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Meteoroid Engineering Model (MEM)A Meteoroid Model for the Inner Solar SystemIn an attempt to overcome some of the deficiencies of existing meteoroid models, NASA's Space Environments and Effects Program sponsored a three year research effort at the University of Western Ontario. The resulting understanding of the sporadic meteoroid environment - particularly the nature and distribution of the sporadic sources - was then incorporated into a new meteoroid environment model (MEM) by members of the Space Environments Team at NASA's Marshall Space Flight Center. This paper discusses some of the revolutionary aspects of MEM which include: a) identification of the sporadic radiants with real sources of meteoroids, such as comets, b) a physics-based approach which yields accurate fluxes and directionality for interplanetary spacecraft anywhere from .2 AU to 2 AU, and c) velocity distributions obtained from theory and validated against observation. Use of the model, which gives penetrating fluxes and average impact speeds on the surfaces of a cube-like structure are also described, along with its current limitations and plans for future improvements.
Document ID
20040111321
Acquisition Source
Marshall Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
McNamara, H.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Jones, J.
(University of Western Ontario London, Ontario, Canada)
Kaufman, B.
(NASA Headquarters Washington, DC United States)
Suggs, R.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Cook, W.
(Morgan Research Corp. Huntsville, AL, United States)
Smith, S.
(Morgan Research Corp. Huntsville, AL, United States)
Date Acquired
August 21, 2013
Publication Date
January 1, 2004
Subject Category
Lunar And Planetary Science And Exploration
Meeting Information
Meeting: Meteoroids Conference 2004
Location: Ontario
Country: Canada
Start Date: August 1, 2004
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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