Results 141 to 150 of about 48,168 (266)
A class of exact MHD models for astrophysical jets [PDF]
N. Vlahakis, K. Tsinganos
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Abstract We investigated the regolith parent rock (“protolith”) properties of Mare Tranquillitatis and Marius Hills on the Moon, utilizing lunar pit craters (“lua”) to contextualize observations of rock abundance and crater degradation. We discovered a significant difference in underlying materials: the region around the Tranquillitatis lua is ...
E. S. Costello +5 more
wiley +1 more source
On gravitational chirality as the genesis of astrophysical jets [PDF]
R W Tucker, T J Walton
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Variations in Satellite Charge Drag Coefficient With Solar Cycle
Abstract Ionospheric plasma interaction with charged satellite surfaces can lead to a substantial increase in orbital drag. In this context, natural events related to solar activity can have a detrimental effect on a satellite's lifespan and introduce uncertainty in orbital trajectory predictions.
A. Fazel‐Najafabadi +2 more
wiley +1 more source
Diffuse astrophysical neutrinos from dark matter around blazars
Neutrinos from blazars can originate from inelastic scatterings between protons within their jets and sub-GeV dark matter (DM) around them, explaining IceCube detections of neutrinos from TXS 0506+056 that are otherwise challenging for models of its jet.
Andrea Giovanni De Marchi +3 more
doaj +1 more source
Numerical Simulations of Magnetized Astrophysical Jets and Comparison with Laboratory Laser Experiments [PDF]
V. S. Belyaev +7 more
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Abstract Understanding and forecasting extreme radiation belt electron fluxes has been a major goal in space weather since their discovery in 1958. In this study, by combining electron flux data from multiple satellite missions in different orbits, including Van Allen Probes, Electron Losses and Fields Investigation, and Colorado Inner Radiation Belt ...
Man Hua +6 more
wiley +1 more source
Observed jet power and radiative efficiency of black hole candidates in the Kerr+PFDM model
In this research, we explore the electromagnetic energy emitted by astrophysical black holes within the Kerr+PFDM (Kerr + perfect fluid dark matter) spacetime, a model comprising rotating black holes surrounded by dark matter.
Bakhtiyor Narzilloev +3 more
doaj +1 more source
Dynamics of the twisted magnetic flux-tube in the astrophysical jets [PDF]
Ebru Devlen
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Large-Scale Hydrodynamic Simulations of Astrophysical Jets [PDF]
J. H. Beall +6 more
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