<?xml version="1.0" encoding="utf-8"?><rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns="http://purl.org/rss/1.0/" xmlns:dc="http://purl.org/dc/elements/1.1/"><channel rdf:about="http://www.atmos-meas-tech.net/xml/rss1_0.xml"><title>AMT - Latest Articles</title><link>http://www.atmos-meas-tech.net/</link><description>Atmospheric Measurement Techniques Latest Articles</description><items><rdf:Seq><rdf:li resource="http://www.atmos-meas-tech.net/5/321/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/289/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/275/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/267/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/259/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/243/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/225/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/195/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/193/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/181/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/161/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/149/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/141/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/123/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/99/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/73/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/37/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/17/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/5/1/2012/" /><rdf:li resource="http://www.atmos-meas-tech.net/4/2851/2011/" /></rdf:Seq></items></channel><item rdf:about="http://www.atmos-meas-tech.net/5/321/2012/"><title>Atmospheric ice nucleators active &amp;ge; &amp;minus;12 &amp;deg;C can be quantified on PM&lt;sub&gt;10&lt;/sub&gt; filters</title><link>http://www.atmos-meas-tech.net/5/321/2012/</link><description>&lt;b&gt;Atmospheric ice nucleators active &amp;ge; &amp;minus;12 &amp;deg;C can be quantified on PM&lt;sub&gt;10&lt;/sub&gt; filters&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 321-327, 2012&lt;br /&gt;&lt;br /&gt;Author(s): F. Conen, S. Henne, C. E. Morris, and C. Alewell&lt;br /&gt;&lt;br /&gt;Small number concentrations render it difficult to quantify ice nucleators
(IN) in the atmosphere active at warm temperatures. A useful new method for
IN measurement based around filter collections is proposed. It makes use of
quartz filters used in 24 h PM&lt;sub&gt;10&lt;/sub&gt; monitoring (720 m&lt;sup&gt;3&lt;/sup&gt; air
sample). Small subsamples (1.8 mm diameter) from the effective filter area
and from the clean fringe (blank) are subjected to immersion freezing tests.
We applied the method to eight filters from the High Alpine Research Station
Jungfraujoch (3580 m above sea level) in the Swiss Alps. All filters carried
IN active at &amp;minus;7 &amp;deg;C and below. Number concentrations of IN active at
&amp;minus;8, &amp;minus;10, and &amp;minus;12 &amp;deg;C were on average 3.3, 10.7, and 17.2 m&lt;sup&gt;&amp;minus;3&lt;/sup&gt;,
respectively. Several-fold larger numbers of IN active at &amp;ge; &amp;minus;12 &amp;deg;C
per unit mass of PM&lt;sub&gt;10&lt;/sub&gt; were found in air masses influenced by Swiss and
southern German atmospheric boundary layer air, compared to a Saharan dust
event. In combination with data on PM&lt;sub&gt;10&lt;/sub&gt; mass, the method may be used to
re-construct time series of IN number concentrations.</description><dc:date>2012-02-02T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/289/2012/"><title>Validation of MIPAS IMK/IAA temperature, water vapor, and ozone profiles with MOHAVE-2009 campaign measurements</title><link>http://www.atmos-meas-tech.net/5/289/2012/</link><description>&lt;b&gt;Validation of MIPAS IMK/IAA temperature, water vapor, and ozone profiles with MOHAVE-2009 campaign measurements&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 289-320, 2012&lt;br /&gt;&lt;br /&gt;Author(s): G. P. Stiller, M. Kiefer, E. Eckert, T. von Clarmann, S. Kellmann, M. García-Comas, B. Funke, T. Leblanc, E. Fetzer, L. Froidevaux, M. Gomez, E. Hall, D. Hurst, A. Jordan, N. Kämpfer, A. Lambert, I. S. McDermid, T. McGee, L. Miloshevich, G. Nedoluha, W. Read, M. Schneider, M. Schwartz, C. Straub, G. Toon, L. W. Twigg, K. Walker, and D. N. Whiteman&lt;br /&gt;&lt;br /&gt;MIPAS observations of temperature, water vapor, and ozone in October 2009 as
derived with the scientific level-2 processor run by Karlsruhe Institute of
Technology (KIT), Institute for Meteorology and Climate Research (IMK) and
CSIC, Instituto de Astrofísica de Andalucía (IAA) and retrieved from version
4.67 level-1b data have been compared to co-located field campaign
observations obtained during the MOHAVE-2009 campaign at the Table Mountain
Facility near Pasadena, California in October 2009. The MIPAS measurements were validated
regarding any potential biases of the profiles, and with respect to their
precision estimates. The MOHAVE-2009
measurement campaign provided measurements of atmospheric profiles of
temperature, water vapor/relative humidity, and ozone from the ground to the
mesosphere by a suite of instruments including radiosondes, ozonesondes, frost point
hygrometers, lidars, microwave radiometers and Fourier transform infra-red (FTIR)
spectrometers. For MIPAS
temperatures (version V4O_T_204), no significant bias was detected in
the middle stratosphere; between 22 km and the tropopause MIPAS
temperatures were found to be biased low by up to 2 K, while below the tropopause, they
were found to be too high by the same amount. These findings confirm earlier
comparisons of MIPAS temperatures to ECMWF data which revealed similar
differences. Above 12 km up to 45 km, MIPAS
water vapor (version V4O_H2O_203) is well within 10% of the data of
all correlative instruments.
