MIAMI, modeling of the magnetosphere-ionosphere-atmosphere system final report on NASA grant NAGW5-1097.

Cover of: MIAMI, modeling of the magnetosphere-ionosphere-atmosphere system |

Published by National Aeronautics and Space Administration, National Technical Information Service, distributor in [Washington, DC, Springfield, Va .

Written in English

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Edition Notes

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Other titlesMIAMI :, Modeling of the magnetosphere-ionosphere-atmosphere system.
Series[NASA contractor report] -- NASA/CR-208287., NASA contractor report -- NASA CR-208287.
ContributionsUnited States. National Aeronautics and Space Administration.
The Physical Object
Pagination1 v.
ID Numbers
Open LibraryOL17595603M

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National Aeronautics and Space Administration.;]. Magnetosphere-Ionosphere-Atmosphere Coupling. Overview. but also provide support for other modeling efforts by allowing access to the database of input data and intermediary products.

The system will also be designed to be extensible, allowing additional data products and models to be integrated into the system. Page A1. THE MAGNETOSPHERE, IONOSPHERE, AND ATMOSPHERE. Appendix A1 was largely developed by the following workshop group: James Slavin (Group Leader), R.

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Magnetosphere, region in the atmosphere where magnetic phenomena and the high atmospheric conductivity caused by ionization are important in determining the behaviour of charged particles. The Earth, in contrast to Mars and Venus, has a significant surface magnetic field (approximately gauss).

Search the world's most comprehensive index of full-text books. My library. associated plasmas are added to the system. Similarly, the multi‐fluid MHD modeling of the magnetosphere-ionosphere-atmosphere system book by Kidder et al.

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A magnetosphere is a region of space surrounding an astronomical object in which charged particles are affected by that object's magnetic field.

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Enter and Address, Intersection or Landmark to locate an area or property. Turn layers on and off from the Layer View List. Use the Map Tools to navigate and interact with the map. @article{osti_, title = {Introduction to the ionosphere and magnetosphere}, author = {Ratcliffe, J A}, abstractNote = {Processes involved in the formation of the ionosphere and magnetosphere are discussed.

The nature of the ionospheric layers and phenomena such as geomagnetism, ionospheric currents, ionospheric storms, and solar disturbances are covered. College of Administrative Science, Department of Management Information Systems and Management Science, University of Alabama, Huntsville, AL.Modeling Magnetospheric Impact on the Ionosphere: Status and Challenges for the Upcoming Solar Cycle J.

Raeder, D. Larson, W. Li, A. Vapirev Space Science Center, University of New Hampshire T. Fuller-Rowell, N.

Maruyama NOAA & CIRES M.-C. Fok, A. Glocer NASA/GSFC.Outside Saturn's magnetosphere, a million-mile-per-hour flow of electrically charged particles (electrons and ions) from the sun, called the solar wind, spreads out through the solar system.

When the solar wind encounters Saturn's own magnetic field, the protective bubble of Saturn’s magnetosphere forms.

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