4.7 Article

Long-range transport of Ambrosia pollen to Poland

Journal

AGRICULTURAL AND FOREST METEOROLOGY
Volume 148, Issue 10, Pages 1402-1411

Publisher

ELSEVIER SCIENCE BV
DOI: 10.1016/j.agrformet.2008.04.005

Keywords

aerobiology; ragweed; Ambrosia; back-trajectory analysis; planetary boundary layer

Funding

  1. European Union's Sixth Framework Programme
  2. European project [MTKD-CT-2004-003170]
  3. Polish Ministry of Education and Science [128/E-366/6 PR UE/DIE265]
  4. Copenhagen Global Change Initiative
  5. National Centre for Environmental Prediction (NCEP)
  6. World Meteorological Organization (WMO) World Weather Watch Programme

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The long-range transport of Ambrosia pollen to Poland is intermittent and mainly related to the passage of air masses over the Carpathian and Sudetes mountains. These episodes are associated with hot dry weather, a deep Planetary Boundary Layer (PBL) in the source areas and winds from the south. Such episodes can transport significant amounts of Ambrosia pollen into Poland. The study investigates Ambrosia pollen episodes at eight sites in Poland during the period 7th-10th September 2005, by examining temporal variations in Ambrosia pollen and back-trajectories. PBL depths in the likely source areas were calculated with the Eta meteorological model and evaluated against the mountain heights. Considerable amounts of Ambrosia pollen were recorded at several monitoring sites during the night or early in the morning of the investigated period. Trajectory analyses shows that the air masses arriving at the Polish sites predominantly came from the south, and were in the Czech Republic, Slovakia and Hungary the previous day indicating these countries as potential source areas. We have shown the progress of Ambrosia plumes into Poland from the south of the country, probably from Slovakia and Hungary, and demonstrated how Lagrangian back-trajectory models and meteorological models can be used to identify possible transport mechanisms of Ambrosia pollen from potential source regions. (C) 2008 Elsevier B.V. All rights reserved.

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