Computer Science – Numerical Analysis
Scientific paper
Mar 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24..943m&link_type=abstract
In Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 2: G-M p 943-944 (SEE N94-16173 03-91)
Computer Science
Numerical Analysis
Ablation, Atmospheric Entry, Computerized Simulation, Interplanetary Dust, Iron Meteorites, Micrometeorites, Particle Size Distribution, Spherules, Stony Meteorites, Deep Water, Micrometeoroids, Numerical Analysis, Ocean Bottom
Scientific paper
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.
Matsuzaki Hiroyuki
Yamakoshi Kazuo
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