Sentences with phrase «high radiation flux»
He especially enjoys research focused on the study of matter at extreme conditions of high pressure, high temperature, and high radiation flux.
https://www.unlv.edu/ Not exact matches
In a very massive star, photon radiation — the outward flux of photons that is generated due to the star's very high interior temperatures — pushes gas from the star outward in opposition to the gravitational force that pulls the gas back in.
The correlation we observed is compatible with the hypothesis that the highest - energy particles originate from nearby extragalactic sources whose flux has not been substantially reduced by interaction with the cosmic background radiation.
As the atmospheric opacity is increased (e.g., 2xCO2), the physical location of the TAU = 1 level will rise to a higher altitude, but the outgoing flux will still come from the TAU = 1 level since radiation doesn't care about the geometric scale), and the TAU = 1 level will still correspond to the same temperature (since the solar input energy is unchanged).
(& we have assumed that the energy - in flux is constant) If the new GHG temperature is the same or higher than the air temp, then there will be NO energy absorption by radiation by the new GHGs or any other air or GHG molecules.
The increase / decrease of net upward LW flux going from one level to a higher level equals the net cooling / heating of that layer by LW radiation — in equilibrium this must be balanaced by solar heating / cooling + convective / conductive heating / cooling, and those are related to flux variation in height in the same way.
If it is in an isothermal layer, it will radiate upward as much as downward; it will decrease the baseline TRPP net flux and increase the baseline TOA flux by the same amount, but it will decrease the baseline TOA flux by a greater amount if it is absorbing radiation with a higher brightness temperature from below (the baseline upward flux at TRPP), so it will increase the amount by which the baseline net flux at TRPP is greater than that at TOA.
Recent accurate laboratory measurements of the absorption in the CO2 band by CLOUD (1952) were used to calculate the radiation flux in the atmosphere with the aid of the MIDAC high speed digital computor.»
The other fluxes (shortwave and longwave radiation at both surface and top of atmosphere) show more «normal» cycles (though somewhat higher values).
Ice significantly reduces the heat flux between ocean and atmosphere; through its high albedo it has a strong influence on the radiation budget of the entire Arctic.
The atmosphere is analogous to a flexible lens that is shaped by the density distribution of the gas molecules, of the atmosphere in the space between the sphere holding them, and space; Incoming heat gets collected in many ways and places,, primarily by intermittent solar radiation gets stored, in vast quantities, and slowly but also a barrage of mass and energy fluxes from all directions; that are slowly transported great distances and to higher altitudes mostly by oceanic and atmospheric mass flows.
ETH Zurich has expertise in developing and refining technologies geared towards the production of solar fuels and has unique experimental research facilities for controlled experimentation under high - flux solar radiation.
It might help you if you had a few concepds in mind too when considering this subject, like «space» is the big energy «sink» with old sol (and the internal heat generating processes (including nuclear) of the earth) as sources... any mechanism that results in a delay of energy leaving earth, such as a «bounce - back» or a re-rad of energy (like back radiation) certainly is going to increase the «energy flux» in the system, and this in any way you want to frame the argument translates to a «higher» energy state, and a higher so - called temperature» (movement in matter, velocity of air molecules or oscillations in certain «resonant molecules) as well.
Likewise, the emission of CO2 within its absorption bands is just as effective as its interception, therefore this energy is partitioned throughout the atmosphere and radiated back to earth in its majority (because the escape of energy through the optically thick higher levels of the atmosphere reduces the flux, whereas the earth is still optically close by and a ready recipient of IR radiation.