Results 81 to 90 of about 48,168 (266)
Formation and collimation of relativistic MHD jets - simulations and radio maps
We present results of magnetohydrodynamic (MHD) simulations of jet formation and propagation, discussing a variety of astrophysical setups. In the first approach we consider simulations of relativistic MHD jet formation, considering jets launched from ...
Fendt, Christian +2 more
core +1 more source
SMAP Satellite Microwave Radiometry to Monitor River Flow and Lake Level in the Lower Mekong Basin
Abstract The NASA Soil Moisture Active Passive Mission (SMAP) satellite passive microwave radiometry (PMR) capability is demonstrated for measurements of river stage, river discharge, and lake level with in situ gauging data in the Lower Mekong Basin (LMB).
A. Podkowa +3 more
wiley +1 more source
Abstract Oxychlorines (i.e., perchlorates (ClO4−) and chlorates (ClO3−)) have been detected by several landed missions on Mars at various locations. These missions have provided crucial information about the geographic distribution and abundances of oxychlorines on Mars but have not definitively identified the cation and anion type of in situ, solid ...
J. V. Clark +15 more
wiley +1 more source
Shear Acceleration in Relativistic Astrophysical Jets
18 pages, ApJ in press; final version (small typos corrected to match published version), Journal-ref ...
Rieger, Frank M., Duffy, Peter
openaire +2 more sources
Abstract The fifth generation of ECMWF atmospheric reanalyses data (ERA5), operational observed data, S‐band radar data and Large Eddy Simulation (LES) tool were employed to investigate the evolution of local small‐scale convection in Ziyang City of Sichuan Province on 11 April 2022 in spring.
Xiaolong Cheng, Hui Luo, Yueqing Li
wiley +1 more source
This is the first in a series of papers that introduces a new paradigm for understanding the jet in M87: a collimated relativistic flow in which strong magnetic fields play a dominant dynamical role.
Asada +32 more
core +1 more source
Dust-driven Dynamos in Accretion Disks [PDF]
Magnetically driven astrophysical jets are related to accretion and involve toroidal magnetic field pressure inflating poloidal magnetic field flux surfaces.
Chrysostomou A. +10 more
core +4 more sources
Abstract The Gravity Recovery and Climate Experiment (GRACE) and its successor, GRACE‐Follow On, play an important role in monitoring mass transport across the Earth. Compared to spherical harmonic solutions, mass concentration (mascon) solutions offer less signal leakage and a “higher” spatial resolution. How the shapes, sizes, and positions of mascon
Dong Fang +4 more
wiley +1 more source
Let There Be Neutrons! Hadronic Photoproduction from a Large Flux of High-energy Photons
We propose that neutrons may be generated in high-energy, high-flux photon environments via photo-induced reactions on pre-existing baryons. These photohadronic interactions are expected to occur in astrophysical jets and surrounding material ...
Matthew R. Mumpower +6 more
doaj +1 more source
The thick accretion disk and donor’s wind on the example of CYG X-1 are computed. The main aim of the present simulations is to calculate the precessing thick accretion disk and ON- and OFF-state generation by the methods of 3D numerical hydrodynamics ...
V. V. Nazarenko, S. V. Nazarenko
doaj +1 more source

