Sure, he also equated (perhaps unknowingly) GCM's
with radiation modelling techniques so that the audience might further confuse the former with the straight - forward latter.
Not exact matches
In December 2017, writing in Computer Methods in Applied Mechanics and Engineering, Yankeelov and collaborators at UT Austin and Technical University of Munich, showed that they can predict how brain tumors (gliomas) will grow and respond to X-ray
radiation therapy
with much greater accuracy than previous
models.
Experts say the dose from the backscatter is negligible when compared
with naturally occurring background
radiation, but a linear
model shows even such trivial amounts increase the number of cancer cases
In further studies, the researchers tested the capacity of ANG to prevent and mitigate
radiation - induced bone marrow failure, and in pre-clinical
models, they found that survival following
radiation exposure was increased after treatment
with recombinant ANG protein.
In a bid to progress beyond the shotgun approach to fighting cancer — blasting malignant cells
with toxic chemicals or
radiation, which kills surrounding healthy cells in the process — researchers at the Harvard - MIT Division of Health Sciences and Technology (HST) are using nanotechnology to develop seek - and - destroy
models to zero in on and dismantle tumors without damaging nearby normal tissue.
«In this study we've used a bacterium
with unrivalled resistance to
radiation as a
model for the type of bacteria we might find signs of on Mars.
The scientists worked
with model bacteria that are representative of the sort of microbial lifeforms that might be expected to have emerged on Mars and used a Raman spectrometer to track how the detectable signal from them changed
with increasing exposure to
radiation.
«Our results are based on a realistic
modelling of the accretion of gas onto the black holes, and of the
radiation they emit, which is compatible
with current astronomical observations.
All these accessories, plus a
model rifle, were tagged
with retroreflectors, which can reflect a beam of
radiation back to its source regardless of the angle of incidence.
New climate
models — made by using estimated
radiation levels from that time, along
with data from the Magellan spacecraft about Venus's current surface — suggest that Venus would have been only 11 °C (52 °F).
Several natural causes were tested
with the
model, including volcano eruptions and changes in the sun's
radiation.
By comparing recent measurements
with results from new
models, the network challenged the long - debated assumption that the Sun's slight change in
radiation could cause Earth's climate to change.
New computer
modeling suggests that high temperature TPV conversion — which captures infrared
radiation from very hot surfaces — could one day rival combined - cycle turbine systems when combined
with thermal storage using liquid metal at temperatures around 1,300 degrees Celsius.
This
model describes three types of forces: electromagnetic interactions, which cause all phenomena associated
with electric and magnetic fields and the spectrum of electromagnetic
radiation; strong interactions, which bind atomic nuclei; and the weak nuclear force, which governs beta decay — a form of natural radioactivity — and hydrogen fusion, the source of the sun's energy.
The latest study of the afterglow of the big bang — the so - called cosmic microwave background
radiation — confirms even more precisely the standard
model of cosmology — and that's a victory for the theory — but it leaves researchers
with no discrepancies that might point to a deeper understanding.
Starting
with data taken from observations of the cosmic background
radiation — a flash of light that occurred 380,000 years after the big bang that presents the earliest view of cosmic structure — the researchers applied the basic laws that govern the interaction of matter and allowed their
model of the early universe to evolve.
With the inclusion of
radiation pressure, the 2017
models show how these two factors can create spirals like those also observed around the same star.
To calculate the exposure risks, or the chance that a person will be diagnosed
with cancer, Cucinotta and others studying cosmic
radiation examine and develop theoretical
models.
T - cells (red, yellow, and blue) attack a tumour in a mouse
model of breast cancer following treatment
with radiation and a PD - L1 immune checkpoint inhibitor, as seen by transparent tumour tomography.
Injecting breast cancer
with oxygen - filled microbubbles makes tumors three - times more sensitive to
radiation therapy and improves survival in animal
models of the disease.
Here we show the usefulness of combining survey sequencing
with dense
radiation - hybrid (RH) maps for extracting maximum comparative genome information from
model organisms.
They were able to combine their data
with observations from other telescopes and revealed an almost featureless spectrum that could not be completely explained by a blackbody
model (blackbodies are opaque objects that emit thermal
radiation).
The analysis ascribes that a large EF underestimate is the dominant source of error in all
models with a large positive temperature bias, whereas an EF overestimate compensates for an excess of absorbed shortwave
radiation in nearly all the
models with the smallest temperature bias.
Older skylights were simply a single thickness of glass in a frame, newer
models come
with laminated or tempered glass, and low - e and tinted coatings to control heat transmission and UV
radiation.
Lessons from simple toy
models and experience
with more sophisticated GCMs suggests that any perturbation to the TOA
radiation budget from whatever source is a pretty good predictor of eventual surface temperature change.
