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Seasonal and diurnal variations of ultrafine particle concentration in urban Gwangju, Korea: Observation of ultrafine particle events

机译:韩国光州市区超微粒子浓度的季节性和昼夜变化:超微粒子事件的观测

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Ultrafine particle concentration (3-100 nm) was continuously measured in summer (6/7/2006-17/8/2006), fall (1/10/ 2006-31/10/2006), winter (2/2/2007-7/3/2007), and spring (7/4/2007-7/5/2007) in urban Gwangju, Korea. By considering the size range with elevated concentration and hypothesizing the source or formation pathways, we classified ultrafine particle events into: (1) "10-100nm traffic event," (2) "50-100nm residential heating event," and (3) "10-30nm photochemical event." Coincidence of NO_x, CO, O_3, and solar radiation with ultrafine particle concentration was used as an indicator for the traffic, residential heating, and photochemical contributions. We showed that particles due to traffic and residential heating led to enhanced ultrafine particle concentration in winter, while in summer particles formed by photochemical activity led to increased ultrafine particle concentration. The average ultrafine particle number concentrations were 8.8 × 10~3, 7.4 × 10~3, and 7.9 × 10~3cm~(-3) with geometric mean diameters (GMDs) of 25, 48, and 53 nm in the photochemical, traffic, and residential heating events, respectively. Our ultrafine particle concentrations and other gas concentrations (NO_x and CO) were found to be lower than observations in Atlanta and in Fresno, probably due to lower source strength such as traffic and residential heating in current site. We occasionally observed particle growth after formation of particles in the photochemical event with growth rates of 2.2-4.7 nmh~(-1). Morphological and elemental analysis for size-selected ultrafine particles showed that mixtures of sulfate and metals with the presence of semi-transparent part inside the particle were observed in the photochemical event (49 over 200 particles), while in the traffic event agglomerated carbonaceous particles were observed (66 over 130 particles), which were rarely detected in the photochemical event.
机译:在夏季(6/7 / 2006-17 / 8/2006),秋季(1/10 / 2006-31 / 10/2006),冬季(2/2/2007)连续测量超细颗粒浓度(3-100 nm) -7/3/2007)和春季(7/4 / 2007-7 / 5/2007)在韩国光州举行。通过考虑浓度升高的大小范围并假设来源或形成途径,我们将超细颗粒事件分类为:(1)“ 10-100nm交通事件”,(2)“ 50-100nm住宅供暖事件”和(3) “ 10-30nm光化学事件。” NO_x,CO,O_3与太阳辐射与超细颗粒浓度的重合度被用作交通,住宅供暖和光化学贡献的指标。我们发现,由于交通和住宅取暖导致的颗粒在冬季导致超细颗粒浓度增加,而在夏季,由光化学活性形成的颗粒导致超细颗粒浓度增加。在光化学,交通流中,平均超细颗粒数浓度为8.8×10〜3、7.4×10〜3和7.9×10〜3cm〜(-3),几何平均直径(GMD)为25、48和53 nm。 ,以及住宅供暖事件。发现我们的超细颗粒物浓度和其他气体浓度(NO_x和CO)低于亚特兰大和弗雷斯诺的观测值,这可能是由于源强度较低,例如当前站点的交通和居民取暖。我们偶尔在光化学事件中观察到颗粒形成后的颗粒生长,其生长速率为2.2-4.7 nmh〜(-1)。尺寸选择的超细颗粒的形态学和元素分析表明,在光化学事件中观察到硫酸盐和金属的混合物内部存在半透明部分(超过200个颗粒为49个),而在交通事件中观察到的是聚集的碳质颗粒。观察到(130个粒子中有66个),这在光化学事件中很少被发现。

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