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Author: Tra Phuong Dinh
Publisher:
ISBN:
Category : Cirrus clouds
Languages : en
Pages : 73
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Book Description
Simulations of tropical-tropopause-layer (TTL) cirrus under the influence of a large-scale equatorial Kelvin wave have been performed in two dimensions. These simulations show that, even under the influence of the large-scale wave, radiatively induced dynamics in TTL cirrus plays an important role in the transport of water vapor in the vertical direction. In a typical TTL cirrus, the heating that results from absorption of radiation by ice crystals induces a mesoscale circulation. Advection of ice and water vapor by the radiatively induced circulation leads to the persistence of the cloud and upward advection of the cloudy air. Upward advection of the cloudy air is equivalent to upward transport of water vapor when the air above the cloud is drier than the cloudy air, and downward transport otherwise. In TTL cirrus, microphysical processes also contribute to transport of water vapor in the vertical direction. Ice nucleation and growth, followed by sedimentation and sublimation, always lead to downward transport of water vapor. The magnitude of the downward transport by microphysical processes increases with the relative humidity of the air surrounding the cloud. Moisture in the surrounding environment is important because there is continuous interactions between the cloudy and environmental air throughout the cloud boundary. In our simulations, when the air surrounding the cloud is subsaturated, hence drier than the cloudy air, the magnitude of the downward transport due to microphysical processes is smaller than that of the upward transport due to the radiatively induced advection of water vapor. The net result is upward transport of water vapor, and equivalently hydration of the lower stratosphere. On the other hand, when the surrounding air is supersaturated, hence moister than the cloudy air, microphysical and radiatively induced dynamical processes work in concert to induce downward transport of water vapor, that is dehydration of the lower stratosphere. TTL cirrus processes also depend sensitively on the deposition coefficient of water vapor on ice crystals. The deposition coefficient determines the depositional growth rate of ice crystals, hence microphysical and radiative properties of the cloud. In our simulations, larger values of the deposition coefficient correspond to less ice crystals nucleated during homogeneous freezing, larger ice crystal sizes, faster ice sedimentation, smaller radiative heating rate and weaker dynamics. These results indicate that detailed observations of the relative humidity in the vicinity of TTL cirrus and accurate laboratory measurements of the deposition coefficient are necessary to quantify the impact of TTL cirrus in the dehydration of the stratosphere. This research highlights the complex role of microphysical, radiative and dynamical processes in the transport of water vapor within TTL cirrus. It shows that under certain realistic conditions, TTL cirrus may lead to upward transport of water vapor, which results in moistening of the lower stratosphere. Thus it is not accurate to always associate TTL cirrus with stratospheric dehydration.
Author: Tra Phuong Dinh
Publisher:
ISBN:
Category : Cirrus clouds
Languages : en
Pages : 73
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Book Description
Simulations of tropical-tropopause-layer (TTL) cirrus under the influence of a large-scale equatorial Kelvin wave have been performed in two dimensions. These simulations show that, even under the influence of the large-scale wave, radiatively induced dynamics in TTL cirrus plays an important role in the transport of water vapor in the vertical direction. In a typical TTL cirrus, the heating that results from absorption of radiation by ice crystals induces a mesoscale circulation. Advection of ice and water vapor by the radiatively induced circulation leads to the persistence of the cloud and upward advection of the cloudy air. Upward advection of the cloudy air is equivalent to upward transport of water vapor when the air above the cloud is drier than the cloudy air, and downward transport otherwise. In TTL cirrus, microphysical processes also contribute to transport of water vapor in the vertical direction. Ice nucleation and growth, followed by sedimentation and sublimation, always lead to downward transport of water vapor. The magnitude of the downward transport by microphysical processes increases with the relative humidity of the air surrounding the cloud. Moisture in the surrounding environment is important because there is continuous interactions between the cloudy and environmental air throughout the cloud boundary. In our simulations, when the air surrounding the cloud is subsaturated, hence drier than the cloudy air, the magnitude of the downward transport due to microphysical processes is smaller than that of the upward transport due to the radiatively induced advection of water vapor. The net result is upward transport of water vapor, and equivalently hydration of the lower stratosphere. On the other hand, when the surrounding air is supersaturated, hence moister than the cloudy air, microphysical and radiatively induced dynamical processes work in concert to induce downward transport of water vapor, that is dehydration of the lower stratosphere. TTL cirrus processes also depend sensitively on the deposition coefficient of water vapor on ice crystals. The deposition coefficient determines the depositional growth rate of ice crystals, hence microphysical and radiative properties of the cloud. In our simulations, larger values of the deposition coefficient correspond to less ice crystals nucleated during homogeneous freezing, larger ice crystal sizes, faster ice sedimentation, smaller radiative heating rate and weaker dynamics. These results indicate that detailed observations of the relative humidity in the vicinity of TTL cirrus and accurate laboratory measurements of the deposition coefficient are necessary to quantify the impact of TTL cirrus in the dehydration of the stratosphere. This research highlights the complex role of microphysical, radiative and dynamical processes in the transport of water vapor within TTL cirrus. It shows that under certain realistic conditions, TTL cirrus may lead to upward transport of water vapor, which results in moistening of the lower stratosphere. Thus it is not accurate to always associate TTL cirrus with stratospheric dehydration.
