«We created the largest database of
surface ozone from hourly observations at more than 4,800 monitoring sites worldwide, and we're making these data freely available to anyone who wants to investigate the impact of ozone on human health, vegetation, and climate.»
Not exact matches
Emissions
from vehicles, power plants, industrial operations, and other human activities are a primary cause of
surface ozone, which is one of six main pollutants regulated in the U.S. by the Clean Air Act.
Without the
ozone layer, ultraviolet rays
from the sun would reach the
surface at nearly full force, causing skin cancer and, more seriously, killing off the tiny photosynthetic plankton in the ocean that provide oxygen to the atmosphere and bolster the bottom of the food chain.
Even down on the Red Planet's
surface, the Curiosity rover might be able to get in on the act: Because Mars's atmosphere has no
ozone to block ultraviolet light, sensors on the rover will be able to detect those wavelengths and thereby monitor certain trace gases spewing
from the comet — unless a dust storm blocks the view to space, Lemmon says.
In order to keep aerosols
from harming the
ozone, the particles would need to neutralize sulfuric, nitric, and hydrochloric acid on their
surface.
Over the last 50 years satellite and ground - based records over Antarctica show
ozone column amounts ranging
from 100 to 400 Dobson units, which translates to about 1 millimeter (1/25 inch) to 5 millimeters (1/6 inch) of
ozone in a layer if all of the
ozone were brought down to the
surface.
In the high atmosphere,
ozone plays a crucial role in shielding the
surface from harmful levels of ultraviolet light.
The
ozone concentrations in his measurements remained nearly constantly below the detection limit of approx. 10 ppbv in the entire vertical range
from the
surface of Earth to an altitude of around 15 kilometres.
On Earth, temperature inversion occurs because
ozone in the stratosphere absorbs much of the sun's ultraviolet radiation, preventing it
from reaching the
surface, protecting the biosphere, and therefore warming the stratosphere instead.
Ozone high in the atmosphere protects Earth's
surface from ultraviolet light.
Because
ozone in the troposphere is a precursor to OH, they deployed weather balloons equipped with measuring devices known as sondes to measure the amount of
ozone in the air
from the
surface to the stratosphere.
Earth's
ozone layer, 10 kilometres above the
surface, is produced when light
from the Sun interacts with molecules of oxygen in our atmosphere, and it produces an unmistakable signal that could be detected by JWST.
Short - lived bromine compounds naturally released
from the ocean
surface, however, have a more pronounced impact on
ozone than their short - lived industrial cousins.
«If the star is active (as indicated by the X-ray flux) then [a planet in orbit] needs an
ozone layer to shield its
surface from the harsh UV that would sterilize the
surface,» Kaltenegger said.
It contributes to the water vapor continum in the window and this is similar to the
ozone, producing a flux change that can be seen
from above as
from the
surface.
Certain particles may have a damaging effect on the
ozone layer, vital for keeping harmful UV rays away
from the
surface of the Earth.
I used was the
surface temperature responses
from histAll --(histGHG + histNatural) to obtain the response to aerosols +
ozone + land - use and derive the enhancement of the response for that case relative to WMGHGs that I called E. Calculation of TCR based on histAll in a model is approximately the same as calculating the sum of responses to histGHG, histNat, and histInhomogeneous where the latter includes the factor E.
The TOAR database contains the world's largest collection of
ozone metrics, calculated consistently
from hourly
ozone observations at all available
surface monitoring sites around the globe.
Consistency for
surface ozone levels was more difficult to achieve due to the influence of emissions
from up - wind regions.
A team of researchers
from the NASA's Jet Propulsion Laboratory in California and the Wageningen University in the Netherlands measured the amount of
ozone between 10,000 and 30,000 feet above the Earth's
surface.
Ozone, made
from three bound oxygen atoms, helps filter the sun's harmful UV rays
from Earth's
surface.
Like the other greenhouse gases,
ozone blocks heat
from the Earth's
surface and prevents it
from escaping into outer space.
The point being that w / out ongoing decimation
from soot, wind,
ozone (
surface ozone pollution that warms
from UV), the AO and greenhouse gases, the ice would have been more likely to recover
from the impact of such an event.
The lack of
ozone is chilling the middle and upper atmosphere, altering wind patterns in a way that keeps comparatively warm air
from reaching the
surface.
The springtime stratospheric
ozone hole &
surface ozone also have an impact, and the combination of soot &
surface ozone would exceed the impact
from greenhouse gases (soot deposition alone is on par with greenhouse gases in the boreal thaw).
Due to the important role of
ozone in driving temperature changes in the stratosphere as well as radiative forcing of
surface climate, several different groups have provided databases characterizing the time - varying concentrations of this key gas that can be used to force global climate change simulations (particularly for those models that do not calculate
ozone from photochemical principles).
This process occurs variously
from 20 to 40 km above the
surface in the
Ozone Layer.
Now with a slightly different group, Li has compiled data
from multiple sources and performed model simulations to investigate the possibility that Arctic stratospheric
ozone is connected to the ENSO via the North Pacific sea -
surface temperature (SST).
However, many of the aerosols scientists have suggested using, such as diamond dust or alumina, are harmful to the
ozone (a layer that protects the Earth's
surface from some of the sun's ultraviolet rays) and human health.
Ozone is vital in protecting the Earth's
surface from solar UV and is itself a tiny trace gas in the atmosphere.
Last week, one of these unexpected disasters was suddenly revealed: a paper in Science argued that powerful thunderstorms threaten to rip a hole in the atmospheric
ozone layer that protects the planet's
surface from dangerous ultraviolet (UV) radiation
from the sun.
'' «It all amounts to a mystery, but a troubling one because
ozone protects life at the
surface from incoming ultraviolet radiation, and any thinning of total
ozone in the stratosphere is cause for concern.
