Architecture‐Driven Sensor Stability in Weft‐Knitted Engineering Textiles
Textile‐integrated sensor architectures are systematically compared to evaluate their electromechanical behavior under combined mechanical and environmental loading. Pocket‐based integration exhibits stable and reproducible signals, whereas tunnel‐based routing shows higher sensitivity accompanied by increased variability.
Adnan Maroof Khan +5 more
wiley +1 more source
Case Report: Indocyanine green fluorescence imaging in complex focal nodular hyperplasia resection: report of two cases. [PDF]
Du F +8 more
europepmc +1 more source
Adaptive Foam 3D Printing of Ultralight and Multifunctional Materials
Adaptive foam 3D printing, enabled by expandable microspheres, imparts cellular structures to thermoplastic and thermosetting polymers, manufactured through a variety of processes including fused filament fabrication, direct ink writing, digital light processing, and inkjet printing.
Nariman Rajabifar, Amir Ameli
wiley +1 more source
Core-envelope miscibility in sub-Neptunes and super-Earths. [PDF]
Gilmore T, Stixrude L.
europepmc +1 more source
Exploring central star variability of planetary nebulae using gaia photometry. [PDF]
NegmEldin MA, Ali A, Hamed GM, Essam A.
europepmc +1 more source
Simulations of multi-phase gas in and around galaxies. [PDF]
Gronke M, E Schneider E.
europepmc +1 more source
Magnetic activity and spectral behavior of RS CVn binary system (IM Pegasi) in the ultraviolet. [PDF]
Sanad MR, Rahman HIA, Badawy WA.
europepmc +1 more source
Magnetic activities of two contact binaries in quadruple stellar systems. [PDF]
Yang Y, Wang S.
europepmc +1 more source
Physicochemical Controls on the Compositions of the Earth and Planets. [PDF]
Sossi PA +4 more
europepmc +1 more source
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Effects of pulsation and mass loss on stellar evolution
Nature, 1984There is much evidence that many post-main sequence stars are losing mass, that the integrated mass loss is sufficient to affect their evolution and that epochs of substantial mass loss are normal for almost all stars. However, neither the precise timing, nor the mechanisms, nor the full consequences of this mass loss are yet well understood.
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