The well-known
dry bias of MIPAS water vapor above 50 km due to neglect of non-LTE effects
in the current retrievals has been confirmed. Some instruments indicate that
MIPAS water vapor might be biased high by 20 to 40% around 10 km (or 5 km
below the tropopause), but a consistent picture from all comparisons could
not be derived. MIPAS ozone (version V4O_O3_202) has a high bias of up
to +0.9 ppmv around 37 km which is due to a non-identified continuum like
radiance contribution. No further significant biases have been detected.
Cross-comparison to co-located observations of other satellite instruments
(Aura/MLS, ACE-FTS, AIRS) is provided as well.</description><dc:date>2012-02-02T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/275/2012/"><title>Volcanic SO&lt;sub&gt;2&lt;/sub&gt; and SiF&lt;sub&gt;4&lt;/sub&gt; visualization using 2-D thermal emission spectroscopy &amp;ndash; Part 1: Slant-columns and their ratios</title><link>http://www.atmos-meas-tech.net/5/275/2012/</link><description>&lt;b&gt;Volcanic SO&lt;sub&gt;2&lt;/sub&gt; and SiF&lt;sub&gt;4&lt;/sub&gt; visualization using 2-D thermal emission spectroscopy &amp;ndash; Part 1: Slant-columns and their ratios&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 275-288, 2012&lt;br /&gt;&lt;br /&gt;Author(s): W. Stremme, A. Krueger, R. Harig, and M. Grutter&lt;br /&gt;&lt;br /&gt;The composition and emission rates of volcanic gas plumes provide insight of
the geologic internal activity, atmospheric chemistry, aerosol formation and
radiative processes around it. Observations are necessary for public security
and the aviation industry. Ground-based thermal emission infrared
spectroscopy, which uses the radiation of the volcanic gas itself, allows for
continuously monitoring during day and night from a safe distance. We present
measurements on Popocatépetl volcano based on thermal emission
spectroscopy during different campaigns between 2006–2009 using a Scanning
Infrared Gas Imaging System (SIGIS). The experimental set-up, measurement
geometries and analytical algorithms are described. The equipment was
operated from a safe distance of 12 km from the volcano at two different
spectral resolutions: 0.5 and 4 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt;. The 2-dimensional scanning
capability of the instrument allows for an on-line visualization of the
volcanic SO&lt;sub&gt;2&lt;/sub&gt; plume and its animation.
SiF&lt;sub&gt;4&lt;/sub&gt; was also identified in the infrared spectra recorded at both
resolutions. The SiF&lt;sub&gt;4&lt;/sub&gt;/SO&lt;sub&gt;2&lt;/sub&gt; molecular ratio can be calculated from
each image and used as a highly useful parameter to follow changes in
volcanic activity. A small Vulcanian eruption was monitored during the night
of 16 to 17 November 2008 and strong ash emission  together with a pronounced
SO&lt;sub&gt;2&lt;/sub&gt; cloud was registered around 01:00 a.m. LST (Local Standard Time). Enhanced SiF&lt;sub&gt;4&lt;/sub&gt;/SO&lt;sub&gt;2&lt;/sub&gt; ratios were observed
before and after the eruption. A validation of the results from thermal
emission measurements with those from absorption spectra of the moon taken at
the same time, as well as an error analysis, are presented. The inferred
propagation speed from sequential images is used in a subsequent paper (Part 2)
to calculate the emission rates at different distances from the crater.</description><dc:date>2012-02-02T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/267/2012/"><title>Correcting orbital drift signal in the time series of AVHRR derived convective cloud fraction using rotated empirical orthogonal function</title><link>http://www.atmos-meas-tech.net/5/267/2012/</link><description>&lt;b&gt;Correcting orbital drift signal in the time series of AVHRR derived convective cloud fraction using rotated empirical orthogonal function&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 267-273, 2012&lt;br /&gt;&lt;br /&gt;Author(s): A. Devasthale, K.-G. Karlsson, J. Quaas, and H. Grassl&lt;br /&gt;&lt;br /&gt;The Advanced Very High Resolution Radiometer (AVHRR) instruments onboard the
series of National Oceanic and Atmospheric Administration (NOAA) satellites
offer the longest available meteorological data records from space. These
satellites have drifted in orbit resulting in shifts in the local time
sampling during the life span of the sensors onboard. Depending upon the
amplitude of the diurnal cycle of the geophysical parameters derived,
orbital drift may cause spurious trends in their time series. We investigate
tropical deep convective clouds, which show pronounced diurnal cycle
amplitude, to estimate an upper bound of the impact of orbital drift on
their time series. We carry out a rotated empirical orthogonal function
analysis (REOF) and show that the REOFs are useful in delineating orbital
drift signal and, more importantly, in subtracting this signal in the time
