I was at an international conference on aerosol in September and I made a comment that we're getting to the stage with CLOUD where we will understand the processes extremely well, but we still won't be able to reduce the errors because we don't have good enough
atmospheric observations of what the concentrations of these vapors are in the atmosphere versus altitude.
GLOBALVIEW data products are designed to enhance the spatial and temporal distribution of
atmospheric observations of CO2, CH4 and other related atmospheric measurements.
The researchers hope that their technique may prove especially useful when upcoming space missions such as NASA's James Webb Space Telescope and the European Space Agency's Ariel Space Mission start providing more detailed
atmospheric observations of potentially habitable exoplanets.
Not exact matches
Trapped beneath Earth's ocean
of air, ground - based observatories will be stymied by starlight - warping turbulence, and by airglow — faint light emitted by
atmospheric chemical reactions that can corrupt delicate
observations.
Combining
observations from satellites and ground stations with climate models, they evaluated different factors that affect telescope vision, such as the amount
of water vapour, wind speeds and
atmospheric turbulence.
Trapped below Earth's ocean
of air, even the largest ground - based observatories will be stymied by starlight - warping turbulence and by airglow, faint light emitted by
atmospheric chemical reactions that can corrupt delicate
observations.
«Although a direct causal link has not been established between the
atmospheric phenomena observed in late October 2012 and the record - breaking sea - ice loss observed during the preceding summer months, all
of the
observations are consistent with such an interpretation,» states the Oceanography article.
Observations obtained a month later by members
of the Planetary Sciences Group using the PlanetCam camera developed by this team and fitted to the 2.2 - m telescope at the Calar Alto Observatory in Almería (Spain) enabled the speed
of this
atmospheric structure to be confirmed.
Mission leaders were relieved and eager to begin their studies
of cloud and haze effects, which «constitute the largest uncertainties in our models
of future climate — that's no exaggeration,» says Jens Redemann, an
atmospheric scientist at NASA's Ames Research Center in Mountain View, California, and the principal investigator for
ObseRvations of Aerosols above CLouds and their IntEractionS (ORACLES).
This global biological recordbased on daily
observations of ocean algae and land plants from NASAs Sea - viewing Wide Field -
of - View Sensor (SeaWiFS) missionwill enable scientists to study the fate
of atmospheric carbon, terrestrial plant productivity and the health
of the oceans food web.
«Advances in global climate models and high quality ocean,
atmospheric and land
observations are helping us push the frontiers
of snowpack prediction.»
What is more, because Jupiter's microwave emissions vary in wavelength based on the pressure (as well as temperature)
of the
atmospheric layers where they originate,
observations at multiple wavelengths allow researchers to create a cross-section through the atmosphere.
«But no one has had a comprehensive set
of observations of what really happens after you seed a cloud,» says Jeff French, an
atmospheric scientist at the University
of Wyoming (UW) and SNOWIE principal investigator.
Using published data from the circumpolar arctic, their own new field
observations of Siberian permafrost and thermokarsts, radiocarbon dating,
atmospheric modeling, and spatial analyses, the research team studied how thawing permafrost is affecting climate change and greenhouse gas emissions.
Other than in previous publications, optical rogue waves in this system are clearly ruled by
atmospheric turbulence in a gas cell, effectively enabling the
observation of a storm in a test tube.
«It may even be possible to predict sea ice cover a year in advance with high - quality
observations of sea ice thickness and snow cover over the whole Arctic,» said Cecilia Bitz, co-author and professor
of atmospheric sciences at the University
of Washington.
Observations of atmospheric carbon dioxide made by aircraft at altitudes between 3 and 6 kilometers (10,000 - 20,000 feet) show that seasonal carbon dioxide variations have substantially changed during the last 50 years.
The findings come from a multi-year airborne survey
of atmospheric chemistry called HIAPER Pole - to - Pole
Observations, or HIPPO.
This discovery, and other
observations made by the Penn State team, provide insight into the complexity
of weather and
atmospheric composition on exoplanets, and may someday be useful for gauging the habitability
of Earth - size planets.
Hubble
observations of the planet's
atmospheric temperature profile represent the first time astronomers have detected this precipitation process, called a «cold trap,» on an exoplanet.
«The
atmospheric carbon dioxide
observations are important because they show the combined effect
of ecological changes over large regions,» says Graven.
In addition, satellite
observations of the ocean surface and
atmospheric data were included.
The UM Rosenstiel School researchers used historical
observations of cloud cover as a proxy for wind velocity in climate models to analyze the Walker circulation, the
atmospheric air flow and heat distribution in the tropic Pacific region that affects patterns
of tropical rainfall.
To arrive at their results, the researchers combined
observations from the past century with climate simulations
of the
atmospheric response to the AMO.
