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Validation and applications of the POLAR codeThe Potentials of Large Objects in the Auroral Region (POLAR) code was written to model the charging of large spacecraft by auroral electrons in low polar orbit. It has also proven to be a powerful tool for analysis of active and voltage-plasma interactions. POLAR combines 3-D object definition, direct solution to Poisson's equation, space charge transport, and surface charge computation. Physical effects treated by POLAR include the plasma wake and ram, the geomagnetic field, ionization, sheath and barrier formation, and photo and secondary electron generation and transport. Polar development is complete and it is now available to the aerospace community. The methodology of POLAR is reviewed but concentration is on the applications of POLAR to physical problems and observations with the intent of demonstrating both the code's capabilities, and its limitations. These applications include the Space Shuttle, the Defense Meteorological Satellite Program (DMSP) satellites, sounding rockets, plasma chamber experiments, and things not yet flown.
Document ID
19920013123
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Cooke, David L.
(Phillips Lab. Kirkland AFB, NM., United States)
Katz, Ira
(Nova Univ. Dania, FL., United States)
Jongeward, Gary
(Nova Univ. Dania, FL., United States)
Lilley, John R., Jr.
(Nova Univ. Dania, FL., United States)
Tautz, Maurice
(RADEX, Inc., Bedford MA., United States)
Date Acquired
September 6, 2013
Publication Date
February 1, 1992
Publication Information
Publication: NASA. Johnson Space Center, 5th Annual Workshop on Space Operations Applications and Research (SOAR 1991), Volume 2
Subject Category
Spacecraft Design, Testing And Performance
Accession Number
92N22366
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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