The test samples were made up at a binder to stone dust ratio of 1 8 by weight.
Results indicated that all specimens have compressive strength greater than 7 MPa, while cement-to-limestone dust ratio was recognized as the most important factor with the regard to compressive strength.
The drag torque shows good agreement with the water vapor density measured by other instruments during the E5 encounter, but indicates a rather higher mass density on other passes (E3, E14), possibly indicating variations in gas composition and/or gas:dust ratio.
Median vent:floor dust ratios were greater than 1 for the major congeners in the PentaBDE commercial product (BDE 47 – 2.1; BDE 99 – 1.2; BDE 100 – 2.1; BDE 153 – 2.1; BDE 154 – 2.0), but unity for BDE 209 and 0.6 for BDE 183 (The inconsistent results for BDE 99 may be due to coelution issues with TBB).
Based on their observations, Fritz et al. (2011) argued that the extinction at the visual band (AV) toward the GC may be as high as AV ~ 59 mag (with the exact AV depending on the chosen gas-to-dust ratio NH/AV), much larger than AV ~ 31 estimated by Rieke et al. (1989) which is commonly adopted in the astronomical literature.
superthermality of ions (via (kappa _i)), electron-to-dust density ratio (via (mu _e)), dust kinematic viscosity of medium (via (eta _0)), strength of magnetic field (via (Omega _d)) and obliqueness of magnetic field (via (l_z))) on the characteristics of DA shock structures has been highlighted in the present study.
In multivariate analyses, eye irritation was positively correlated with floor dust [odds ratio (OR) = 1.46; 95% confidence intervals (CI), 1.14-1.86] and reported lack of office cleanliness (OR = 1.52; 95% CI, 1.11-2.08).
A unique local diagnostic of the gas-to-dust mass ratio, Rg/d, is provided by comparisons between in situ dust data and the local ISM properties inferred from observations of interstellar gas inside and outside of the heliosphere.
The gas-to-dust mass ratio, Rg/d, can be independently determined from the in situ dust measurements, and then compared with the predictions of the LIC photoionization models.
A third characteristic of the depletion pattern appears when depletions in tenuous and translucent clouds are combined to display the gas-to-dust mass ratio, Rg/d, as a function of the percentage of the dust mass carried by Fe (Fig. 3, left, and Frisch and Slavin (2003)).
superthermality of ions, magnetic field, electron-to-dust-density ratio, kinematic viscosity, ion-to-electron-temperature ratio and obliqueness.