Author: Tao Wang
Publisher:
ISBN:
Category :
Languages : en
Pages :
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Book Description
Two mechanisms appear to be primarily responsible for the formation of cirrus clouds in Tropical Tropopause Layer (TTL): detrainment from deep convective anvils and in situ initiation. Here we propose to identify TTL cirrus clouds by analyzing water content measurements from the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO) and Aura Microwave Limb Sounder (MLS). Using ice water content (IWC) and water vapor (H2O) abundances we identify TTL cirrus clouds that contain too much ice to have been formed in situ -- and therefore must be of convective origin. We use two methods to infer amounts of water vapor available for in situ formation. Clouds with IWC greater than this threshold are categorized as being of convective origin; clouds with IWC below the threshold are ambiguous -- they could either form from in situ or still be of convective origin. Applying the thresholds from December 2008 to November 2009, we found that at least 19.2% of tropical cirrus were definitively of convective origin at the tropopause (375 K) during boreal winter. At each level, we found three maxima in the occurrence of convective cirrus: western Pacific, equatorial Africa, and South America. Averaged over the entire tropics (30oS to 30oN), we found convective cirrus occurs more frequently in boreal winter and less frequently in boreal summer, basically following the a decreasing trend from DJF, MAM, SON, to JJA. During boreal summer, we found that only 4.6% of tropical cirrus come from convection. Sensitivity tests show that the thresholds derived at 390 K have the largest uncertainty. At lower levels, especially 375 K, our thresholds are robust.
Author: Kai-Wei Chang
Publisher:
ISBN:
Category : Stratospheric circulation
Languages : en
Pages : 0
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Book Description
As a gateway of troposphere-to-stratosphere transport, the tropical tropopause layer (TTL) plays a key role in determining the concentration and distribution of water vapor in the upper troposphere and lower stratosphere (UTLS). This dissertation presents three studies on the dynamical and radiative processes that influence the TTL and also the Brewer-Dobson circulation (BDC) in the global UTLS. Water vapor in the tropical lower stratosphere is strongly correlated with TTL temperatures, which are closely associated with latent heating (LH) in tropical convection. The first study examines the role of latent heating (LH) vertical distribution in TTL cooling and upper-tropospheric warming associated with equatorial wave responses. Using cross-spectral analysis on time series of LH and UTLS temperature, we show that heating above 6 km was found to have the highest coherence with the equatorial wave cooling and warming pattern in the mean temperature profile. We distinguish the effects of convective and stratiform LH, whose heating altitudes differ. Stratiform LH exhibits higher coherence with temperature throughout the UTLS, especially in the equatorial Rossby wave response as seen in the cross-spectral analysis. Highest coherences occur mostly at time scales of the Madden-Julian Oscillation (MJO), suggesting the importance of MJO convection in TTL cooling and subsequent dehydration processes. The second study explores the relationship of TTL cirrus clouds to gravity and Kelvin waves. Motivated by the recent interest in understanding how the vertical gradient of temperature anomalies (dT'/dz) from waves influence clouds, we collocate lidar observations of TTL clouds and wave temperature anomalies from radio occultation to understand how cloud occurrence relates to wave anomalies. Throughout the TTL, 57% of clouds were found in the wave phases where both the temperature anomaly (T') and dT'/dz were negative. In contrast, 24% of clouds were in the phase of negative T' but positive dT'/dz, suggesting that regions of negative dT'/dz significantly promote the formation and/or maintenance of clouds. We show that larger (smaller) values T' are associated with a lower (higher) probability of cloud occurrence, demonstrating connection of wave amplitude to TTL cloud formation. The BDC is a balance between wave-mean-flow interaction and radiative heating rates in the middle atmosphere. Since clouds modulate the amount of upwelling radiation, they can also influence the radiative heating in the UTLS. Using the CloudSat/CALIPSO 2B-FLXHR-LIDAR data set and the MERRA-2 reanalysis, the final study evaluates cloud effects on the BDC by comparing the mass circulation diagnosed from clear-sky and all-sky radiative heating rates. Cloud effects are strongest during boreal winter when the vertical and meridional components of the BDC below 80 hPa exhibit differences on the order of 0.1 mm/s and 10 cm/s, respectively. These magnitudes are comparable to the BDC itself, illustrating that cloud effects on radiative heating rates can have a significant influence on the strength of tropical upwelling and meridional mixing. TTL cirrus, which tends to impose weak heating in the TTL, were found to enhance the tropical upwelling and also the poleward transport, while the aggregate effect of all other cloud types was to weaken them instead.
