The theory of Anthropogenic Global Warming, in particular, is based
on radiation physics.
Not exact matches
The Big Bang Theory was as proven as something could get four years ago by the winner of the Nobel Prize in
physics who discovered
radiation in our universe
on a scale and pattern that could only be explained by a gigantic explosion that created our universe 6 billion years ago.
«The evidence that these new gravitational waves are from merging neutron stars has been captured, for the first time, by observatories
on Earth and in orbit that detect electromagnetic
radiation, including visible light and other wavelengths,» said Chad Hanna, assistant professor of
physics and of astronomy & astrophysics and Freed Early Career Professor at Penn State.
His colleagues have publicly stated his writing children's books
on science had an adverse effect
on his scientific reputation, and people could not take him seriously when he and his colleagues proposed that there should be a cosmic background
radiation, which we now know to be one of the greatest discoveries of 20th - century
physics.
MARIE AND PIERRE CURIE, who married in 1895 and shared the 1903 Nobel Prize in
physics for their research
on radiation.
The findings appeared in the May issue of Scientific Reports and were presented by UNLV scientist Francis Cucinotta, a leading scholar
on radiation and space
physics.
«Research
on the ISS is being conducted in areas as diverse as high - energy particle
physics, Earth remote sensing, protein crystallization, human physiology,
radiation, plant cultivation experiments, fluids, combustion, materials science and biology,» she said.
Participation in these courses provides valuable hands -
on laboratory training in cutting - edge research in fields such as biomedical optics, atomic and nuclear
physics, acoustics, and
radiation dosimetry.
Francis Cucinotta, professor in the Department of Health
Physics and Diagnostic Sciences, studies the impact of
radiation on humans, including astronauts.
The Space Science Laboratory (as part of the wider Solar
Physics and Space Plasma Research Centre (SP2RC) at The University of Sheffield) was recently awarded the STFC grant «Dynamics of key
radiation belt emissions» (April 2018 to March 2021) and the successful applicant would have the opportunity to contribute to this active research project (depending
on the topic of PhD chosen).
It depends: The health
physics society site is an excellent resource
on radiation dose and effect: http://hps.Org/.
The idea for a spinoff medical technology company originated several years ago when Medlin and his adviser, Endre Takacs, were working in Clemson's Atomic and Medical
Physics lab
on an experiment with bioengineers to systematically study the effects of low - dose
radiation on living cell cultures.
In addition, the first conceptual paper
on adaptive
radiation therapy in
Physics in Medicine and Biology, co-authored by Dr. Wong, was selected as one of the journal's 25 most important papers published in its 60 - year history.
Brian Wirth, UT - ORNL Governor's Chair for Computational Nuclear Engineering, was nominated by the AAAS section
on physics for «advancing knowledge of
radiation damage mechanisms and fuel performance in fission and fusion energy via multiscale modeling using high performance computing validated by experiments.»
In addition to UNLV's work, consortium members will focus
on nuclear and particle
physics, nuclear engineering, and nuclear instrumentation and
radiation detection.
CT + Review and Essentials gives you an 18 module / 17 credit course focused
on contrast administration, cross-sectional anatomy,
physics and instrumentation,
radiation safety, dosimetry, and more!
The research was led by UNLV professor Francis Cucinotta, a former NASA scientist and a leading scholar
on radiation and space
physics, and featured in dozens of publications around the globe.
Also a useful tie in for the
physics topic
on «
radiation».
One is to acknowledge that calculation of
radiation transport through a partially opaque atmosphere is one of those problems that seems easy until you try to write down the equations, and then you find it's a monster — the great mathematical physicist S. Chandrasekhar spent years working
on it and wrote a book full of equations
on stellar atmospheres that I think hardly anyone in atmospheric
physics even tries to read.
By the way, my arguments assume that tokamak
physics and technology works well and is reasonably simple, meaning that not many more components will have to be added to the system to allow it to operate
on a steady basis for very long periods of time between the long shutdowns needed to change out
radiation - damaged, radioactive materials.
Most people don't understand the details of atmospheric
physics or principal components analysis, and so take many statements about «back -
radiation» and «hockeysticks»
on trust.
Looking in a textbook about atmospheric
physics, meteorology or climate
physics it is getting quite clear that atmospheres are more complex then just reducing their thermal structure
on the effects of solar
radiation and greenhouse gases alone.
