Description and evaluation of tropospheric chemistry and aerosols in the Community Earth System Model (CESM1.2)

The Community Atmosphere Model (CAM), version 5, is now coupled to extensive tropospheric and stratospheric chemistry, called CAM5-chem, and is available in addition to CAM4-chem in the Community Earth System Model (CESM) version 1.2. The main focus of this paper is to compare the performance of configurations with internally derived "free running" (FR) meteorology and "specified dynamics" (SD) against observations from surface, aircraft, and satellite, as well as understand the origin of the identified differences. We focus on the representation of aerosols and chemistry. All model configurations reproduce tropospheric ozone for most regions based on in situ and satellite observations. However, shortcomings exist in the representation of ozone precursors and aerosols. Tropospheric ozone in all model configurations agrees for the most part with ozonesondes and satellite observations in the tropics and the Northern Hemisphere within the variability of the observations. Southern hemispheric tropospheric ozone is consistently underestimated by up to 25%. Differences in convection and stratosphere to troposphere exchange processes are mostly responsible for differences in ozone in the different model configurations. Carbon monoxide (CO) and other volatile organic compounds are largely underestimated in Northern Hemisphere mid-latitudes based on satellite and aircraft observations. Nitrogen oxides (NOx) are biased low in the free tropical troposphere, whereas peroxyacetyl nitrate (PAN) is overestimated in particular in high northern latitudes. The present-day methane lifetime estimates are compared among the different model configurations. These range between 7.8 years in the SD configuration of CAM5-chem and 8.8 years in the FR configuration of CAM4-chem and are therefore underestimated compared to observational estimations. We find that differences in tropospheric aerosol surface area between CAM4 and CAM5 play an important role in controlling the burden of the tropical tropospheric hydroxyl radical (OH), which causes differences in tropical methane lifetime of about half a year between CAM4-chem and CAM5-chem. In addition, different distributions of NOx from lightning explain about half of the difference between SD and FR model versions in both CAM4-chem and CAM5-chem. Remaining differences in the tropical OH burden are due to enhanced tropical ozone burden in SD configurations compared to the FR versions, which are not only caused by differences in chemical production or loss but also by transport and mixing. For future studies, we recommend the use of CAM5-chem configurations, due to improved aerosol description and inclusion of aerosol–cloud interactions. However, smaller tropospheric surface area density in the current version of CAM5-chem compared to CAM4-chem results in larger oxidizing capacity in the troposphere and therefore a shorter methane lifetime

Exploring the Bimodal Solar System via Sample Return from the Main Asteroid Belt: The Case for Revisiting Ceres

Abstract: Sample return from a main-belt asteroid has not yet been attempted, but appears technologically feasible. While the cost implications are significant, the scientific case for such a mission appears overwhelming. As suggested by the “Grand Tack” model, the structure of the main belt was likely forged during the earliest stages of Solar System evolution in response to migration of the giant planets. Returning samples from the main belt has the potential to test such planet migration models and the related geochemical and isotopic concept of a bimodal Solar System. Isotopic studies demonstrate distinct compositional differences between samples believed to be derived from the outer Solar System (CC or carbonaceous chondrite group) and those that are thought to be derived from the inner Solar System (NC or non-carbonaceous group). These two groups are separated on relevant isotopic variation diagrams by a clear compositional gap. The interface between these two regions appears to be broadly coincident with the present location of the asteroid belt, which contains material derived from both groups. The Hayabusa mission to near-Earth asteroid (NEA) (25143) Itokawa has shown what can be learned from a sample-return mission to an asteroid, even with a very small amount of sample. One scenario for main-belt sample return involves a spacecraft launching a projectile that strikes an object and flying through the debris cloud, which would potentially allow multiple bodies to be sampled if a number of projectiles are used on different asteroids. Another scenario is the more traditional method of landing on an asteroid to obtain the sample. A significant range of main-belt asteroids are available as targets for a sample-return mission and such a mission would represent a first step in mineralogically and isotopically mapping the asteroid belt. We argue that a sample-return mission to the asteroid belt does not necessarily have to return material from both the NC and CC groups to viably test the bimodal Solar System paradigm, as material from the NC group is already abundantly available for study. Instead, there is overwhelming evidence that we have a very incomplete suite of CC-related samples. Based on our analysis, we advocate a dedicated sample-return mission to the dwarf planet (1) Ceres as the best means of further exploring inherent Solar System variation. Ceres is an ice-rich world that may be a displaced trans-Neptunian object. We almost certainly do not have any meteorites that closely resemble material that would be brought back from Ceres. The rich heritage of data acquired by the Dawn mission makes a sample-return mission from Ceres logistically feasible at a realistic cost. No other potential main-belt target is capable of providing as much insight into the early Solar System as Ceres. Such a mission should be given the highest priority by the international scientific community

Comparação entre dois fios de sutura não absorvíveis na anastomose traqueal término-terminal em cães Comparison of two nonabsorbable suture materials in the end-to-end tracheal anastomosis in dogs

Doze cães sem raça definida, com idade variando entre 1 e 6 anos e peso de 6 a 20kg, foram submetidos a ressecção traqueal e anastomose término-terminal, na qual foram testados os fios poliéster trançado não capilar e náilon monofilamento. Seis animais, cada três com um mesmo tipo de fio de sutura, sofreram a excisão equivalente a três anéis traqueais. Com 15 dias foi executada uma nova intervenção onde se ressecou o equivalente a mais seis anéis, perfazendo um total de nove. Ao final de outros 15 dias foram sacrificados. Os outros seis animais, cada três com um mesmo tipo de fio, foram submetidos à excisão equivalente a três anéis traqueais e mantidos por 43 dias. As traquéias foram avaliadas por exames clínicos, radiográficos, macroscópicos e histopatológicos. O fio de náilon monofilamento apresentou menos reação tecidual do que o poliéster trançado não capilar, promoveu uma anastomose segura e com menor chance de formação de granuloma.<br>Twelve mongrel dogs, with age between 1 and 6 years old and weight between 12 and 40 pounds, were submitted to tracheal resection and end-to-end anastomosis in which were tested braided polyester no capillary and monofilament nylon materiais. Six animais, every threeones with a same type of suture material, suffered the excision equivalent to three tracheal rings. A new intervention was performed with fifteen days, in which the equivalent of more six tracheal rings were removed, completing the total of nine. At the end of more fifteen days they were sacrificed. The other six animals, every three with a same type of suture material, were submitted to the excision equivalent to three tracheal rings and maintained for 43 days. The tracheal anastomosis were evaluated to clinic, radiographic, macroscopic and histopathologic studies. The monofilament nylon material exhibited less reaction than polyester and promoted a secure anastomosis with less risk of granuloma formation

LOCAL REGIMES: Does Globalization Challenge the "Growth Machine"&quest;

This article explores the possible impacts that globalization might have upon the nature of local governments and the economic development policies that they adopt. We begin by outlining the theory of how "corporate regimes" dominate most urban centers, why they implement skewed economic development policies, and why globalization appears to be exacerbating these problems. Research on state-and-local economic development outside urban centers indicates that several types of business development exist and that they differ significantly in their implications for improving conditions in a community. This suggests that other types of corporate regimes are possible. The logic of globalization points toward the need to establish more progressive corporate regimes willing to implement some of the reforms advocated by critics of the "growth machine." Copyright 2001 by The Policy Studies Organization.