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Dynamical zodiacal cloud models constrained by high resolution spectroscopy of the zodiacal light
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Moseley, S. H. Mather, J. C. Madsen, G. J. Reynolds, R. J. Ipatov, S. I. Kutyrev, A. S. |
| Copyright Year | 2005 |
| Description | We have developed a set of self-consistent dynamical models of the Zodiacal cloud, following the orbital evolution of dust particles. Three populations were considered, originating from the Kuiper belt, asteroids and comets. Using the models developed, we investigated how the solar spectrum is changed by scattering by the zodiacal cloud grains and compared the obtained spectra with the observations. |
| File Size | 253547 |
| Page Count | 2 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20050169817 |
| Archival Resource Key | ark:/13960/t4gn35h16 |
| Language | English |
| Publisher Date | 2005-01-01 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Solar Spectra Spectroscopy Dust High Resolution Scattering Kuiper Belt Clouds Meteorology Zodiacal Light Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |