Weak lensing by large scale structure or 'cosmic shear' is a potentially powerful cosmological probe to shed new light on Dark Matter, Dark Energy and Modified Gravity.
This suggest that, in these locations, the probe beam was only weakly scattered close to the focus but still deflected by larger scale structures.
The cosmological interpretation of weak lensing by large-scale structures requires knowledge of the redshift distribution of the source galaxies.
It is based on the weak distortions induced by large-scale structures on the observed shapes of distant galaxies through gravitational lensing.
Attempts to understand the variability in SEP intensities have been focused on two aspects: (1) source factors involving CME properties, (2) environmental factors such as ambient magnetosonic speed, preceding CMEs, deflection by large-scale structures, seed particles, and turbulence.
Another example is, for instance, horizontal mixing processes through the transport barriers, either by small-scale structures (filaments or laminae) or by large-scale structures (streamers), are thought to play a significant role in the variability of atmospheric trace gases in the middle stratosphere (Krüger et al. 2005).
We present here hydrodynamic simulations of structure formation implementing the effect of the cooling by dust on large scale structure formation.
The acquired images, which correspond to the 3D structure of the parenchyma, are then transformed into physical, albeit larger scale, structures by 3D printing, and their mechanical properties are characterized.
Amplification of the larger scale structures is accommodated by the accumulation of displacements on smaller scale structures.
