I have difficulty rationalizing how 2 % of the molecules in the air (H2O and CO2) can heat themselves, the other 98 % of the air molecules, and the earth surface, by 33K only
through back radiation of IR.
For example, increased well - mixed CO2 and water vapor decrease the rate of heat loss
through back radiation.
Re # 36: «This incoming shortwave is balanced by * net * ocean heat loss
through back radiation (41 %)» The key word * net * should have been used.
This incoming shortwave heating is balanced by ocean heat loss
through back radiation (41 %), evaporative heat loss (53 %), and heat loss by conduction and convection (6 %).
Not exact matches
These low gamma
radiation levels are promising, but researchers still have to study other ways people on the islands could absorb
radiation — like
through their diet — before giving Marshall Islands inhabitants the green light to move
back.
Later that day we realized the migraine was in fact a tumor, and he fought
through rounds of
radiation and chemotherapy to battle
back for the last day of school, which was his goal.
They don't have to be scientists to understand that the higher energy waves of visible light from the Sun can penetrate
through CO2, H2O, CH4, NOZ etal in the atmosphere, but the lower energy
radiation of infra - red waves, from Earth's surface, have problems getting
back out
through these molecules, and a new energy balance has to be established in the form of rising temperature.
Visible and near - visible
radiation from the sun easily gets
through, but thermal
radiation from the surface can't easily get
back out.
I'm a professional infrared astronomer who spent his life trying to observe space
through the atmosphere's
back -
radiation that the environmental activists claim is caused by CO2 and guess what?
This is basically
back to classical meteorology before
radiation madness struck: sun heats surface, surface looses heat
through the atmosphere to space.
The use of dark, nonreflective materials for parking, roofs, walkways, and other surfaces raises ambient temperatures when
radiation from the sun is absorbed and transferred
through convection and conduction
back to surrounding areas.
to reflect near - IR
radiation back onto the filament while allowing visible light
through, resulting in additional heating of the filament and a concomitant reduction in electrical power (up to 30 %) required to maintain the same filament temperature.
The atmosphere acts like the glass in a greenhouse, allowing much of the shortwave solar
radiation to travel
through unimpeded, but trapping a lot of the longwave heat energy trying to escape
back to space.
If we assume that the
back radiation leads indeed to the decrease of the gradient
through the upper part of the ocean then we will have the decrease of the flow of heat from the bulk to the surface.
The total
radiation leaving one side of the layer is the external
radiation reflected
back by the interface,
radiation emitted internally by the layer and transmitted
through the interface,
radiation scattered by sites inside the layer and transmitted
through the interface, and
radiation transmitted
through the layer from the surroundings on the opposite side.
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.
One suggestion he came up with was that the energy coming in from the sun in the form of visible and ultra-violet light (known
back then as «luminous heat») was easily able to pass
through Earth's atmosphere and heat up the planet's surface, but that the «non-luminous heat» (now known as infra - red
radiation) then emitted by the Earth's surface could not make it
back in the opposite direction quite so readily.