High Velocity Cloud Interactions with Their Ambient Environment


Book Description

High velocity clouds (HVCs) are collections of gas around the Milky Way galaxy and other galaxies with masses ranging from tens of thousands of solar masses to millions of solar masses. These cool clouds can potentially supply new cool material to the disks of galaxies. Many unanswered questions exist about HVCs; e.g. "How do HVCs form?", "How long can HVCs survive while interacting with the hot ambient material?", and "How do HVCs affect, and how are they affected by, our Galaxy?" Using detailed multi-dimensional numerical simulations, this study focuses on how HVCs interact with their ambient environments and how these interactions affect the cloud's metal concentration, condensation and evaporation rates, and morphology. Using the results of these simulations this study suggests methods to determine the origins of HVCs based on observed metal concentrations, and how initial parameter space affects the condensation of ambient material onto HVCs.




High-Velocity Clouds


Book Description

On the occasion of the retirement of Ulrich Schwarz, a symposium was held in Groningen in May of 1996, celebrating his contributions to the study of the int- stellar medium, including his work on the high-velocity clouds. The coming together of many specialists in the latter ?eld prompted the idea of compiling a book c- taining their contributions, and summarizing the status of our understanding of the high-velocity cloud phenomenon. This seemed especially worthwhile at the time, since many exciting developments were taking place. After the discovery of some H i clouds with high velocities, about 40 years ago, the subject had been dominated by 21-cm observations of H i emission. Starting in the mid-1980s much progress was being made because of the availability of new instruments, such as large ground-based optical telescopes and UV observatories in space. The connections between the work on high-velocity clouds and other studies of the properties of the (hot) interstellar medium also became clearer.




High-Velocity Clouds


Book Description

On the occasion of the retirement of Ulrich Schwarz, a symposium was held in Groningen in May of 1996, celebrating his contributions to the study of the int- stellar medium, including his work on the high-velocity clouds. The coming together of many specialists in the latter ?eld prompted the idea of compiling a book c- taining their contributions, and summarizing the status of our understanding of the high-velocity cloud phenomenon. This seemed especially worthwhile at the time, since many exciting developments were taking place. After the discovery of some H i clouds with high velocities, about 40 years ago, the subject had been dominated by 21-cm observations of H i emission. Starting in the mid-1980s much progress was being made because of the availability of new instruments, such as large ground-based optical telescopes and UV observatories in space. The connections between the work on high-velocity clouds and other studies of the properties of the (hot) interstellar medium also became clearer.







Ambient Assisted Living and Enhanced Living Environments


Book Description

Ambient Assisted Living and Enhanced Living Environments: Principles, Technologies and Control separates the theoretical concepts concerning the design of such systems from their real-world implementations. For each important topic, the book bridges theory and practice, introducing the instruments needed by professionals in their activities. To this aim, topics are presented in a logical sequence, with the introduction of each topic motivated by the need to respond to claims and requirements from a wide range of AAL/ELE applications. The advantages and limitations of each model or technology are presented through concrete case studies for AAL/ELE systems. The book also presents up-to-date technological solutions to the main aspects regarding AAL/ELE systems and applications, a highly dynamic scientific domain that has gained much interest in the world of IT in the last decade. In addition, readers will find discussions on recent AAL/ELE technologies that were designed to solve some of the thorniest business problems that affect applications in areas such as health and medical supply, smart city and smart housing, Big Data and Internet of Things, and many more. - Introduces readers to technologies supporting the development of Ambient Assisted Living applications - Explains state-of-the-art technological solutions for the main issues regarding AAL and Enhanced Living Environments - Reports the development process of scientific and commercial applications and platforms that support AAL and ELE - Identifies the advanced solutions in the context of Enhanced Living Environments




High-velocity Clouds


Book Description







On the Interactions Between Clouds and Atmospheric Circulation in the Tropics and Midlatitudes


Book Description

Cloud radiative feedbacks are the largest source of uncertainty in climate projections. It has been shown that narrowing this uncertainty will require a better understanding of the two-way interactions between clouds and the atmospheric circulation. Understanding cloud-circulation interactions and constraining cloud-climate feedbacks are therefore important and urgent goals in climate research. These topics are investigated in this thesis. In Part A, satellite observations are used to study the interactions between clouds and atmospheric circulation over the Southern Ocean. Atmospheric motions modify the boundary-layer stratification, inversion strength, and large-scale vertical motion, and in doing so, modulate clouds. Surface heat fluxes also significantly modulate shallow clouds. The ability of climate models to simulate these processes is investigated. Climate models consistently struggle to accurately represent shallow clouds in subfreezing environments. The implications of these model biases for uncertainty in cloud-climate feedbacks is discussed. In Part B, cloud-circulation interactions are investigated over the warm and convective tropical oceans. In these regions, the average shortwave and longwave cloud radiative effects are individually large but nearly cancel at the top of the atmosphere. It has been hypothesized that this cancellation is caused by two-way interactions between clouds, atmospheric circulation, and sea surface temperature (SST). This hypothesis is investigated using a variety of satellite observations and climate model simulations. First, observations from polar-orbiting satellites are used to investigate the relationships between large-scale circulation and cloud properties. Next, a cloud-tracking algorithm is applied to geostationary satellite observations and is used to study the evolution of clouds, the ambient environment, and the underlying SST over the life cycle of convective storms. Finally, a climate model in global radiative-convective equilibrium configuration is used to investigate the impact of cloud-circulation-SST interactions on tropical climate. All three studies are consistent with the hypothesis that cloud-circulation-SST interactions cause the close balance in cloud radiative effects over warm tropical oceans. It is hypothesized that this mechanism could constrain cloud-climate feedbacks in the warm and convective tropics.