Примери за използване на Radiative на Английски и техните преводи на Български
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The radiative zone.
The first thing is this is not a"radiative" technology.
The radiative zone is just beyond the core of the Sun.
The solar radiative zone.
The radiative heat transfer is governed by Stephen- Boltzman law.
The assumption of a radiative balance is unphysical.
The density of the solar plasma is much less than in the radiative zone.
Astrometric sensors measure the radiative flux of up to three billion stars simultaneously.
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Applied primarily for low-thrust engines, radiative cooling uses walls that sustain high temperatures.
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Modo is an integrated GUI front-end to the MODTRAN5 radiative transfer code, running on the IDL virtual machine.
Hopf's work is also of the greatest importance to the hydrodynamics,theory of turbulence and radiative transfer theory.
This technique of calculating radiative absorption is widely used among researchers in space and nuclear science projects.
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After bouncing around in the radiative zone, our photon has lost much of its energy, and has shifted into the visible spectrum.
Calculations indicate that very small stars, below about 16% of a solar mass,are so cool that they have no radiative core at all.
He also published a book Mathematical problems of radiative equilibrium in 1934 which was reprinted in 1964.
He published his famous paper on classical electron theory,which included mass renormalisation and radiative reaction in 1938.
Uneven radiative forcing by explosions of ammunition or accidents at nuclear power plants is a major cause of development of local radiation damage.
They say the the Eddington Limit,which is a balance between a star's outward radiative force and the inward gravitational force, plays a role.
By contrast, the Sun's surface temperature is approximately 5,800 K. Recent analysis of SOHO mission data favors a faster rotation rate in the core than in the radiative zone above.
Next, he concentrated on the theory of radiative transfer and the quantum theory of the negative ion of hydrogen from 1943 to 1950.
In 1906 he studied the transport of energy through a star by radiation andpublished an important paper on radiative equilibrium of the atmosphere of the sun.
Next he looked at the theory of radiative transfer and the quantum theory of the negative ion of hydrogen from 1943 to 1950, followed by hydrodynamic and hydromagnetic stability from 1950 to 1961.
Energy at the core isthen carried out by radiation and that bounces around for about 170,000 years in the radiative zone until it gets to the top of the convective zone.
While at Manchester he continued his research into radiative equilibrium and the structure of stellar atmospheres, and his work on these topics led to his election to a Fellowship of the Royal Society.
In practice, however, all exchanges of energy are subject to inefficiencies,such as friction and radiative heat loss, which increase the entropy of the system being observed.
A study in 2011 calculated that the heat-trapping potential of contrail cirrus is actually greater than that of carbon emissions produced by airplanes,due to the way contrail clouds warm the planet through a process called radiative forcing.
Energy from the core is carried outward by radiation,which bounces around the radiative zone, taking about 170,000 years to get from the core to the top of the convective zone.