A chemical analyzer for charged ultrafine particles
and Physics
cess
Atmospheric
Measurement
Techniques
Open Access
Biogeosciences
Open Access
Atmos. Meas. Tech., 6, 2339–2348, 2013
www.atmos-meas-tech.net/6/2339/2013/
doi:10.5194/amt-6-2339-2013
© Author(s) 2013. CC Attribution 3.0 License.
Climate
1 Junior Professorship in Atmospheric Chemistry, University of Bayreuth, 95440 Bayreuth, Germany
of the Past
S. G. Gonser1,2 and A. Held1,2
2 Bayreuth
Center of Ecology and Environmental Research, University of Bayreuth, 95440 Bayreuth, Germany
Received: 28 March 2013 – Published in Atmos. Meas. Tech. Discuss.: 18 April 2013
Revised: 15 July 2013 – Accepted: 31 July 2013 – Published: 11 September 2013
1
Introduction
Geoscientific
Instrumentation
Methods
andfor the Earth’s
Aerosol particles are of significant
relevance
radiation balance (ForsterData
et al., Systems
2007) and human health
Open Access
(Delfino et al., 2005; Stieb et al., 2002). It is well known
that part of the aerosol forms in the atmosphere through nucleation of gas-phase precursor
molecules. The formation of
Geoscientific
these so-called secondary aerosol particles can be observed
in the planetaryModel
boundaryDevelopment
layer at a multitude of locations
around the world both in natural backgrounds as well as in
polluted industrial areas (e.g. Kulmala et al., 2004). Typically, particle nucleation events begin in the morning hours
Hydrology and
and the nucleated particles grow for several hours to a few
Earth System
days by coagulation and condensation,
reaching diameters in
the order of 100 nm. Typical aerosol
growth
Sciencesand nucleation
rates are in the range of 1–20 nm h−1 and 0.01–10 cm−3 s−1 ,
respectively (Kulmala et al., 2004). Once the initial nuclei
are formed the particles will grow due to condensation of
certain trace gases. The main contributors to the growth of
Science
particles are thought toOcean
be sulfuric
acid, oxidation products
of volatile organic compounds (VOCs), ammonia salts such
as ammonium sulfate and aminium salts, as has been shown
by several studies using direct as well as indirect methods
(e.g. Barsanti et al, 2009; Held et al., 2004; Laaksonen et
al., 2008; Riipinen et al., 2009; Smith et al., 2010). Even
Solid
though there is a general idea
about Earth
the mechanisms governing the growth of freshly nucleated particles a lot of processes remain unrevealed. This is due to the challenging task
of performing online chemical analysis of sub-30 nm particles. The small mass of these ultrafine particles is a limiting
factor. For example, a particle of 10 nm diameter has a mass
The Cryosphere
of a few attograms (10−18 g). The preferred method to perform such measurements is the mass spectrometric approach,
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Abstract. New particle formation is a frequent phenomenon
in the atmosphere and of major significance for the Earth’s
climate and human health. To date the mechanisms leading
to the nucleation of particles as well as to aerosol growth are
not completely understood. A lack of appropriate measurement equipment for online analysis of the chemical composition of freshly nucleated particles is one major limitation. We have developed a Chemical Analyzer for Charged
Ultrafine Particles (CAChUP) capable of analyzing particles
with diameters below 30 nm. A bulk of size-separated particles is collected electrostatically on a metal filament, resistively desorbed and subsequently analyzed for its molecular
composition in a time of flight mass spectrometer. We report
on technical details as well as characterization experiments
performed with the CAChUP. Our instrument was tested in
the laboratory for its detection performance as well as for its
collection and desorption capabilities. The manual application of defined masses of camphene (C10 H16 ) to the desorption filament resulted in a detection limit between 0.5 and
5 ng, and showed a linear response of the mass spectrometer.
Flow tube experiments of 25 nm diameter secondary organic
aerosol from ozonolysis of alpha-pinene also showed a linear
relation between collection time and the mass spectrometer’s
signal intensity. The resulting mass spectra from the collection experiments are in good agreement with published work
on particles generated by the ozonolysis of alpha-pinene. A
sensitivity study shows that the current setup of CAChUP is
ready for laboratory measurements and for the observation of
new particle formation events in the field.
Earth System
Dynamics
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Correspondence to: S. G. Gonser ()
Open Access
A chemical analyzer for charged ultrafine particles
Open Access
Published by Copernicus Publications on behalf of the European Geosciences Union.
M
2340
S. G. Gonser and A. Held: A chemical analyzer for charged ultrafine particles
as the achieved detection limits are low enough to analyze
chemical components of ultrafine particles.
To date there are two instruments available which are capable of performing online measurements of the chemical
composition of sub-30 nm aerosol particles in the field: (I)
NAMS – the Nano Aerosol Mass Spectrometer (Wang et al.,
2006) and (II) TDCIMS – the Thermal Desorption Chemical
Ionization Mass Spectrometer (Voisin et al., 2003). NAMS is
capable of measuring the quantitative atomic composition of
individual particles down to diameters of 7 nm (Wang et al.,
2006). Its principle of operation is the laser-induced ablation
of single particles captured in an ion trap, and the subsequent
elemental analysis with a time of flight mass spectrometer
(TOF-MS). Due to the high energetic laser pulse the particles break up into ionized atomic elements. Thus, molecular
information about the sampled aerosol is not available. The
TDCIMS, in contrast, analyzes the molecular composition of
a particle bulk of one size range, down to diameters of 6 nm
(Smith et al., 2004). The particles are charged in a unipolar charger, size selected in a differential mobility analyzer
(DMA), collected on a filament and subsequently evaporated.
The resulting gas is chemically ionized and analyzed for
its molecular composition in a triple-quadrupole mass spectrometer, an ion trap mass spectrometer (Held et al., 2009), or
a high-resolution time of flight mass spectrometer (Winkler
et al., 2012). Both instruments are custom-built. Considering the scarcity of available instrumentation to measure the
molecular composition of sub-30 nm particles, we present
the design and first measurement results of an additional
aerosol mass spectrometer for this size range. In principle,
our instrument is similar to the TDCIMS, with a few major
differences: firstly, for charging the particles we optionally
use a non-radioactive source, thus facilitating the transport
of the instrument to field sites in consideration of the transport restrictions regarding radioactive material. Secondly, we
use a compact TOF-MS, minimizing the overall size of our
instrument while accepting a lower mass resolution. Thirdly,
we use electron ioniza (...truncated)