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C. P. Sajan B. Basavalingu S. Ananda K. Byrappa 《Journal of the Geological Society of India》2011,77(1):82-88
The photocatalytic degradation of Indigo Caramine dye using commercial TiO2 and fine grained natural rutile has been carried out. The commercial TiO2 and natural rutile were characterized using powder X- ray diffraction (XRD) and Fourier transformed infra red spectroscopy
(FTIR). The study on the photodegradation of Indigo Caramine dye using commercial TiO2 and natural rutile were investigated both under Solar and UV irradiation. The degradation of Indigo Caramine dye was checked
by the following parameters like Chemical Oxygen Demand (COD), %T, irradiation time and duration. In both cases using commercial
TiO2 and natural rutile, the COD of the dye solution was reduced from 288 mg/L to less than 20 mg/L, and similarly the %T was
increased from 76% to 97% and the percentage decomposition upto 97% within the irradiation duration of 3.5 hrs. The preliminary
results obtained on the photodegradation of Indigo Caramine dye are highly encouraging and further work is being carried out
for the use of the natural rutile or anatase sources for the other organic decomposition and treatment of industrial effluents. 相似文献
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We present multifrequency radio continuum as well as H i observations of the superwind galaxy NGC 1482, with both the Giant Metrewave Radio Telescope (GMRT) and the Very Large Array (VLA). This galaxy has a remarkable hourglass-shaped optical emission-line outflow as well as bipolar soft X-ray bubbles on opposite sides of the galactic disc. The low-frequency, lower-resolution radio observations show a smooth structure. From the non-thermal emission, we estimate the available energy in supernovae, and examine whether this would be adequate to drive the observed superwind outflow. The high-frequency, high-resolution radio image of the central starburst region located at the base of the superwind bi-cone shows one prominent peak and more extended emission with substructure. This image has been compared with the infrared, optical red continuum, Hα, and soft and hard X-ray images from Chandra to understand the nature and relationship of the various features seen at different wavelengths. The peak of the infrared emission is the only feature that is coincident with the prominent radio peak, and possibly defines the centre of the galaxy.
The H i observations with the GMRT show two blobs of emission on opposite sides of the central region. These are rotating about the centre of the galaxy and are located at ∼2.4 kpc from it. In addition, these observations also reveal a multicomponent H i absorption profile against the central region of the radio source, with a total width of ∼250 km s−1 . The extreme blue- and redshifted absorption components are at 1688 and 1942 km s−1 , respectively, while the peak absorption is at 1836 km s−1 . This is consistent with the heliocentric systemic velocity of 1850 ± 20 km s−1 , estimated from a variety of observations. We discuss possible implications of these results. 相似文献
The H i observations with the GMRT show two blobs of emission on opposite sides of the central region. These are rotating about the centre of the galaxy and are located at ∼2.4 kpc from it. In addition, these observations also reveal a multicomponent H i absorption profile against the central region of the radio source, with a total width of ∼250 km s
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Heliana Teixeira Ángel Borja J. Ananda Ranasinghe Daniel M. Dauer Steven Degraer Antoine Grémare Roberto J. Llansó João C. Marques Anna Occhipinti-Ambrogi Rafael Sardá Ronald G. Velarde 《Marine pollution bulletin》2010,60(4):589-600
Benthic indices are typically developed independently by habitat, making their incorporation into large geographic scale assessments potentially problematic because of scaling inequities. A potential solution is to establish common scaling using expert best professional judgment (BPJ). To test if experts from different geographies agree on condition assessment, sixteen experts from four regions in USA and Europe were provided species-abundance data for twelve sites per region. They ranked samples from best to worst condition and classified samples into four condition (quality) categories. Site rankings were highly correlated among experts, regardless of whether they were assessing samples from their home region. There was also good agreement on condition category, though agreement was better for samples at extremes of the disturbance gradient. The absence of regional bias suggests that expert judgment is a viable means for establishing a uniform scale to calibrate indices consistently across geographic regions. 相似文献
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J. Ananda Ranasinghe Kenneth C. Schiff Tim K. Mikel Ronald G. Velarde 《Marine pollution bulletin》2010,60(6):827-833
To assess benthic macrofaunal community condition in Southern California, 838 sites were sampled using spatially random designs in 1994, 1998, or 2003. Benthic community condition was assessed on a four-category scale and the area in each category estimated. Overall, benthic macrofauna in Southern California were in good condition during 2003, with 98% of the area in reference condition or deviating only marginally. There was no evidence of disturbance near Channel Islands or small wastewater discharges, and virtually none on the mainland shelf. In contrast, bay and estuary macrofaunal communities were more frequently disturbed with nearly 13% of the area supporting disturbed benthos. The condition of the mainland shelf did not change substantially over the 9-year period, with 1.6-2.8% of the area in poor benthic condition. Southern California benthic condition evaluations may be improved by extending the depth and salinity ranges of assessment tools, and improving trend detection methods. 相似文献
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Ananda Pascual Arancha Lana Charles Troupin Simón Ruiz Yannice Faugère Romain Escudier 《Marine Geodesy》2015,38(3):260-276
We present an initial assessment of SARAL/AltiKa data in the coastal band. The study focuses on the Ibiza Channel where the north-south water exchanges play a key role in controlling the circulation variability in the western Mediterranean. In this area, the track 16 of SARAL/AltiKa intercepts the domain covered by a coastal high-frequency (HF) radar system, which provides surface currents with a range up to 60 km. We evaluate the performance of the SARAL/AltiKa Ssalto/Duacs delayed-time along-track products compared to the HF radar surface velocity fields. SARAL/AltiKa data are retrieved at a distance of only 7 km from the coast, putting in evidence the emerging capabilities of the new altimeter. The derived velocities resolved the general features of the seasonal mesoscale variability with reasonable agreement with HF radar fields (significant correlations of 0.54). However, some discrepancies appear, which might be caused by instrumental hardware radar errors, ageostrophic velocities as well as inaccurate corrections and editing in the altimeter data. Root mean square (rms) differences between the estimated SARAL/AltiKa and the HF radar velocities are about 13 cm/s. These results are consistent with recent studies in other parts of the ocean applying similar approaches to Topex/Poseidon and Jason-1 missions and using coastal altimeter corrections. 相似文献