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91.
Rodrigo Augusto Bellezoni Cristiano Kenji Iwai Vagner Roberto Elis Wanderley da Silva Paganini Jorge Hamada 《Environmental Earth Sciences》2014,71(5):2429-2439
In Brazil, the large quantities of solid waste produced are out of step with public policies, technological developments, and government budgets for the division. In small municipalities, the common lack of technological knowledge and financial conditions for suitable waste disposal has resulted in a large number of illegal dumps. Therefore, small sanitary landfill facilities are working with simplified operations focusing on cost reduction and meeting the economic and technological standards of the city without endangering the environment or public health. Currently, this activity is regulated at a federal level although there is some uncertainty regarding the risk of soil and aquifer contamination as theses facilities do not employ liners. Thus, this work evaluates a small landfill to identify changes in soil and groundwater using geotechnical parameters, monitoring wells, and geophysical tests performed by electrical profiling. It is verified that based on current conditions, no contaminants have migrated via underground water aquifers, and overall no significant changes have occurred in the soil. It is concluded that, despite its simplicity, the method investigated is a viable alternative for the final disposal of municipal solid waste from small cities, especially in developing countries. 相似文献
92.
Blooms of cyanobacteria are responsible for many problems in freshwater ecosystems. The massive growth of these microorganisms may limit the utilization of freshwater for human requirements since, apart from other problems, the production of toxic substances has been found to occur frequently during blooming periods. Ecologically, cyanobacterial blooms can modify dramatically the ecosystem through their low edibility within the food web and the huge primary production. Thus, saprobic processes are stimulated and the characteristics related to anaerobic conditions are also more extreme.Cyanobacterial blooms are many times explained as the consequence of the eutrophication of waterbodies. However, factors promoting bloom formation and ecological succession of cyanobacteria are not well understood yet. 相似文献
93.
The pattern and magnitude of the global ocean overturning circulation is believed to be strongly controlled by the distribution
of diapycnal diffusivity below 1000 m depth. Although wind stress fluctuation is a candidate for the major energy sources
of diapycnal mixing processes, the global distribution of wind-induced diapycnal diffusivity is still uncertain. It has been
believed that internal waves generated by wind stress fluctuations at middle and high latitudes propagate equatorward until
their frequency is twice the local inertial frequency and break down via parametric subharmonic instabilities, causing diapycnal
mixing. In order to check the proposed scenario, we use a vertically two-dimensional primitive equation model to examine the
spatial distribution of “mixing hotspots” caused by wind stress fluctuations. It is shown that most of the wind-induced energy
fed into the ocean interior is dissipated within the top 1000 m depth in the wind-forced area and the energy dissipation rate
at low latitudes is very small. Consequently, the energy supplied to diapycnal mixing processes below 1000 m depth falls short
of the level required to sustain the global ocean overturning circulation. 相似文献
94.
M. Shimojo T. S. Bastian A. S. Hales S. M. White K. Iwai R. E. Hills A. Hirota N. M. Phillips T. Sawada P. Yagoubov G. Siringo S. Asayama M. Sugimoto R. Brajša I. Skokić M. Bárta S. Kim I. de Gregorio-Monsalvo S. A. Corder H. S. Hudson S. Wedemeyer D. E. Gary B. De Pontieu M. Loukitcheva G. D. Fleishman B. Chen A. Kobelski Y. Yan 《Solar physics》2017,292(7):87
Observations of the Sun at millimeter and submillimeter wavelengths offer a unique probe into the structure, dynamics, and heating of the chromosphere; the structure of sunspots; the formation and eruption of prominences and filaments; and energetic phenomena such as jets and flares. High-resolution observations of the Sun at millimeter and submillimeter wavelengths are challenging due to the intense, extended, low-contrast, and dynamic nature of emission from the quiet Sun, and the extremely intense and variable nature of emissions associated with energetic phenomena. The Atacama Large Millimeter/submillimeter Array (ALMA) was designed with solar observations in mind. The requirements for solar observations are significantly different from observations of sidereal sources and special measures are necessary to successfully carry out this type of observations. We describe the commissioning efforts that enable the use of two frequency bands, the 3-mm band (Band 3) and the 1.25-mm band (Band 6), for continuum interferometric-imaging observations of the Sun with ALMA. Examples of high-resolution synthesized images obtained using the newly commissioned modes during the solar-commissioning campaign held in December 2015 are presented. Although only 30 of the eventual 66 ALMA antennas were used for the campaign, the solar images synthesized from the ALMA commissioning data reveal new features of the solar atmosphere that demonstrate the potential power of ALMA solar observations. The ongoing expansion of ALMA and solar-commissioning efforts will continue to enable new and unique solar observing capabilities. 相似文献