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Given that dispersal through bridging is very uncommon among very large individuals (GC and JML, personal observations), constraints on bridging could help to explain the evolution of SSD in spiders.
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Since agile satellite task planning has no baseline, so we did the simulation experiments with scenario simulation and data under agile satellite observation constraints generated randomly.
High-resolution images are reconstructed by alternating the projections onto two constraint sets: the observation constraint defined by the given low-resolution image and the prior constraint derived from the training data at the high resolution (HR).
These observations provide constraints on the coronal heating mechanism(s) and highlight the importance of the interface region between photosphere and corona.
Three-dimensional seismic mapping of interpretative sub-surface time slice sections, incorporating age data and detailed structural observations places constraints on the structural architecture and stratigraphic evolution of the Icotea pull-apart basin in the central Maracaibo basin, Venezuela.
FAPAR is difficult to measure directly, but is inferred from models describing the transfer of solar radiation in plant canopies, using remote sensing observations as constraints [25, 38, 39].
Solar Orbiter's location, combined with the fact that the spacecraft will nearly co-rotate with the sun on some portions of its orbit, will furnish observations placing constraints on solar wind models.
A range of different observations equations, constraints and unknowns (i.e. parameters) are allowed in the adjustment routine, among them: tie points, lines, perspective centers derived from direct georeferencing (i.e. GNSS), ground control points (GCP), the lever-arm vector separating the GNSS antenna and the perspective center, rigid relative orientation between cameras.
FAPAR is difficult to measure directly, but is inferred from models describing the transfer of solar radiation in plant canopies, using remote sensing observations as constraints [ 25, 38, 39].
In this first analysis, we have retained a large range of values for the entrainment coefficients (indeed, a larger range than found in existing experimental studies) to avoid discounting plausible values from the study, and have taken ranges for k s and k w and no further probability judgements to let the observations induce constraints.
The mineralogical features determined by our TEM observation put constraints on the peak temperatures for the severely heated MMs.
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