Angular distributions of albedo protons at the near earth orbit
β Scribed by Wang, Kaiti; Huang, Ming-Huey A.
- Book ID
- 119673594
- Publisher
- American Geophysical Union
- Year
- 2008
- Tongue
- English
- Weight
- 518 KB
- Volume
- 113
- Category
- Article
- ISSN
- 0148-0227
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A recently published model of the Near Earth Object (NEO) orbital-magnitude distribution (Bottke et al., 2002, Icarus 156, 399-433.) relies on five intermediate sources for the NEO population: the Ξ½ 6 resonance, the 3 : 1 resonance, the outer portion of the main belt (i.e., 2.8-3.5 AU), the Mars-cro
The orbital and absolute magnitude distribution of the near-Earth objects (NEOs) is difficult to compute, partly because only a modest fraction of the entire NEO population has been discovered so far, but also because the known NEOs are biased by complicated observational selection effects. To circu