Author: Helmut K. Weickmann
Publisher:
ISBN:
Category : Convection (Meteorology)
Languages : en
Pages : 44
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Book Description
Author: Paul Edward Neevel
Publisher:
ISBN:
Category : Clouds
Languages : en
Pages : 78
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Book Description
Author: Jacqueline Nugent
Publisher:
ISBN:
Category :
Languages : en
Pages : 56
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Book Description
Pervasive cirrus clouds in the upper troposphere and tropical tropopause layer (TTL) in- fluence the climate by altering the top-of-atmosphere radiation balance and stratospheric water vapor budget. These cirrus are often associated with deep convection, which global climate models must parameterize and struggle to accurately simulate. By comparing high- resolution global models from the DYAMOND intercomparison that explicitly simulate deep convection to satellite observations, we assess how well these models simulate deep convec- tion, convectively generated cirrus, and deep convective injection of water into the TTL over representative tropical land and ocean regions. The DYAMOND models simulate deep convective precipitation, organization, and cloud structure fairly well over land and ocean regions, but with clear inter-model differences. All models produce frequent overshooting convection whose strongest updrafts humidify the TTL and are its main source of frozen water. Inter-model differences in cloud properties and convective injection exceed differences between land and ocean regions in each model. We argue that global storm-resolving mod- els can better represent tropical cirrus and deep convection in present and future climates than coarser-resolution climate models. To realize this potential, they must use available observations to perfect their ice microphysics and dynamical flow solvers.
Author: David K. Lynch
Publisher: Oxford University Press
ISBN: 0195351398
Category : Science
Languages : en
Pages : 499
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Book Description
Cirrus clouds are high, thin, tropospheric clouds composed predominately of ice. In the last ten years, considerable work has shown that cirrus is widespread--more common than previously believed--and has a significant impact on climate and global change. As the next generation weather satellites are being designed, the impact of cirrus on remote sensing and the global energy budget must be recognized and accommodated. This book, the first to be devoted entirely to cirrus clouds, captures the state of knowledge of cirrus and serves as a practical handbook as well. Each chapter is based on an invited review talk presented at Cirrus, a meeting hosted by the Optical Society of America and co-sponsored by the American Geophysical Union and the American Meteorological Society. All aspects of cirrus clouds are covered, an approach that reaches into diverse fields. Topics include: the definition of cirrus, cirrus climatologies, nucleation, evolution and dissipation, mixed-phase thermodynamics, crystallinity, orientation mechanisms, dynamics, scattering, radiative transfer, in situ sampling, processes that produce or influence cirrus (and vice versa), contrails, and the influence of cirrus on climate.
Author: Felix Plöger
Publisher: Forschungszentrum Jülich
ISBN: 3893366954
Category :
Languages : en
Pages : 129
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Book Description
Author: Mekonnen Gebremichael
Publisher: Springer Science & Business Media
ISBN: 904812915X
Category : Science
Languages : en
Pages : 327
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Book Description
With contributions from a panel of researchers from a wide range of fields, the chapters of this book focus on evaluating the potential, utility and application of high resolution satellite precipitation products in relation to surface hydrology.
Author: Rick Russotto
Publisher:
ISBN:
Category :
Languages : en
Pages : 100
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Book Description
Thin cirrus clouds in the tropical tropopause layer (TTL) play potentially important roles in Earth's radiation budget and in the transport of water into the stratosphere. Radiative heating of these clouds results in mesoscale circulations that maintain them against sedimentation and redistribute water vapor. In this study, the System for Atmospheric Modeling (SAM) cloud-resolving model is modified in order to calculate the fall speeds, growth rates, and radiative absorption coefficients of non-spherical ice crystals. This extended model is used in simulations that aim to constrain the effects of ice crystal shape on the time evolution of thin cirrus clouds and to identify the physical processes responsible. Model runs assuming spheroidal crystals result in a higher center of cloud ice mass than in the control, spherical case, which is roughly 60% due to a reduction in fall speeds and 40% due to stronger updrafts caused by stronger radiative heating. Other effects of ice crystal shape on the cloud evolution include faster growth and sublimation in supersaturated and subsaturated environments, respectively, and local temperature increases caused by diabatic heating. Effects of ice crystal shape on the total and mean ice crystal masses are within about 10% but do not appear to be entirely negligible. Comparisons of modeled ice crystal size distributions with recent airborne observations of TTL cirrus show that incorporating non-spherical shape has the potential to bring the model closer to observations. It is hoped that this work will eventually lead towards a more realistic physical representation of thin tropical cirrus in global climate models.
