Interaction of interplanetary dust particles with magnetic clouds

Retention of helium in subducted interplanetary dust particles.

Circumstellar aluminum oxide and silicon carbide in interplanetary dust particles

A systematic NanoSIMS isotope imaging study of sub-micrometer phases in interplanetary dust particles (IDPs) has led to the discovery of two presolar grain types that previously were observed only in primitive meteorites. A 350 · 600 nm Al2O3 grain has a large O enrichment and a slight O depletion, as well as a Mg excess due to the decay of extinct Al. Because of its relatively large size and p...

Magnetohydrodynamic simulation of the interaction 1 between two interplanetary magnetic clouds and its

synthesis of amido alkylnaphthols using nano-magnetic particles and surfactants

we used dbsa and nano-magnetic for the synthesis of amido alkylnaphtols.

Migration of interplanetary dust.

We numerically investigate the migration of dust particles with initial orbits close to those of the numbered asteroids, observed trans-Neptunian objects, and comet Encke. The fraction of silicate asteroidal particles that collided with the Earth during their lifetime varied from 11% for 100 micron particles to 0.008% for 1 micron particles. Almost all asteroidal particles with diameter d >/= 4...