Computer Science
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986icar...68..377s&link_type=abstract
Icarus (ISSN 0019-1035), vol. 68, Dec. 1986, p. 377-394.
Computer Science
33
Asteroids, Comets, Interplanetary Medium, Particle Tracks, Zodiacal Dust, Density (Number/Volume), Grains, Particle Trajectories, Solar Flares, Stratosphere
Scientific paper
The possibility is explored whether an IDP (interplanetary dust particle) is cometary or asteroidal from measurements of the solar flare track density within its constituent mineral grains. Dust particles that are larger than 1 micron, when injected into the Solar System from comets and asteroids, will spiral into the sun due to the Poynting-Robertson effect. During the process of spiraling in, such dust particles accumulate solar flare tracks. The accumulated track density for a given dust grain is a function of the duration of its space exposure and its distance from the sun. Using a computer model, it was determined that the expected track density distributions from grains produced by comets are very different from those produced by asteroids. Individual asteroids produce populations of particles that arrive at 1 AU with scaled track density distributions containing 'spikes,' while comets supply particles with a flatter and wider distribution of track densities.
No associations
LandOfFree
Solar flare track densities in interplanetary dust particles The determination of an asteroidal versus cometary source of the zodiacal dust cloud does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Solar flare track densities in interplanetary dust particles The determination of an asteroidal versus cometary source of the zodiacal dust cloud, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar flare track densities in interplanetary dust particles The determination of an asteroidal versus cometary source of the zodiacal dust cloud will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1124553