The
physics of greenhouse gases (= by definition gases that absorb thermal
radiation) is essential to get appropriate physical models explaining the observations quantitatively and allow to evaluate what happen
on changed conditions by virtual experiments.
In terms of building
physics, this increases the probability that condensation might form
on the outer surface of the façade due to the cooling effect of long - wave
radiation of heat during the night.
The meeting will mainly cover the following themes, but can include other topics related to understanding and modelling the atmosphere: ● Surface drag and momentum transport: orographic drag, convective momentum transport ● Processes relevant for polar prediction: stable boundary layers, mixed - phase clouds ● Shallow and deep convection: stochasticity, scale - awareness, organization, grey zone issues ● Clouds and circulation feedbacks: boundary - layer clouds, CFMIP, cirrus ● Microphysics and aerosol - cloud interactions: microphysical observations, parameterization, process studies
on aerosol - cloud interactions ●
Radiation: circulation coupling; interaction between
radiation and clouds ● Land - atmosphere interactions: Role of land processes (snow, soil moisture, soil temperature, and vegetation) in sub-seasonal to seasonal (S2S) prediction ●
Physics - dynamics coupling: numerical methods, scale - separation and grey - zone, thermodynamic consistency ● Next generation model development: the challenge of exascale, dynamical core developments, regional refinement, super-parametrization ● High Impact and Extreme Weather: role of convective scale models; ensembles; relevant challenges for model development
Correct
physics tells us that the Sun's
radiation can,
on average, only raise the temperature in colder regions well up in the troposphere.
See this medical
physics ppt dealing with the interaction of ionizing
radiation with matter
on a molecular level.
It depends
on a major error by Houghton who used the Schuster - Schwarzchild «two - stream approximation» which is used in astrophysics but breaches the most basic of
radiation physics, Poynting's Theorem, which states that the vector sum of all arriving vectors at a point.
The big difference between this scenario is that the
radiation from the lamp AND the
radiation from the glass originate in materials at significantly higher temperatures than the gases and hence heat IS transferring from HOT to COLD unlike the fanciful «back radiative greenhouse effect» which truly defies the laws of
Physics relying instead
on pixie dust magic!
The biggest error of all the errors in the
physics of the radiative greenhouse conjecture is that they «explain» the surface temperature of 288K using Stefan - Boltzmann calculations based
on the direct solar
radiation PLUS about TWICE as much supposed thermal energy input from the colder atmosphere.
Nearly all of the equations in
physics are approximations, and those used in climate science that I have seen to date are all based
on some simplifications (equilibrium, for example; or ignoring the fact that 22 % if incoming TOA
radiation is absorbed in the upper atmosphere.)
[62] see the graph comparing surface
radiation absorbed by the air and
radiation of the air to the surface in Dr. Ferenc M. Miskolczi
Physics of the planetary greenhouse effect International conference
on global warming, New York, March -4, 2008.
The sensitivity of the models is, as I think you are saying, constrained by it's parametrizations, which are bounded by observational data
on TOA
radiation data etc. (although not all very tightly constrained) but this is not what is being questioned about the models, rather the issue is whether the model hindcasts matching historical temperatures to some degree is evidence that they have correct
physics, or is merely a result of modelers making the choices for inputs which will produce a reasonable result.
The
physics that must be included to investigate the moist greenhouse is principally: (i) accurate
radiation incorporating the spectral variation of gaseous absorption in both the solar
radiation and thermal emission spectral regions, (ii) atmospheric dynamics and convection with no specifications favouring artificial atmospheric boundaries, such as between a troposphere and stratosphere, (iii) realistic water vapour
physics, including its effect
on atmospheric mass and surface pressure, and (iv) cloud properties that respond realistically to climate change.
This website ran an article a few weeks back, or had some comments from Tom C, or somebody
on exactly how CO2 infuences
radiation at a quantum
physics level.
They provide material
on the science of climate change assuming that the users already have a basic understanding of geophysical fluid dynamics, and relevant physical processes such as
radiation transfer, diffusion, the hydrological cycle, and cloud
physics along with some understanding of air chemistry, hydrology, and oceanography.
In this way I've benefited from courses
on global climate change, climatology, future energy supply and demand, the
physics of the greenhouse effect and planetary
radiation balance, and climate politics and policy options.
Well Debs it's pretty basic isn't — the complex
radiation models built
on Nasif's alleged incorrect
physics seem to validate out
on observed data.