Not exact matches
Wu was the first to verify — and later refine — Enrico Fermi's theory of radioactive beta - decay, which describes
how some unstable atoms
emit radiation when transforming into more stable atoms.
Researchers looked at seven of these worlds — distant planets whose mass lies between one and 10 times ours — including 55 Cancri e (at right, compared to Earth) and GJ1214b, evaluating
how the x-ray and extreme ultraviolet
radiation emitted by their parent stars might affect their atmospheres over their remaining lifetimes.
To determine the location of a star's habitable zone, one must first learn
how much total
radiation it
emits.
They then looked at another source of data: that of the Clouds» and Earth's Radiant Energy System (CERES) satellite instruments which measure fluxes of reflected and
emitted radiation from Earth to space, to help scientists understand
how the climate varies over time.
But these clocks are constrained in
how precisely they can divide time because when caesium electrons jump from a certain state to another they
emit radiation with a frequency of only 9 giga - hertz, or 9 billion cycles per second.
«Radio emissions from the regions in which clusters collide were first detected almost 20 years ago, but no one was able to explain
how electrons could be accelerated to the point where they
emitted radiation in this frequency band.
But pulsars
emit gamma rays, and scientists such as KIPAC's Roger Romani can study these to measure their rotation and understand
how high - energy
radiation is generated in their intense magnetic fields.
What other things in the Earth system will change when it warms up that will affect
how much SW
radiation is reflected back into space [eg ice - albedo feedback, cloud changes] or affect what proportion of
emitted LW
radiation is allowed to escape to space [eg Water Vapour, cloud changes].
Miskolczi's optical thickness is
how much of the surface
emitted IR
radiation reaches the top untouched and is equivalent to 15 %.
How can the earth be radiating a crude BB type spectrum corresponding to the surface Temperature when Trenberth claims that only 40 W / m ^ 2 escapes to space in the atmospheric window, and folks insist that the main body of the atmosphere (gases) does not
emit thermal
radiation.
«The top - of - atmosphere (TOA) Earth
radiation budget (ERB) is determined from the difference between
how much energy is absorbed and
emitted by the planet.
1) Werner Becker of the Max Planck Institute for Extraterrestrial Physics said in 2006, «The theory of
how pulsars
emit their
radiation is still in its infancy, even after nearly forty years of work.»
But there may be a difference in
how much energy is
emitted as
radiation versus hot gas.
tallbloke says: August 8, 2011 at 4:46 am 1) Werner Becker of the Max Planck Institute for Extraterrestrial Physics said in 2006, «The theory of
how pulsars
emit their
radiation is still in its infancy, even after nearly forty years of work.»
How you conceive of these two sentences, «What happens is that if more
radiation reaches the surface, then it warms up and more
radiation is
emitted to space.
One particularly thorny aspect of the MJO is determining
how much heat is transferred between the ocean and throughout the atmosphere by convection and
how much heat is absorbed or
emitted in the form of
radiation.
10
How the Atmosphere Affects Climate (Page 273) Earth's atmosphere can absorb and reflect
radiation emitted from the Sun and from Earth's surface.
So
radiation has a chance if directed downward to reach the surface no matter
how high in the atmosphere it is
emitted, it's just that the chance fades quickly as you count lengths or shells.
How is convection going to «wipe out» a molecule's ability to absorb /
emit certain wavelengths of
radiation?
First, the quote is not dealing with what the result of reabsorbing its own
radiation is but
how to calculate the total
emitted power of a body with a complex shape.
Similarities may exist in the spectral nature of the
radiation being
emitted from a gas and the
radiation being
emitted from a differential area on a blackbody surface; but without a clearly defined surface, I don't see
how Planck's blackbody
radiation law can be applied.
How a gas, atom, molecule, etc responds to thermal
radiation, or
emits thermal
radiation, is dependent on the conditions of the environment it is placed within.
Does Hitran simply use a plank distribution to determine the amount of
emitted radiation and if so
how does the model determine the temperature?
B)
How does» Across the wavelengths where the earth is
emitting its own
radiation (4μm - 40μm) it has an emissivity close to 1.»
The temperature determines
how much long wave IR
radiation is
emitted by the surface and greenhouse gases.
Shortly after that first staff up - rising had been suppressed by issuing manuals for learning
how to type at great speed, they expressed concern that those «machines» allegedly
emitted dangerous
radiation.