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Solar Dynamics
Results: 616

#	Item
131	Introduction to Turbulence and Heating in the Solar Wind Ben Chandran University of New Hampshire NASA LWS Summer School, Boulder, CO, 2012 Add to Reading List Source URL: www.heliophysics.ucar.edu Language: English - Date: 2012-06-07 12:04:50 Plasma physics Turbulence Magnetohydrodynamic turbulence Magnetohydrodynamics Alfvén wave Plasma Solar wind Sun James Clerk Maxwell Prize in Plasma Physics Physics Space plasmas Fluid dynamics
132	Venus Transit of 2012 Observed by the Helioseismic and Magnetic Imager (HMI) on board the Solar Dynamics Observatory (SDO) Sébastien Couvidat and the HMI team PICARD Workshop, September 25-26, 2013 Add to Reading List Source URL: smsc.cnes.fr Language: English - Date: 2013-11-14 08:24:50 Physics Venus Solar Dynamics Observatory Spaceflight Distortion Point spread function Astronomical unit Sun Astronomy Optics Space
133	Microsoft PowerPoint - thermal.ppt Add to Reading List Source URL: www.heliophysics.ucar.edu Language: English - Date: 2010-12-14 17:05:35 Physics Sun Light sources Astronomy Atmospheric dynamics Corona Solar wind Heliosphere Wind Space plasmas Plasma physics Astrophysics
134	Curation of meteorites in the NASA Johnson Space Center, Houston, Texas BEVAN M. FRENCH Solar System Exploration Division National Aeronautics and Space Administration Add to Reading List Source URL: s3.amazonaws.com Language: English - Date: 2011-05-06 05:15:29 Planetary science Meteorite Lunar meteorite Fluid dynamics Moon rock ANSMET Achondrite Chondrite Lunar and Planetary Institute Meteorite types Meteorites Astronomy
135	On Becoming a Scientist, Studying the Earth and the Sun Add to Reading List Source URL: www.leif.org Language: English - Date: 2012-11-29 06:54:30 Space Plasma physics Light sources Geomagnetism Space science Solar Dynamics Observatory Solar observatory Solar wind Comet tail Physics Space plasmas Astronomy
136	Shocks: Homework 1. Solar wind with Mach number Msw ≫ 1 hits the Earth’s magnetosphere. Assume the magnetic field in the wind is small enough to be neglected. A simplified of the day-side magnetosphere. Flow streamli Add to Reading List Source URL: www.vsp.ucar.edu Language: English - Date: 2012-06-04 12:37:41 Aerodynamics Fluid mechanics Plasma physics Planetary science Shock waves Magnetopause Magnetosheath Mach number Bow shock Physics Space plasmas Fluid dynamics
137	Energy spectrum of solar cosmic rays * G.A. Bazilevskaya Lebedev Physical Institute, Russian Academy of Sciences SEE-2005 Add to Reading List Source URL: www.iono.noa.gr Language: English - Date: 2005-11-04 19:09:08 Plasma physics Dynamics Fermi acceleration Fusion power Solar energetic particles Plasma Corona Solar flare Alfvén wave Physics Astrophysics Space plasmas
138	Using 2012 Venus transit for solar metrology Marcelo Emilio(1), Sebastian Couvidat(2), Rock Bush(3), Jeff Kuhn(4), Isabelle SchollObservatório Astronômico - Universidade Estadual de Ponta Grossa, Av. General Ca Add to Reading List Source URL: smsc.cnes.fr Language: English - Date: 2015-02-23 09:47:00 Astrometry Venus Plasma physics Space plasmas Astronomical transit Transit of Venus Solar Dynamics Observatory Astronomical unit Eclipse Astrology Astronomy Astrological aspects
139	The Constant Size and Shape of the Sun R. I. Bush Stanford University M. Emilio Universidade Estadual de Ponta Grossa, Parana, Brazil Add to Reading List Source URL: smsc.cnes.fr Language: English - Date: 2015-02-23 09:44:15 Physics Plasma physics Solar telescopes Space plasmas Solar Dynamics Observatory Spaceflight Sun Star Passive solar building design Astronomy Light sources Space
140	2012 LWS Heliophysics Summer School Problem Set on Turbulence and Heating in the Solar Wind 1. Turbulent Heating. Matthaeus & Goldstein (JGR, 87, 6011, 1982) analyzed an interval of slow-solar-wind data taken by instrum Add to Reading List Source URL: www.vsp.ucar.edu Language: English - Date: 2012-06-05 11:11:33 Plasma physics Water waves Fluid dynamics Corona Sun Turbulence Solar wind Plasma Proton Physics Space plasmas Light sources

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