Solar wind - PDFSEARCH.IO - Document Search Engine

Solar wind
Results: 2293

#	Item
491	TR&T Update Mona Kessel LWS Deputy Program Scientist Heliophysics Division MOWG October 2006 Add to Reading List Source URL: lws-trt.gsfc.nasa.gov Language: English - Date: 2012-09-12 17:54:28 Astronomy Astrophysics Solar wind Heliosphere Magnetosphere Sun Coronal mass ejection Aurora Corona Space plasmas Physics Plasma physics
492	CME Propagation Author : Dr. Anand Balaraman, Department of Physics, Georgia Southern University. Email: Add to Reading List Source URL: www.vsp.ucar.edu Language: English - Date: 2014-03-27 14:52:44 Space Plasma physics Sun Jets Planetary science Coronal mass ejection Solar wind Heliosphere Corona Space plasmas Astronomy Physics
493	WIND ENERGY SOLAR ENERGY BIOMASS ENERGY MARINE ENERGY TRANSMISSION STORAGE Add to Reading List Source URL: www.res-australia.com Language: English - Date: 2014-06-03 07:02:34 Technology Renewable Energy Systems Renewable energy in the United Kingdom Wind power Renewable energy commercialization Renewable energy Wind farm Sustainable energy Offshore wind power Energy Low-carbon economy Environment
494	2012 LWS Heliophysics Summer School Problem Set on the Three Solar Wind 1 Estimating coronal temperatures using Parker model In the lecture we saw that the speed of the solar wind near Earth at 1 AU ranges from about 27 Add to Reading List Source URL: www.heliophysics.ucar.edu Language: English - Date: 2012-06-04 12:37:41 Astrophysics Astronomy Sun Light sources Corona Solar wind Plasma Wind Alfvén wave Space plasmas Physics Plasma physics
495	National Wind and Solar PV SEA: Renewable Energy EIA Applications Received before December 2012 _ Technology Legend Technology Powerlines Co-Generation Add to Reading List Source URL: www.sawea.org.za - Date: 2013-07-26 07:23:13
496	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.heliophysics.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
497	HSS-magnetosphere-toffoletto Add to Reading List Source URL: www.heliophysics.ucar.edu Language: English - Date: 2011-07-28 11:47:48 Plasma physics Astronomy Planetary science Jets Geomagnetism Magnetosphere Space weather Solar wind Ionosphere Space plasmas Physics Astrophysics
498	Microsoft PowerPoint - HSS-year1Schedule27jul.ppt Add to Reading List Source URL: www.vsp.ucar.edu Language: English - Date: 2010-12-14 17:05:41 Physics Sun Space Space science Heliophysics International Heliophysical Year Solar wind Heliosphere Solar flare Space plasmas Plasma physics Astrophysics
499	1. The magnetic moment of Earth is approximately 31,000 nT- RE3 . The solar wind has a bulk velocity of 400 km/sec and a density of 5 cm-3 at 1 AU. Assume a very simple model of Earth’s magnetopause in which it is a pl Add to Reading List Source URL: www.heliophysics.ucar.edu Language: English - Date: 2012-06-04 12:42:45 Astronomy Planetary science Plasma physics Magnetopause Solar wind Magnetosheath Bow shock Magnetic field Magnetosphere Physics Space plasmas Astrophysics
500	Aab. Space Rex. Vol. 17, No. 415, pp280, 1996 CopyrightCo.%‘~ Printed in Great Britain. All ri8hts resewedl $9.50 + 0.00 Pergamon Add to Reading List Source URL: cosray.phys.uoa.gr Language: English Physics Light sources Astronomy Sun Corona Solar cycle Sunspot Solar wind Space plasmas Plasma physics Astrophysics

UPDATE