Available aerocapture "corridor width" (allowable range of atmospheric entry angle) also depends on height rate of change of atmospheric density, as characterized by density scale height.
The extractions of the atmospheric mixing angle θ23 rely on the standard model cross sections for ντ+N→τ−+X in ντ appearance experiments.
Because the neutral atmospheric bending angle decreases exponentially with height, the retrieved profiles above about 40 km may contain measurement errors due to ionospheric noise.
Radiometric consistency among collocated multi-temporal imagery is difficult to maintain, however, due to variations in sensor characteristics, atmospheric conditions, solar angle, and sensor view angle that can obscure surface change detection.
Because our major purpose is to examine the effect of magnetic inclination at two locations with different dip angles, background atmospheric parameters and solar zenith angles for both calculations were chosen to be the same as those at Yamagawa when coseismic disturbances were observed after the M9.0 Tohoku-Oki earthquake in 2011, and only (I) was changed with the locations.
Other works that stand out include Mr. Aitchison's simplified, mystical landscape of Holy Island off western Scotland, revisited in memory; Ms. Rego's grotesquely distorted portraits of oddly clothed women who seem to be victims of mysterious circumstances; and Mr. Wonnacott's ingeniously angled, atmospheric portraits of himself and his family.
This was followed by radiometric correction of all the images for variation in sun angle and atmospheric effects.
where P is the local pressure, T the time, and e0 the Sun's topocentric elevation angle without atmospheric refraction correction.
Perez et al. [10] developed a luminous efficacy model for all sky types as a function of the solar zenith angle (Z), atmospheric precipitable water content (W), and the sky brightness index.
This is supported by comparing bubble shapes generated in actual boiling experiments and dynamic contact angles under atmospheric conditions on Teflon-coated nano/microstructured surfaces.
In both days, the position of the GasFinder laser unit was sequentially moved (e.g., from positions A to E in Figs. 2 and 3) to scan the fumaroles' atmospheric plumes from different angles and viewing directions.
