Abstract (EN):
This work describes the changes in mineralogy and
magnetic parameters of the waste pile materials from burning
and unburned zones in the S. Pedro da Cova, Midões and
Lomba areas of the Douro Coalfield, Portugal. X-ray
diffraction analysis has provided information about the
mineral phases and the reactions that occurred during the
combustion process, and hence been used to identify the
temperatures reached. The unburned coal waste materials
contain quartz, illite, mica (mainly muscovite) and in many
cases pyrophyllite. Some of the burnt coal waste samples have
similar mineralogy to the unburned materials, but some
contain mullite and cristobalite, suggesting that higher
temperatures were involved in the combustion process. Lowfield
magnetic susceptibility (') and isothermal remanent
magnetization (IRM) determinations were used to indicate the
source of the magnetic mineralogy and the waste material
contamination in burning parts of the S. Pedro da Cova and
Lomba piles. In S. Pedro da Cova, the two highest values of '
(1217.60 and 556.22 x10-8 m3/kg) were found in zones where
the temperature was higher than 200°C, and in Lomba the two
highest values (705.84 and 211.67 x10-8 m3/kg) were found
where the temperature was higher than 70°C. These
temperatures were measured with a digital infrared
thermometer when the samples were collected. In unburned
zones ' ranges from 13.58 to 16.62 x10-8 m3/kg. The IRM
values of the S. Pedro da Cova samples show that remanence
saturation was achieved at a magnetic field lower than 300
mT, suggesting the presence of a low-coercivity structure,
magnetite-like phase. However, in the samples from Lomba,
the imparted field was insufficient to achieve remanence
saturation, probably because ‘hard magnetic structures’ are
also present. The ‘Index of Geo-accumulation’ at S. Pedro da
Cova and Lomba shows that the samples represent a strong to
very strong contamination. Here the highest ' occurs where
the combustion temperature was also very high, suggesting
that the burning process was the main cause of the magnetic
enhancement.
Idioma:
Inglês
Tipo (Avaliação Docente):
Científica
Notas:
Comunicação apresentada na conferência "Goldschmidt 2010: Earth, Energy, and the Environment"