The study authors based their analysis on a combination
of satellite
observations of rainfall and vegetation and an
atmospheric circulation model to track the movement
of air masses.
MAGIC has been designed to be the most suitable instrument among imaging
atmospheric Cherenkov telescopes to perform this kind
of observations.»
Roe and his U.W. co-author,
atmospheric physicist Marcia Baker, argue in Science that, because
of this inherent climate effect, certainty is a near impossibility, no matter what kind
of improvements are made in understanding physical processes or the timescale
of observations.
The model is supported by
observations from satellites, ground - based networks that measure ozone - depleting chemicals in the real world, and by
observations from two decades
of NASA aircraft field campaigns, including the most recent Airborne Tropical Tropopause Experiment (ATTREX) in 2013 and the
Atmospheric Tomography (ATom) global
atmospheric survey, which has made three deployments since 2016.
The ARM Facility has provided the world's
atmospheric scientists with continuous
observations of cloud and aerosol properties and their impacts on the Earth's energy balance for more than 20 years.
Your statement that «Thus it is natural to look at the real world and see whether there is evidence that it behaves in the same way (and it appears to, since model hindcasts
of past changes match
observations very well)» seems to indicate that you think there will be no changes in ocean circulation or land use trends, nor any subsequent changes in cloud responses thereto or other
atmospheric circulation.
I am excited about our results because they open a new window on very fundamental processes in brown dwarfs (
atmospheric circulation, heat exchanges, and cloud formation) and, at the same time, they also explain a number
of past
observations that puzzled brown dwarf experts.
The Aerosol Measurement Science Group (AMSG) coordinates ARM Facility
observations of aerosols and
atmospheric trace gases with user needs.
In combinations with numerical simulations, these
observations can help constrain the properties
of the waves, as well as the background states for wave propagation, for instance, the
atmospheric stratification.
«These unexpected
observations remind us keenly
of how little we understand about
atmospheric dynamics in outer planet atmospheres,» the authors wrote in their paper.
Eclipse
observations, where Jupiter eclipses Io for a few hours approximately every two days, also offer another way
of testing
atmospheric support.
With HST - Spitzer transit and eclipse
observations we constrain the compositions and
atmospheric thermal structure
of twenty
of the brightest exoplanets.
These
observations represent the first constraints on the
atmospheric dynamics
of a highly irradiated brown dwarf, and the atmospheres
of irradiated giant planets at high surface gravity.
The
observations are best described by
atmospheric models for which most
of the incident energy is re-radiated away from the day side.
Satellite
observations indicate that the iron - fertilised phytoplankton blooms north
of South Georgia are amongst the most intense south
of the Polar Front and form the largest seasonal sink
of atmospheric CO2 in the Southern Ocean.
Previous proofs have relied on complex climate models, but this proof doesn't need such models — just careful
observations of the land, ocean and
atmospheric gases.»
Therefore, what Hansen's models and the real - world
observations tell us is that climate sensitivity is about 40 % below 4.2 °C, or once again, right around 3 °C for a doubling
of atmospheric CO2.
Miller, S. M., et al. (2016), A multiyear estimate
of methane fluxes in Alaska from CARVE
atmospheric observations, Global Biogeochem.
Many
of the planets discovered by EDEN around nearby stars will be suitable for in - depth
atmospheric characterization, mass, radius, and bulk density measurements through follow - up
observations with large ground - and space - based telescopes, such as NASA's James Webb Space Telescope.
The Finnish Meteorological Institute started meteorological
observations on the island in 1881, and
atmospheric trace gas and aerosol measurements as member
of the EMEP - network in 1980.
Other types
of atmospheric pollution can interfere with astronomic
observations as well.
This high frequency
observation was made possible by the combination
of ideal
atmospheric condition (dryness)
of the Atacama Desert, high surface accuracy
of the antenna, and proper functions
of all components as an entire array system including the Band 10 receiver.
Scientists are using airborne
observations of atmospheric trace gases, aerosols, and cloud properties from the North Slopes
of Alaska to improve their understanding
of global climate, with the goal
of reducing the uncertainty in global and regional climate simulations and projections.
The biogeochemical impacts
of this «fertilization» remain unclear, as direct oceanic
observations of atmospheric deposition are limited and models often can not resolve the important processes.
This method tries to maximize using pure
observations to find the temperature change and the forcing (you might need a model to constrain some
of the forcings, but there's a lot
of uncertainty about how the surface and
atmospheric albedo changed during glacial times... a lot
of studies only look at dust and not other aerosols, there is a lot
of uncertainty about vegetation change, etc).
LASSO will enhance ARM
observations by using large - eddy simulation (LES) modeling to provide context and a self - consistent representation
of the atmosphere surrounding the Southern Great Plains (SGP)
atmospheric observatory.