scholarly journals Determination of photochemically available iron in ambient aerosols

1996 ◽  
Vol 101 (D9) ◽  
pp. 14441-14449 ◽  
Author(s):  
Ronald L. Siefert ◽  
Samuel M. Webb ◽  
Michael R. Hoffmann
Keyword(s):  
2010 ◽  
Vol 24 (11) ◽  
pp. 1625-1628 ◽  
Author(s):  
Li Li ◽  
Shihuai Deng ◽  
Wu Wang ◽  
Huaijian Li ◽  
Xiaohong Zhang ◽  
...  

2020 ◽  
Author(s):  
Guo Li ◽  
Hang Su ◽  
Nan Ma ◽  
Guangjie Zheng ◽  
Uwe Kuhn ◽  
...  

<p>Direct measurement of the acidity (pH) of ambient aerosol particles/droplets has long been a challenge for atmospheric scientists.  A novel and facile method was introduced recently by Craig et al. (2018), where the pH of size-resolved aerosol droplets was directly measured by two types of pH-indicator papers (pH ranges: 0 – 2.5 and 2.5 – 4.5) combined with RGB-based colorimetric analyses using a model of G-B (G minus B) versus pH<sup>2</sup>.  Given the wide pH range of ambient aerosols, we optimize the RGB-based colorimetric analysis on pH papers with a wider detection range (pH ~ 0 to 6).  Here, we propose a new model to establish the linear relationship between RGB values and pH: pH<sub>predict</sub> = a×R<sub>normal</sub> + b×G<sub>normal</sub> + c×B<sub>normal</sub>.  This model shows a wider applicability and higher accuracy than those in previous studies, and is thus recommended in future RGB-based colorimetric analyses on pH papers.  Moreover, we identify one type of pH paper (Hydrion<sup>®</sup> Brilliant pH dip stiks, Lot Nr. 3110, Sigma-Aldrich) that is more applicable for ambient aerosols in terms of its wide pH detection range (0 to 6) and strong anti-interference capacity.  The determined minimum sample mass (~ 180 µg) highlights its potential to predict aerosol pH with a high time resolution (e.g., ≤ 1 hour).  We further show that the routinely adopted way of using pH color charts to predict aerosol pH may be biased by the mismatch between the standard colors on the color charts and the real colors of investigated samples.  Thus, instead of using the producer-provided color chart, we suggest an in-situ calibration of pH papers with standard pH buffers.</p><p>Reference:</p><p>Craig, et al., Direct determination of aerosol pH: Size-resolved measurements of submicrometer and supermicrometer aqueous particles. Analytical Chemistry, 90 (19), 11232-11239, 2018.</p><p>Cheng, et al., Reactive nitrogen chemistry in aerosol water as a source of sulfate during haze events in China. Science Advances, 2 (12), e1601530, 10.1126/sciadv.1601530, 2016.</p><p>Zheng, et al., Exploring the severe winter haze in Beijing: The impact of synoptic weather, regional transport and heterogeneous reactions. Atmospheric Chemistry and Physics, 15, 2969-2983, 2015.</p><p>Li, et al., Multifactor colorimetric analysis on pH-indicator papers: an optimized approach for direct determination of ambient aerosol pH, Atmos. Meas. Tech. Discuss., https://doi.org/10.5194/amt-2019-394, in review, 2019.</p>


1996 ◽  
Vol 110 (4) ◽  
pp. 364-370 ◽  
Author(s):  
George F. Schäppi ◽  
Christian Monn ◽  
Brunello Wüthrich ◽  
Hans-Urs Wanner

1994 ◽  
Vol 38 ◽  
pp. 91-97
Author(s):  
B. L. Davis ◽  
H. Chen

Determination of the species of compounds present in ambient aerosols has received increasing interest in recent years (Harrison and Pio, 1983; Davis, 1984; Davis and Maughan, 1984; Harrison and Sturges, 1984; Sturges et al, 1989; Possanzini et al, 1992; Havliek et al., 1993), but the U.S. Environmental Protection Agency's conversion to the PM10 standard in 1987 has made quantitative analysis of fine particle aerosols more difficult because of the much smaller deposited mass on these filters, as well as the increased proportion of carbon-bearing material naturally present in the smaller diameter portion of the atmospheric aerosol size distribution. Under the old TSP (Total Suspended Particulate) collection protocol, filter loads of 400-2000 μg cm-2 of 10-20 μm mean diameter particles, corresponding to 24-hour collections at ambient concentrations of 100 to 500 μg m-3 at 40 CFM flow rates, resulted in excellent diffraction patterns scanned directly from filter segments.


2020 ◽  
Vol 240 ◽  
pp. 117800
Author(s):  
Gang Zhao ◽  
Fei Li ◽  
Chunsheng Zhao

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


1999 ◽  
Vol 190 ◽  
pp. 549-554
Author(s):  
Nino Panagia

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.


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