Absorption of solar radiation by
ozone shields the terrestrial
surface from harmful ultraviolet light and warms the stratosphere, producing maximum temperatures of − 15 to 10 °C (5 to 50 °F) at an altitude of 50 km (30 miles).
52 • Immune system suppression Natural Capital Degradation Effects of
Ozone Depletion Human Health • Worse sunburn • More eye cataracts • More skin cancers • Immune system suppression Food and Forests • Reduced yields for some crops • Reduced seafood supplies from reduced phytoplankton • Decreased forest productivity for UV - sensitive tree species Wildlife • Increased eye cataracts in some species • Decreased population of aquatic species sensitive to UV radiation • Reduced population of surface phytoplankton • Disrupted aquatic food webs from reduced phytoplankton Figure 20.21 Natural capital degradation: expected effects of decreased levels of ozone in the stratosp
Ozone Depletion Human Health • Worse sunburn • More eye cataracts • More skin cancers • Immune system suppression Food and Forests • Reduced yields for some crops • Reduced seafood supplies
from reduced phytoplankton • Decreased forest productivity for UV - sensitive tree species Wildlife • Increased eye cataracts in some species • Decreased population of aquatic species sensitive to UV radiation • Reduced population of
surface phytoplankton • Disrupted aquatic food webs
from reduced phytoplankton Figure 20.21 Natural capital degradation: expected effects of decreased levels of
ozone in the stratosp
ozone in the stratosphere.
The various kinds of evidence examined by the panel suggest that the troposphere actually may have warmed much less rapidly than the
surface from 1979 into the late 1990s, due both to natural causes (e.g., the sequence of volcanic eruptions that occurred within this particular 20 - year period) and human activities (e.g., the cooling of the upper part of the troposphere resulting
from ozone depletion in the stratosphere).
The wind patterns may have changed due to a combination of the current Pacific Decadal Oscillation which has now started changing, and the
ozone hole allowing more sunlight to reach the
surface rather than being absorbed in the stratosphere; the extra energy
from this may have accelerated the winds.
This stratospheric
ozone layer prevents the Sun's harmful, high - energy radiation
from reaching Earth's
surface.
This is problematic because
ozone blocks harmful radiation — which can damage DNA and lead to skin cancer, among other problems —
from reaching the Earth's
surface.
Chemical processes on the
surface of the cloud particles transform the initially harmless chemicals
from chlorofluorocarbons (CFCs) into aggressive
ozone - depleting substances.
When the intensity of ultraviolet light
from the sun increases, temperature rises in this
ozone rich air and weakens the downdraft, lowers the
surface pressure and with it the strength of the trade winds that blow across the ocean to the low pressure zones that form over the warm waters that accumulate in the west.
Ozone is a molecule made up of three oxygen atoms, and the ozone layer, which stretches from heights of 12 to 19 miles (20 to 30 kilometers) above the Earth's surface, protects life on Earth by shielding it from ultraviolet (UV) radia
Ozone is a molecule made up of three oxygen atoms, and the
ozone layer, which stretches from heights of 12 to 19 miles (20 to 30 kilometers) above the Earth's surface, protects life on Earth by shielding it from ultraviolet (UV) radia
ozone layer, which stretches
from heights of 12 to 19 miles (20 to 30 kilometers) above the Earth's
surface, protects life on Earth by shielding it
from ultraviolet (UV) radiation.
Until the 1990s, the widespread use of chlorofluorocarbons (CFCs) for refrigerants and aerosols created an
ozone hole in the Earth's stratosphere (the second layer of the atmosphere
from Earth's
surface) over Antarctica.
The climate system is highly non-linear8 and relatively little is known about the effect on temperature changes resulting
from human contributions to the changing three - dimensional distributions of
ozone and aerosols, either or both of which may have been partially responsible for the observed discrepancy between
surface and lower to mid-tropospheric temperature changes.
Stratospheric
ozone has been called «good»
ozone because it protects the Earth's
surface from dangerous ultraviolet light.
Its warm here because
Ozone is stopping solar radiation
from getting to the
surface but this heats up the
Ozone.
The
ozone layer blocks harmful radiation — which can damage DNA and lead to skin cancer, among other problems — preventing it
from reaching the Earth's
surface.
The
ozone layer is important, because it prevents harmful ultraviolet radiation
from reaching the
surface of the planet.
Some of the heat flowing back toward space
from the Earth's
surface is absorbed by water vapor, carbon dioxide,
ozone and several other gases in the atmosphere and then re-radiated back toward the Earth's
surface.
These problems are compounded by crop damage
from ozone partly produced by cookstove emissions, and
from surface dimming that results as airborne black carbon intercepts sunlight.
60 • Immune system suppression Natural Capital Degradation Effects of
Ozone Depletion Human Health • Worse sunburn • More eye cataracts • More skin cancers • Immune system suppression Food and Forests • Reduced yields for some crops • Reduced seafood supplies from reduced phytoplankton • Decreased forest productivity for UV - sensitive tree species Wildlife • Increased eye cataracts in some species • Decreased population of aquatic species sensitive to UV radiation • Reduced population of surface phytoplankton Figure 20.21 Natural capital degradation: expected effects of decreased levels of ozone in the stratosp
Ozone Depletion Human Health • Worse sunburn • More eye cataracts • More skin cancers • Immune system suppression Food and Forests • Reduced yields for some crops • Reduced seafood supplies
from reduced phytoplankton • Decreased forest productivity for UV - sensitive tree species Wildlife • Increased eye cataracts in some species • Decreased population of aquatic species sensitive to UV radiation • Reduced population of
surface phytoplankton Figure 20.21 Natural capital degradation: expected effects of decreased levels of
ozone in the stratosp
ozone in the stratosphere.