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Size distribution of interplanetary iron and stony particles related with deep-sea spherules
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Yamakoshi, K. Matsuzaki, H. |
| Copyright Year | 1993 |
| Description | To study origin and evolution of the interplanetary dust, it is very important to investigate the size distribution. Here the changes of the size distributions of meteoroid particles due to the ablative effects during atmospheric entry were investigated by numerical computer simulation. Using the results, the pre-atmospheric size distributions of the interplanetary dust particles could be estimated from that of ablated spherules taken from deep-sea sediments. We are now analyzing deep-sea spherules from some aspects and examining if we could get any information about the interplanetary dust. |
| File Size | 149958 |
| Page Count | 2 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19940011915 |
| Archival Resource Key | ark:/13960/t9n34s14m |
| Language | English |
| Publisher Date | 1993-01-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Micrometeorites Iron Meteorites Computerized Simulation Deep Water Stony Meteorites Ocean Bottom Atmospheric Entry Ablation Spherules Particle Size Distribution Numerical Analysis Micrometeoroids Interplanetary Dust Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
