Abstract

Abstract. This study investigates the processes and conditions favouring the formation of nanoparticles (diameter<10 nm) which are frequently observed on high mountains reaching the low free troposphere. This was done through an analysis of a data set collected at Izaña Global Atmospheric Watch Observatory (Canary Islands; 2367 m above sea level). This high mountain supersite is located well above the stratocumulus layer characteristic of the subtropical oceanic tropospheres. At night, when the catabic flow regime is well established, free troposphere aerosols were measured. The development of orographic buoyant upward flows during daylight resulted in an increase of water vapour, SO2 and NOy concentrations. These ascending airflows perturbed the free troposphere and resulted in high concentrations of 3–10 nm particles (N3–10) due to new particle formation. An analysis of the 5-min average time series allowed the identification of two main types of N3–10 event. In Type I events a linear relationship between N3–10 and SO2 was observed (r2 coefficients 0.70–0.95 and a mean slope of 11 cm−3 ppt−1 for 5-min averaged data; SO2 concentrations from tens to hundreds of ppt). These particles seem to be formed during upward transport (probably within or after the outflows of clouds typically located below Izaña). During Type II events, no correlation between SO2 and N3–10 was observed and 3–10 nm particles were formed in-situ at noon and during the afternoon due to the condensation of vapours linked to photochemistry. New particle formation was observed almost every day owing to the favourable conditions associated with the entry of boundary layer air in the low free troposphere, even if SO2 concentrations are rather low at Izaña (tens to hundreds of ppt). The low surface area of pre-existing particles, low temperature and high radiation intensity clearly favoured the formation of nanoparticles. The low surface area of pre-existing particles in the upward flows is furthered by in-cloud particles scavenging in the stratocumulus layer typically located below Izaña. The higher temperature and the presence of coarse Saharan dust particles decrease the efficiency of the new particle formation mechanisms in summer. Thus, the "N3–10 versus SO2" slope (for r2>0.7 cases) was higher in autumn and winter (~15 cm−3 ppt−1 as average) than in summer (2–8 cm−3 ppt−1). These field observations suggest that elevated mounts that reaches the free troposphere may act as source regions for new particles.

Highlights

  • New particle formation (NPF) by nucleation and subsequent growth processes has become a topic of great interest in atmospheric and environmental sciences

  • A data set of aerosol size distribution, trace gases, a set of radiation components and meteorological data collected during 2007–2008 at Izana Mountain observatory has been analysed with the aim of identifying the processes and conditions favouring the formation of 3–10 nm particles

  • In Type I events, a linear relationship between N3−10 and SO2 was observed (r2 coefficients 0.70–0.95, a mean slope of 11 cm−3 ppt−1 and SO2 concentrations within the range from tens to hundreds of ppt). These particles seem to be formed during the upward transport process, most probably within or after the outflows of the cloud layer typically located well below Izana

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Summary

Introduction

New particle formation (NPF) by nucleation and subsequent growth processes has become a topic of great interest in atmospheric and environmental sciences These particles are initially detected at sizes ≥3 nm and may grow until reaching a size within the range of 50 nm to >100 nm. The aim of this study is to investigate the processes and conditions that favour the formation of 3–10 nm particles observed on such high mountains entering the low free troposphere For this purpose a comprehensive data base, collected at Izana Mountain Observatory (Tenerife, Canary Islands, Fig. 1) during 2007–2008, has been analysed. Because under the trade wind regime condensation level is usually lower than the inversion level, the top of the MBL (frequently located just below the TIL) is characterised by a layer of stratocumulus formed by condensation of water vapour onto the available pre-existing particles (Fig. 2a).

Trace gases
Classification of 3–10 nm particle events
Influence of environmental parameters
Surface of pre-existing particles as a condensation sink
Solar radiation
Temperature
Findings
Summary and conclusions
Full Text
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