Sentence examples for grains masses from inspiring English sources

A distinct property of the mass distribution of interstellar grains in the heliosphere is the deficit of small grains, mass < 10−15 gr (radius 0.04 0.2 μm for density 2.5 gr cm−3), and an excess of large grains, masses > 10−10 gr.

A low maximum 100 grain mass also ensured individual grain mass was little affected by environmental conditions.

Without (i), the grain mass just decreases; without (ii), the grain mass just increases; without (iii), there is no mechanism that produces the large abundance of small grains.

The blue points show the grain mass distribution that results in our model (focusing SWMF).

After harvest, the grains were dried to 13±1%1% of moisture at a grain mass temperature below 40 °C.

We assume that all grains are spherical with material density s; thus, the grain mass m is expressed as.

Right: Percentage of initial total grain mass lost because of dust destruction in the shock vs. shock speed.

For grains with a ≳ 0.1 μm, where most of the grain mass is contained in our cases, the grain velocity is governed by gyroresonance.

Thus, the grain mass m is related to the grain radius by (1 where ρgr is the material density of the grain.

In principle, if the propagation of interstellar dust grains through the heliosphere is known, the grain mass distribution (for the larger grains) in the ISM can be recovered.

If M is larger than half of the grain mass, we assume that the whole grain is fragmented; i.e., Mej = m1.