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Progress in our understanding of cometary dust tails
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Sekanina, Z. |
| Copyright Year | 1976 |
| Description | Various analytical techniques are employed to analyze observations on the character, composition, and size distribution of solid particles in cometary dust tails. Emphasized is the mechanical theory that includes solar gravitational attraction and solar radiation pressure to explain dust particle motions in cometary tails, as well as interactions between dust and plasma. |
| File Size | 2136512 |
| Page Count | 50 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19760014001 |
| Archival Resource Key | ark:/13960/t29931215 |
| Language | English |
| Publisher Date | 1976-01-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Particle Size Distribution Cosmic Dust Particle Motion Astronomical Models Comet Tails Solar Radiation Solar Wind Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
