Results 21 to 30 of about 152,163 (238)
The role of radiative losses in the late evolution of pulse-heated coronal loops/strands [PDF]
Radiative losses from optically thin plasma are an important ingredient for modeling plasma confined in the solar corona. Spectral models are continuously updated to include the emission from more spectral lines, with significant effects on radiative ...
Antiochos +60 more
core +2 more sources
Thermoregulating textiles and fibrous materials for passive radiative cooling functionality
Developing thermoregulating textiles based on passive radiative cooling strategies has recently attracted considerable attention as an emerging means of providing localised thermoregulation for wearers.
Esfandiar Pakdel, Xungai Wang
doaj +1 more source
The effect of radiative cooling on scaling laws of X-ray groups and clusters [PDF]
We have performed cosmological simulations in a ΛCDM cosmology with and without radiative cooling in order to study the effect of cooling on the cluster scaling laws.
Couchman, H M P +4 more
core +3 more sources
We present baroclinic life‐cycle simulations with two versions of the atmosphere model ICON to understand how cloud‐radiative heating and cooling affect an idealized midlatitude cyclone. Both versions simulate the same cyclone when run without radiation,
Aiko Voigt, Behrooz Keshtgar, Klara Butz
doaj +1 more source
Perspectives on the Applications of Radiative Cooling in Buildings and Electric Cars
Cooling energy consumption is a major contributor to various sectors in hot climates with a significant number of warm days throughout the year. Buildings account for 40% of total energy consumption, with approximately ∼30–40% of that used for cooling in
N. S. Susan Mousavi, Brian Azzopardi
doaj +1 more source
Current Status and Future Perspectives of Radiative Sky Cooling
Radiative sky cooling cools an object on the Earth’s surface by emitting thermal radiation through the atmospheric window to the cold universe. As a passive technique to reduce cooling energy requirements without power input, radiative cooling provides a
Guo Chenyue +5 more
doaj
Evolution of Primordial Protostellar Clouds --- Quasi-Static Analysis --- [PDF]
The contraction processes of metal-free molecular clouds of starlike mass (or cloud cores) are investigated. We calculate radiative transfer of the H_2 lines and examine quasi-static contraction with radiative cooling. Comparing two time-scales, the free-
Nishi, Ryoichi +3 more
core +2 more sources
Cooling flows in clusters of galaxies [PDF]
The gas temperature in the cores of many clusters of galaxies drops inward by about a factor of three or more within the central 100kpc radius. The radiative cooling time drops over the same region from 5 or more Gyr down to about 10^8 yr.
Fabian, A. C.
core +3 more sources
Concentrated Radiative Cooling
A fundamental limit of current radiative cooling systems is that only the top surface facing deep-space can provide the radiative cooling effect, while the bottom surface cannot. Here, we propose and experimentally demonstrate a concept of "concentrated radiative cooling" by nesting a radiative cooling system in a mid-infrared reflective trough, so ...
Peoples, Joseph +8 more
openaire +2 more sources
Global Radiative Sky Cooling Potential Adjusted for Population Density and Cooling Demand
Thanks to recent advances in nanophotonics and scalable manufacturing of metamaterials, radiative sky cooling has emerged as a “self-reliant” cooling technology with various potential applications.
Ablimit Aili, Xiaobo Yin, Ronggui Yang
doaj +1 more source

