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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.
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It was found that in this particular HEx, the heat transfer resistance is mainly influenced by both of the fin pitch and height, while the inter-grain mass transfer resistance is independently controlled by the bed length.
A mathematical distributed model along with the linear driving force (LDF) model and Darcy's law have been considered to take into account the effects of heat and both intra/inter-grain mass transfer resistances.
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.
Li et al. (2000) proposed a compaction correction method based on the principle that the grain volume and mass of formation should remain constant, which has resulted in deep debate among Chinese investigators (e.g., Qi and Yang 2001; Li 2001).
However, Bednarek et al.[ 22] showed that RNAi resulted in down-regulation of TaGW2 expression in wheat, inducing significant decreases in grain parameters (viz. final grain fresh, dry and irrigation masses, and grain volume, width, and thickness).
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