuration and atmospheric structure near the solar surface?
- When will activity occur, and is it possible to make accurate and reliable forecasts of space weather and climate?
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You can learn much more about SDO at the mission web site, or by reading the official mission guide.