Filters

2014 - 20182

More filters

2019 - 201912020 - 20231
Reset filters

Settings

Author: Riede, Hella × Type: Text ×

Search Results

Now showing 1 - 2 of 2
  • Thumbnail Image
    Item
    Mercury plumes in the global upper troposphere observed during flights with the CARIBIC observatory from may 2005 until june 2013
    (Basel : MDPI, 2014) Slemr, Franz; Weigelt, Andreas; Ebinghaus, Ralf; Brenninkmeijer, Carl; Baker, Angela; Schuck, Tanja; Rauthe-Schöch, Armin; Riede, Hella; Leedham, Emma; Hermann, Markus; van Velthoven, Peter; Oram, David; O'Sullivan, Debbie; Dyroff, Christoph; Zahn, Andreas; Ziereis, Helmut
    Tropospheric sections of flights with the CARIBIC (Civil Aircraft for Regular Investigation of the Atmosphere Based on an Instrumented Container) observatory from May 2005 until June 2013, are investigated for the occurrence of plumes with elevated Hg concentrations. Additional information on CO, CO2, CH4, NOy, O3, hydrocarbons, halocarbons, acetone and acetonitrile enable us to attribute the plumes to biomass burning, urban/industrial sources or a mixture of both. Altogether, 98 pollution plumes with elevated Hg concentrations and CO mixing ratios were encountered, and the Hg/CO emission ratios for 49 of them could be calculated. Most of the plumes were found over East Asia, in the African equatorial region, over South America and over Pakistan and India. The plumes encountered over equatorial Africa and over South America originate predominantly from biomass burning, as evidenced by the low Hg/CO emission ratios and elevated mixing ratios of acetonitrile, CH3Cl and particle concentrations. The backward trajectories point to the regions around the Rift Valley and the Amazon Basin, with its outskirts, as the source areas. The plumes encountered over East Asia and over Pakistan and India are predominantly of urban/industrial origin, sometimes mixed with products of biomass/biofuel burning. Backward trajectories point mostly to source areas in China and northern India. The Hg/CO2 and Hg/CH4 emission ratios for several plumes are also presented and discussed.
  • Thumbnail Image
    Item
    Strong impact of wildfires on the abundance and aging of black carbon in the lowermost stratosphere
    (Washington, DC : NAS, 2018) Ditas, Jeannine; Ma, Nan; Zhang, Yuxuan; Assmann, Denise; Neumaier, Marco; Riede, Hella; Karu, Einar; Williams, Jonathan; Scharffe, Dieter; Wang, Qiaoqiao; Saturno, Jorge; Schwarz, Joshua P.; Katich, Joseph M.; McMeeking, Gavin R.; Zahn, Andreas; Hermann, Markus; Brenninkmeijer, Carl A. M.; Andreae, Meinrat O.; Pöschl, Ulrich; Su, Hang; Cheng, Yafang
    Wildfires inject large amounts of black carbon (BC) particles into the atmosphere, which can reach the lowermost stratosphere (LMS) and cause strong radiative forcing. During a 14-month period of observations on board a passenger aircraft flying between Europe and North America, we found frequent and widespread biomass burning (BB) plumes, influencing 16 of 160 flight hours in the LMS. The average BC mass concentrations in these plumes (∼140 ng·m−3, standard temperature and pressure) were over 20 times higher than the background concentration (∼6 ng·m−3) with more than 100-fold enhanced peak values (up to ∼720 ng·m−3). In the LMS, nearly all BC particles were covered with a thick coating. The average mass equivalent diameter of the BC particle cores was ∼120 nm with a mean coating thickness of ∼150 nm in the BB plume and ∼90 nm with a coating of ∼125 nm in the background. In a BB plume that was encountered twice, we also found a high diameter growth rate of ∼1 nm·h−1 due to the BC particle coatings. The observed high concentrations and thick coatings of BC particles demonstrate that wildfires can induce strong local heating in the LMS and may have a significant influence on the regional radiative forcing of climate.