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Flare differentially rotates sunspot on Suns surface_arxiv161002969.pdf

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Flare differentially rotates sunspot on Suns surface_arxiv161002969.pdf
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Flare and CME Properties and Rates at Sunspot Minimum_ Hugh S Hudson_ Yan Li_ SolStellAstroPhys_2003.pdf
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Flare-associated type III radio bursts and dynamics of the EUV jet from SDO AIA and RHESSI observations_ arxiv13042907v1.pdf
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Flare SOL2012-07-06_ on the origin of the circular polarization reversal between 17 GHz and 34 GHz_ arxiv170906252.pdf
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Flaring Solar Hale Sector Boundaries_ Leif Svalgaard_ Iain G Hannah_ arXiv10102710.pdf
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First Sunquake of Solar Cycle 24 Observed by Solar Dynamics Observatory_ AG Kosovichev_ arxiv11023954.pdf
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Forecasting a CME by Spectroscopic Precursor_ D Baker_ L van Driel-Gesztelyi_ L M Green_ 2011.pdf
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First Simultaneous Observation of H-alpha Moreton Wave, EUV Wave, and Filament Prominence Oscillations_ arxiv11125915.pdf
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Forward modeling of emission in SDO AIA passbands from dynamic 3D simulations_ Juan Martinez-Sykora_ Bart De Pontieu_ Paola Testa_ Viggo Hansteen_ arxiv11090704.pdf
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First Observation of Time Variation in the Solar-Disk Gamma-Ray Flux with Fermi_ arxiv150806276v1.pdf
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Fundamentals of Solar Astronomy_ Arvind Bhatnagar_ William Livingston_ 2005.pdf
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First Light of the Near-Infrared Narrow-Band Tunable Birefringent Filter at Big Bear Solar Observatory_ Wenda Cao_ Klaus Hartkorn_ Jun Ma_ Yan Xu_ Tom Spirock et al_ Solar Physics_ 2006.pdf
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G-band and Hard X-ray Emissions of the 2006 December 14 flare observed by Hinode SOT and RHESSI_ Kyoko Watanabe_ Sam Krucker_ Hugh Hudson_ Toshifumi Shimizu_ Satoshi Masuda_ Kiyoshi Ichimoto_ SolStellAstroPhys_2004.pdf
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Faculae at the poles of the Sun revisited_ infrared observations_ J Blanco Rodriguez_ F Kneer_ 2010.pdf
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Generation of electric currents in the chromosphere via neutral-ion drag_ V Krasnoselskikh_ G Vekstein_ H S Hudson_ S D Bale_ W P Abbett_ ApJ_2010.pdf
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Factors Affecting The Intensity of Solar Energetic Particle Events_ Nat Gopalswamy_ arxiv11092933.pdf
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Geoeffectiveness and efficiency of CIR, Sheath and ICME in generation of magnetic storms_ arxiv11091073.pdf
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Extending F107s Time Resolution to Capture Solar Flare Phenomena_ Ariel O Acebal_ 2008.pdf
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Geomagnetic Semiannual Variation Is Not Overestimated and Is Not an Artifact of Systematic Solar Hemispheric Asymmetry_ L Svalgaard_ GeoPhysResLetters_2011.pdf
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Explanation of the sea-serpent magnetic structure of sunspot penumbrae_ I N Kitiashvili_ L R Bellot Rubio_ TheAstrophysicalJournal_ 2010.pdf
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