Results 81 to 90 of about 152,163 (238)
Radiative Processes in Cool Star Chromospheres
Observations made with the International Ultraviolet Explorer (IUE) satellite between 1200 A and 3000 A have shown that the spectra of giant and supergiant stars later than about K O are dominated by emission from neutral atoms and singly charged ions.
Jordan, C, Judge, P
openaire +1 more source
Chandra X-Ray Spectral Analysis of Cooling Flow Clusters, 2A 0335+096 and Abell 2199
We report on a spatially resolved analysis of Chandra X-ray data on a nearby typical cooling flow cluster of galaxies 2A 0335+096, together with A 2199 for a comparison. As recently found in the cores of other clusters, the temperature around the central
Fukazawa, Yasushi +2 more
core +1 more source
Stimulated radiative laser cooling
Building a refrigerator based on the conversion of heat into optical energy is an ongoing engineering challenge. Under well-defined conditions, spontaneous anti-Stokes fluorescence of a dopant material in a host matrix is capable of lowering the host temperature.
openaire +2 more sources
Three dimensional (3D) adaptive-mesh refinement (AMR) hydrodynamical simulations of the wind-wind collision between the enigmatic super-massive star \etacar and its mysterious companion star are presented which include radiative driving of the stellar ...
Abdo +58 more
core +1 more source
AntiāEnvironmental Aging Passive Daytime Radiative Cooling
Passive daytime radiative cooling technology presents a sustainable solution for combating global warming and accompanying extreme weather, with great potential for diverse applications.
Jianing Song +3 more
doaj +1 more source
Magnetic Reconnection with Radiative Cooling. I. Optically-Thin Regime
Magnetic reconnection, a fundamental plasma process associated with a rapid dissipation of magnetic energy, is believed to power many disruptive phenomena in laboratory plasma devices, the Earth magnetosphere, and the solar corona.
Braginskii S. I. +6 more
core +1 more source
Winds driven by super-star clusters: The self-consistent radiative solution
Here we present a self-consistent stationary solution for spherically symmetric winds driven by massive star clusters under the impact of radiative cooling. We demonstrate that cooling may modify drastically the distribution of temperature if the rate of
Rodriguez-Gonzalez, Ary +2 more
core +1 more source
Radiative sky cooling: fundamental physics, materials, structures, and applications
Radiative sky cooling reduces the temperature of a system by promoting heat exchange with the sky; its key advantage is that no input energy is required.
Sun Xingshu +4 more
doaj +1 more source
Radiative cooling: arising from practice and in turn serving practice
Radiative cooling, as a renewable cooling technology, is expected to mitigate growing global warming. However, the barrier when promoting radiative cooling from the laboratory to practice is still a blind spot and needs to be discussed right now.
Zhang Quan, Rao Zhonghao, Ma Rujun
doaj +1 more source