The work is an estimate of the global average based on a single - column, time - average
model of the atmosphere and surface (
with some approximations — e.g. the surface is not truly a perfect blackbody in the LW (long - wave) portion of the spectrum (the wavelengths dominated by terrestrial / atmospheric emission, as opposed to SW
radiation, dominated by solar
radiation), but it can give you a pretty good idea of things (fig 1 shows a spectrum of
radiation to space); there is also some comparison to actual measurements.
You can play
with this yourself using the online modtran or ncar
radiation models.
Looking at the surface temperature and the ocean heat content changes together though allows us to pin down the total unrealised forcing (the net
radiation imbalance) and demonstrate that the
models are consistent
with both the surface and ocean changes.
If the
models don't reflect such differences in
radiation balance between the hemispheres, then there is something wrong
with the
models... But globally, the oceans are warming (much) faster in the NH than in the SH...
What climate
models assume is a wide - ranging compendium of physical processes that are either well known but too complicated to incorporate into the climate
model (for example the direct radiational effect of Carbon Dioxide on greenhouse warming is considerably * simplified * compared to the most sophisticated «line - by - line»
radiation models that are available, simply because there isn't enough computer power to make the line - by - line calculation at every location on Earth at every time step within in a GCM), or are not sufficiently well - known to treat them
with complete certainty.
The basic ingredients are easy to list: — absorption / emission properties (or spectroscopic parameters) of CO2 at atmospheric pressures, i.e. data presently available from HITRAN - database combined
with models of line broadening — observed properties of the atmosphere where most important features include clouds and moisture content, but many other factors have some influence — computer
model of the transmission of
radiation along the lines of MODTRAN or GENLN2
In these planetary GCMs, we use a relatively simple two - stream radiative transfer for scattering and absorbing atmospheres,
with assumed diffuse incident of solar
radiation at the top of the
model domain.
If you are designing an atmospheric
model with molecules that absorb or emit ir energy, N2 and O2 would not be
modeled as absorbing or emitting ir energy through vibrational interactions
with electromagnetic
radiation.
Studies
with climate
models have noted that the ITCZ width depends on interactions between
radiation and clouds (Voigt & Shaw 2015) and how the
model represents sub-grid scale convection (Kang et al. 2009), but a physical understanding of why the ITCZ width is affected by these processes is lacking.
The climate
models further hide the «back
radiation» energy by using double the optical depth for low level clouds compared
with reality.
While the authors found decreases in
radiation loss
with short - term temperature increases, I find that the CMIP
models exhibit an INCREASE in radiative loss
with short term warming.
Even though some of the CMIP
models produce a lot of global warming, all of them are still stable in this regard,
with net increases in lost
radiation with warming (NOTE: If analyzing the transient CMIP runs where CO2 is increased over long periods of time, one must first remove that radiative forcing in order to see the increase in radiative loss).
But for e.g. undergraduate lessons simple
models only taking
radiation transport by greenhouse gases together
with the distribution of solar
radiation are sufficient to demonstrate the effect of greenhouse gases on the earth troposphere and that they are essential to explain their basic thermal structure.
Please show where I have relied on «computer
models with an almost 100 % fail rate» for measurements of back
radiation.
Radiative - covective
models put the surface albedo, gas composition and their infrared absorption together
with the solar irradiation into account, this gives a first guess of the top of troposphere, surface temperature and greenhouse effect (= surface temperature —
radiation temperature).
You can take readings on the
model with a light meter and get a quantitative idea how much (for example) a reflector is increasing
radiation.
A SOM is much cheaper and simpler to run compared to a full ocean
model, but still reacts to things happening in the atmosphere, like changes in downwelling
radiation or fluxes associated
with surface wind.
Their forecast is based on the quantity of incoming solar
radiation using 16 - day forecast from the WRF
model combined
with an assessment of the mechanical stability of the landfast ice cover.
However, climate
models forced
with CO2 reveal that global energy accumulation is, instead, primarily caused by an increase in absorbed solar
radiation (ASR).
The strongest upward motion in the
model's TTL is generally driven by dynamics instead of
radiation, occurring in those TTL cloudy regions that overlap
with optically thick clouds in the upper troposphere (UT).
Once a GCM has cycled for several hundred «years» (and do they
model the «solar year»
with it's changing
radiation and incidences, or only the «average» entire year?)
The
radiation obsessed IPCC science
model with its fictitious 33K effect is false.
Bill Gray has a favorite diagram, taken from a 1985 climate
model, showing little nodules in the center
with such labels as «thermal inertia» and «net energy balance» and «latent heat flux» and «subsurface heat storage» and «absorbed heat
radiation» and so on, and they are emitting arrows that curve and loop in all directions, bumping into yet more jargon, like «soil moisture» and «surface roughness» and «vertical wind» and «meltwater» and «volcanoes.»
Overlap
with water vapor is important for
radiation from clear skies, but shouldn't all
models should get relative humidity correct and agree
with observations from space?
Are you saying that because he uses a LTE
model with atmospheric layers to explain carbon dioxide IR
radiation (and re-
radiation), that he is implying that one should find non-smooth temperatures
with increasing height in such layers?