New group paper – traces of an ancient asteroid impact in NW Scotland Posted onOctober 30, 2024byRomain Tartese This gallery contains2 photos. Along the coast of NW Scotland, a few metres of sedimentary rocks were deposited during an impact event 1.2 billion years ago, forming the Stac Fada...
The Earth’s magnetosphere is the outermost layer of the geospace system deflecting energetic charged particles from the Sun and solar wind. The solar wind has major impacts on the Earth’s magnetosphere, but it is unclear whether the same holds for sola
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Edsjo¨, "Weakly interacting massive particle diffusion in the solar system including solar depletion and its effect on earth capture rates," Physical ... J Lundberg,J Edsj? - 《Physical Review D》 被引量: 84发表: 2004年 WIMP diffusion in the solar system including solar WIMP-nucleon scatte...
The fraction of incoming shortwave solar radiation that is reflected by a surface, ranging between 0 and 1. Internal variability The variability in the climate system attributable to the chaotic nature of the climate system. Negative feedbacks Dampening feedbacks in the climate system, reducing an in...
be suitable because of the dust particles in our solar system. A telescope would have to be as far away as the planet Jupiter to look for life in outer space, because the dust becomes thinner the further we travel towards the outer edges ...
Abstract:Aerosol particles are an important part of the Earth system, but their concentrations are spatially and temporally heterogeneous, as well as variable in size and composition. Aerosol particles can interact with incoming so...
In the park, a new electric system caught my attention. Through an intelligent IoT system and an energy island combining wind power, solar power, energy storage, and green hydrogen, 80 percent of the power will be supplied directly with green energy, with the remaining 20 percent traded with...
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Trojan asteroids are small bodies orbiting around the L4 or L5 Lagrangian points of a Sun-planet system. Due to their peculiar orbits, they provide key constraints to the Solar System evolution models. Despite numerous dedicated observational efforts in