Results 171 to 180 of about 9,691 (218)
Mapping Nanoscale Buckling in Atomically Thin Cr2Ge2Te6
Atomic‐resolution STEM is used to resolve nanoscale buckling in monolayer Cr2Ge2Te₆. A noise‐robust image analysis reconstructs three‐dimensional lattice distortions from single plan‐view images, revealing pronounced defect‐driven nm‐scale out‐of‐plane buckling.
Amy Carl +20 more
wiley +1 more source
Functionally rich crop rotations increase calorie and macronutrient outputs across Europe. [PDF]
Vico G +23 more
europepmc +1 more source
The effect of concomitant gradient fields on MRI with long readout radial-based trajectories. [PDF]
Malmberg MA +3 more
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Perspectives on the physics of late-type stars from beyond low earth orbit, the moon and mars. [PDF]
Mathur S, Santos ÂRG.
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Whoosh! visual depictions of direction, speed, and temporality: a corpus analysis of motion events in global comics. [PDF]
Hacımusaoğlu I, Cardoso B, Cohn N.
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Iron Oxide-Based Magnetic Nanoparticles in Oral Infection Control. [PDF]
Yang C +6 more
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Evaluation study of radial and spiral based volumetric thermometry for monitoring of hepatic microwave ablation. [PDF]
Horstmann D +9 more
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Magnetoconvection in Rotating Stars
Astrophysics and Space Science, 2003zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Tagare, S. G., Rameshwar, Y.
openaire +2 more sources
AIP Conference Proceedings, 2007
The treatment of rotating stars brings together several stellar astrophysical disciplines. Models of rotating stars must be able to simulate the stellar structure and evolution, stellar atmospheres models are required to determine the spectral energy distribution and spectral line shapes of rotating stars, and radial and nonradial stellar pulsation is ...
R. G. Deupree +7 more
openaire +1 more source
The treatment of rotating stars brings together several stellar astrophysical disciplines. Models of rotating stars must be able to simulate the stellar structure and evolution, stellar atmospheres models are required to determine the spectral energy distribution and spectral line shapes of rotating stars, and radial and nonradial stellar pulsation is ...
R. G. Deupree +7 more
openaire +1 more source

