Shadow effects on a series-parallel array of solar cells
Shadow effects on series-parallel array of solar cells
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Shadow effects on series-parallel array of solar cells
Analysis of thermal test errors resulting from imperfectly collimated solar simulation beams - relative energy flux density and relative energy in penumbrae of various shadowing objects
Statistical model of lunar surface roughness, shadow, and thermal emission
Apollo thermal control systems and concepts, discussing self-shadowing
Model for lunar surface roughness effect on emission of thermal IR radiation and casting of shadows in sunlight
Hybrid superconductor–semiconductor platforms are foundational to advancing quantum information technologies, motivating the integration of materials with clean interfaces, robust superconductivity, and scalable architectures. Here, in this work, we report the synthesis and analysis of inclined InAs nanowires, conformally coated with β-Sn shells. These nanowires extend in opposite in-plane directions, forming a self-aligned, criss-cross network. This enables the deterministic formation of nanowire-shadow Josephson junctions through angle-controlled, low-temperature Sn deposition. Structural characterization shows uniform polycrystalline β-Sn shells forming a sharp, diffusion-free interface with InAs. Low-temperature transport measurements reveal a hard induced superconducting gap ≈ 600 μeV, switching currents up to ≈ 500 nA, and parallel magnetic field resilience beyond 1T. These results establish β-Sn/InAs nanowire networks as a promising platform for superconducting qubits, low-noise microwave devices, and the exploration of exotic superconducting phases including triplet pairing and topological superconductivity.
We determine the nuclear suppression factor S Pb ( x ) , where x = M J / ψ 2 / W γ p 2 with M J / ψ the J / ψ mass and W γ p the photon-nucleon energy, for the cross section of coherent J / ψ photoproduction in heavy-ion ultraperipheral collisions at the Large Hadron Collider and Relativistic Heavy Ion Collider by performing the χ 2 fit to all available data on the cross section d σ A A → J / ψ A A / d y as a function of the J / ψ rapidity y and the photoproduction cross section σ γ A → J / ψ A ( W γ p ) as a function of W γ p . We find that while the d σ A A → J / ψ A A / d y data alone constrain S Pb ( x ) for x ≥ 10 − 3 , the combined d σ A A → J / ψ A A / d y and σ γ A → J / ψ A ( W γ p ) data allow us to determine S Pb ( x ) in the wide interval 10 − 5 < x < 0.05 . In particular, the data favor S Pb ( x ) , which decreases with a decrease of x in the 10 − 4 < x < 0.01 interval and can be both decreasing or constant for x < 10 − 4 . Identifying S Pb ( x ) with the ratio of the gluon distributions in Pb and the proton R g ( x , Q 0 2 ) = g A ( x , Q 0 2 ) / [ A g p ( x , Q 0 2 ) ] , we demonstrate that the leading twist approximation for nuclear shadowing provides a good description of all the data on d σ A A → J / ψ A A / d y and σ γ A → J / ψ A ( W γ p ) as well as on the experimental values for S Pb ( x ) derived from σ γ A → J / ψ A ( W γ p ) . We also show that modern nuclear parton distributions reasonably reproduce S Pb ( x ) as well. Published by the American Physical Society 2024
Light density and color in earth shadow during lunar eclipse
Relative energy flux densities in the penumbrae of various shadowing objects - data tables
Lightweight inflatable shadow shields for cryogenic space vehicles and performance in conjunction with superinsulation
Shadowing effect and anomalous backscattered intensity in diffuse reflection from plane- parallel layer of random particles
Statistical model of lunar surface roughness for shadow and infrared emission characteristics
Geometrical self-shadowing of random rough surface described by Gaussian statistics in wave backscattering phenomena
Empirical method of correcting azimuthal orientation of Explorer 35 in lunar shadow
Method of correcting azimuthal orientation of Explorer 35 spacecraft while in lunar shadow
Heat transfer from balloon type shadow shield to cryogen storage tank - mathematical discussion
Plasma shadow formation on dark side of moon, using solar wind-moon interaction model