Zobrazeno 1 - 10
of 25 803
pro vyhledávání: '"ADRIAN, J."'
Autor:
Bevan, Adrian J., Taifakou, Fani E., Amjad, Choudhry Z., Horner, Aled, Allwork, C., Drew, A. J.
Publikováno v:
NIMA Volume 1069, December 2024, 169882
In recent decades organic electronics has entered the mainstream of consumer electronics, driven by innovations in scalability and low power applications, and low-cost fabrication methods. The potential for using organic semiconductor electronic devi
Externí odkaz:
http://arxiv.org/abs/2412.04501
Autor:
Astoul, Aurélie, Barker, Adrian J.
Stars and gaseous planets are magnetised objects but the influence of magnetic fields on their tidal responses and dissipation rates has not been well explored. We present the first exploratory nonlinear magnetohydrodynamic (MHD) simulations of tidal
Externí odkaz:
http://arxiv.org/abs/2411.16534
We study local magnetohydrodynamical (MHD) instabilities of differential rotation in magnetised, stably-stratified regions of stars and planets using a Cartesian Boussinesq model. We consider arbitrary latitudes and general shears (with gravity direc
Externí odkaz:
http://arxiv.org/abs/2410.06989
Autor:
Li, Yuzhu, Pillar, Nir, Liu, Tairan, Ma, Guangdong, Qi, Yuxuan, de Haan, Kevin, Zhang, Yijie, Yang, Xilin, Correa, Adrian J., Xiao, Guangqian, Jen, Kuang-Yu, Iczkowski, Kenneth A., Wu, Yulun, Wallace, William Dean, Ozcan, Aydogan
Organ transplantation serves as the primary therapeutic strategy for end-stage organ failures. However, allograft rejection is a common complication of organ transplantation. Histological assessment is essential for the timely detection and diagnosis
Externí odkaz:
http://arxiv.org/abs/2409.05255
The goal of this paper is to review the properties of a Rule 60 cellular automaton on a ring with a Mersenne number circumference and to use this knowledge to explicitly construct all the ground state configurations of the classical Newman-Moore mode
Externí odkaz:
http://arxiv.org/abs/2407.19898
Recent work suggests that inwardly propagating internal gravity waves (IGWs) within a star can be fully converted to outward magnetic waves (MWs) if they encounter a sufficiently strong magnetic field. The resulting magnetic waves dissipate as they p
Externí odkaz:
http://arxiv.org/abs/2404.07085