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The top documents tagged [coronal loops]
Solar Observer 1
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Solar Observer 1
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HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL A.Stepanov (Pulkovo Observatory, St.Petersburg) V.Zaitsev (Institute of Applied Physics,
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II. MAGNETOHYDRODYNAMICS (Space Climate School, Lapland, March, 2009) Eric Priest (St Andrews)
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Instructor Notes These images correspond to the layers of the Sun discussed in the Features of the Sun – 3D Sun lesson. Layers – Photosphere:
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CH. 29.2 – Solar Activity CH. 29 - MARQUES. Terms to know… Sunspot Prominence Granules solar flare coronal mass ejection aurora
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National Science Foundation: NSF and Space Weather Rich Behnke Division of Atmospheric and Geospace Sciences June 21, 2011
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Magnetic fields in the photosphere and heliosphere: structure, statistical parameters, turbulent state Valentyna I. Abramenko Big Bear Solar Observatory
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Xu et al., ApJ 607, L131, 2004: or, how do flare footpoints work? First flare observations in the infrared 1.56 nominally is as deep as deep can be (the
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The Dynamic Evolution of Quiet Sun Magnetic Fields in the Solar Atmosphere W.P. Abbett, Space Sciences Laboratory, Univ. of California, Berkeley
[email protected]
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Andrea Dupree SAO/CfA New England Space Science Consortium (NESSC) March 1, 2006 Some Stellar Problems of Interest to Solar Physics Global properties
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Feb. 2006HMI/AIA Science Team Mtg.1 Heating the Corona and Driving the Solar Wind A. A. van Ballegooijen Smithsonian Astrophysical Observatory Cambridge,
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