MPI-AMRVAC 3.0: Updates to an open-source simulation framework

R. Keppens1, B. Popescu Braileanu1, Y. Zhou1, W. Ruan1, C. Xia2, Y. Guo3, N. Claes1 and F. Bacchini1,4 + Received: 2 November 2022 Accepted: 12 March 2023 Abstract Context. Computational astrophysics nowadays...
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MPI-AMRVAC 3.0: Updates to an open-source simulation framework

A physical model for the magnetosphere of Uranus at solstice time (Pantellini)

by Filippo Pantellini 2020. The magnetosphere of Uranus is subject to strong seasonal variations. The variability is a consequence of...
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A physical model for the magnetosphere of Uranus at solstice time (Pantellini)

Optical levitation-associated atomic loading in a dipole trap

We demonstrate a robust method for the efficient optically levitated loading of ultracold Cs atoms in a crossed dipole trap....
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Optical levitation-associated atomic loading in a dipole trap

Roadmap on all-optical processing

The ability to process optical signals without passing into the electrical domain has always attracted the attention of the research...
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Roadmap on all-optical processing

Mean Estimate Distances for Galaxies with Multiple Estimates in NED-D

Numerous research topics rely on an improved cosmic distance scale (e.g., cosmology, gravitational waves) and the NASA/IPAC Extragalactic Database of...
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Mean Estimate Distances for Galaxies with Multiple Estimates in NED-D

Self-consistent Color–Stellar Mass-to-light Ratio Relations for Low Surface Brightness Galaxies

The color–stellar mass-to-light ratio relation (CMLR) is a widely accepted tool for estimating the stellar mass (M *) of a...
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Self-consistent Color–Stellar Mass-to-light Ratio Relations for Low Surface Brightness Galaxies

Linking gravitational waves and X-ray phenomena with joint LISA and Athena observations

The evolution of cosmic structures, the formation and growth of the first black holes and the connection to their baryonic...
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Linking gravitational waves and X-ray phenomena with joint LISA and Athena observations

Upper limits for PH3 in the atmosphere of Mars

Phosphine (PH3) is proposed to be a possible biomarker in planetary atmospheres and has been claimed to have been observed...
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Upper limits for PH3 in the atmosphere of Mars

Two distinctive regimes in the charge transport of a magnetic topological ultra thin film

The effect of the magnetic impurities on the charge transport in a magnetic topological ultra-thin film (MTF) is analytically investigated...
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Two distinctive regimes in the charge transport of a magnetic topological ultra thin film

Fundamental mode intensity evolution in tapered optical fibres

The mode field intensity, spot size, central peak intensity evolution and adiabaticity are calculated for different points along the transition...
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Fundamental mode intensity evolution in tapered optical fibres

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