Why Space Weather Matters and How Forecasting Will Improve in the DSCOVR Era Doug Biesecker, NOAA/NWS/Space Weather Prediction Center Space Weather is a growing enterprise, with growing recognition of its importance inside and outside government. ...
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Magnetic Influences on Coronal Heating and the Solar Wind Lauren Woolsey, Harvard University Abstract The physical mechanism(s) that generate and accelerate the solar wind have not been conclusively determined after decades of study, though not...
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New Tools for Galactic Archaeology from the Milky Way Gail Zasowski, John Hopkins University One of the critical components for understanding galaxy evolution is understanding the Milky Way Galaxy itself — its detailed structure and...
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Do star formation laws break in the center of the Galaxy? Betsy Mills, University of Arizona I will review our understanding of molecular gas conditions in the central 500 parsecs of the Milky Way, and summarize recent studies that find that the Galactic center deviates...
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Interface Region Imaging Spectrograph Views of How the Solar Atmosphere is Energized Dr. Bart De Pontieu, Lockheed Martin At the interface between the Sun’s surface and million-degree outer atmosphere or corona lies the chromosphere. At...
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Antarctic high altitude balloon observations of solar flares: Life and work on the ice Dr. Hazel Bain, University of California, Berkeley The Gamma-Ray Imager/Polarimeter for solar flares (GRIPS) instrument is a balloon-borne telescope designed to...
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Determining the size of coronal bright points using cross-correlation methods Laurel Farris Share this:TweetPrint
A Faint Flux-Limited LAE Sample at z = 0.3 Isak Wold, UT Austin Observational surveys of Lya emitters (LAEs) have proven to be an efficient method to identify and study large numbers of galaxies over...
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Dark Sky Images Ken Naiff Ken, an retired engineer, is a highly technically skilled and artistic astrophotographer. He will be sharing some of his work and elaborating on the technical methods and processing techniques he...
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