by Nielsen Engineering & Research, Inc., For sale by the National Technical Information Service in Mountain View, CA, [Springfield, Va .
Written in English
|Statement||by Stephen S. Stahara|
|Series||NASA-CR -- 173531, NASA contractor report -- 173531|
|Contributions||Nielsen Engineering & Research, United States. National Aeronautics and Space Administration|
|The Physical Object|
Application of a global solar wind/planetary obstacle interaction computational model: Earth, Venus, Mars, Jupiter and Saturn studies eBook: National Aeronautics and Space Administration NASA: : Kindle StoreAuthor: National Aeronautics and Space Administration NASA. Technical Report: Preliminary development of a global 3-D magnetohydrodynamic computational model for solar wind-cometary and planetary interactions. Preliminary development of a global 3-D magnetohydrodynamic computational model . The U.S. Department of Energy's Office of Scientific and Technical Information. ment and application of a computational model for the determina-tion of the detailed plasma and magnetic field properties of the global interaction of the solar wind with nonmagnetic terrestrial planetary obstacles. The theoretical method is based on an established single .
Scientists have discovered that oxygen ions from Earth's atmosphere are transported to the Moon once a month, during a five-day window when the lunar satellite passes through our planet's protective this time, the Moon passes behind Earth, getting a short reprieve from the blast of the Sun's solar wind – and is sprinkled with a stream of material fleeing Earth instead. Bibliographic Codes, Conference Proceedings Abbreviations This list contains the non-journal abbreviations for the ADS Abstracts Bibliographic Codes, including Conferences, Proceedings, Symposia, Meetings, Reports, and Books. February 9, Lecture 4 - Solar Wind and Planetary Magnetospheres Solar Wind Effects o Depends on magnetic field and atmospheric properties of object. o Planets with magnetic fields essentially have a dipole field (B(r) = M / r3). o Consider two types of magnetosphere: d magnetosphere - solar wind interaction creates a magnetosphere. Unfortunately, this book can't be printed from the OpenBook. If you need to print pages from this book, we recommend downloading it as a PDF. Visit to get more information about this book, to buy it in print, or to download it as a free PDF.
The importance of thermal electron heating in Titan's ionosphere: Comparison with Cassini T34 flyby global interaction model. of Titan, similar to the solar wind – planetary interaction. Report of the Panel on Solar and Heliospheric Physics. To grasp immediately the nature of the field of solar and heliospheric physics, one need only look at the striking image of the solar eclipse shown in Figure The solar atmosphere extends outward from the Sun’s surface, apparently without end. Icy satellites, Interplanetary Dust, Moon, Solar particles/Solar wind Astrobiology, Education/Public Outreach (EPO), Heliophysics, Space-based observing, Spectroscopy Robert Tokar. Magnetospheric Structure and Atmospheric Joule Heating of Habitable Planets Orbiting M-dwarf Stars. to drive an MHD model for the global. environment and the solar wind), planetary magneto-.