series of convective cloud amount. These results will help facilitate the
derivation of homogenized data series of cloud amount from NOAA satellite
sensors and ultimately analyzing trends from them. However, we suggest
detailed comparison of various methods and rigorous testing thereof applying
final orbital drift corrections.</description><dc:date>2012-02-01T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/259/2012/"><title>A method to resolve the phase state of aerosol particles</title><link>http://www.atmos-meas-tech.net/5/259/2012/</link><description>&lt;b&gt;A method to resolve the phase state of aerosol particles&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 259-265, 2012&lt;br /&gt;&lt;br /&gt;Author(s): E. Saukko, H. Kuuluvainen, and A. Virtanen&lt;br /&gt;&lt;br /&gt;The phase state of atmospheric aerosols has an impact on their chemical aging
and their deliquescence and thus their ability to act as cloud condensation
nuclei (CCN). The phase change of particles can be induced by the
deliquescence or efflorescence of water or by chemical aging. Existing
methods, such as tandem differential mobility analysis rely on the size
change of particles related to the water uptake or release.
&lt;br&gt;&lt;br&gt;
To address the need to study the phase change induced by mass-preserving and
nearly mass-preserving processes a new method has been developed. The method
relies on the physical impaction of particles on a smooth substrate and
subsequent counting of bounced particles by a condensation particle counter
(CPC). The connection between the bounce probability and physical properties
of particles is so far qualitative.
&lt;br&gt;&lt;br&gt;
To evaluate the performance of this method, the phase state of ammonium
sulfate and levoglucosan, crystalline and amorphous solid, in the presence of
water vapor was studied. The results show a marked difference in particle
bouncing properties between substances – not only at the critical relative
humidity level, but also on the slope of the bouncing probability with
respect to humidity. This suggests that the method can be used to
differentiate between amorphous and crystalline substances as well as to
differentiate between liquid and solid phases.</description><dc:date>2012-01-30T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/243/2012/"><title>Measurement of turbulent water vapor fluxes using a lightweight unmanned aerial vehicle system</title><link>http://www.atmos-meas-tech.net/5/243/2012/</link><description>&lt;b&gt;Measurement of turbulent water vapor fluxes using a lightweight unmanned aerial vehicle system&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 243-257, 2012&lt;br /&gt;&lt;br /&gt;Author(s): R. M. Thomas, K. Lehmann, H. Nguyen, D. L. Jackson, D. Wolfe, and V. Ramanathan&lt;br /&gt;&lt;br /&gt;We present here the first application of a lightweight unmanned aerial
vehicle (UAV) system designed to measure turbulent properties and vertical
latent heat fluxes (&amp;lambda;&lt;i&gt;E&lt;/i&gt;). Such measurements are crucial to improve our
understanding of linkages between surface moisture supply and boundary layer
clouds and phenomena such as atmospheric rivers. The application of UAVs
allows for measurements on spatial scales complimentary to satellite,
aircraft, and tower derived fluxes. Key system components are: a turbulent
gust probe; a fast response water vapor sensor; an inertial navigation
system (INS) coupled to global positioning system (GPS); and a 100 Hz data
logging system. We present measurements made in the continental boundary
layer at the National Aeronautics and Space Administration (NASA) Dryden
Research Flight Facility located in the Mojave Desert. Two flights
consisting of several horizontal straight flux run legs up to ten kilometers
in length and between 330 and 930 m above ground level (m a.g.l.) are
compared to measurement from a surface tower. Surface measured &amp;lambda;&lt;i&gt;E&lt;/i&gt; ranged from
−53 W m&lt;sup&gt;−2&lt;/sup&gt; to 41 W m&lt;sup&gt;−2&lt;/sup&gt;, and the application of a Butterworth High Pass
Filter (HPF) to the datasets improved agreement to within +/−12 W m&lt;sup&gt;−2&lt;/sup&gt;
for 86% of flux runs, by removing improperly sampled low frequency flux
contributions. This result, along with power and co-spectral comparisons and
consideration of the differing spatial scales indicates the system is able
to resolve vertical fluxes for the measurement conditions encountered.
Challenges remain, and the outcome of these measurements will be used to
inform future sampling strategies and further system development.</description><dc:date>2012-01-27T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/225/2012/"><title>Development and characterization of a single particle laser ablation mass spectrometer (SPLAM) for organic aerosol studies</title><link>http://www.atmos-meas-tech.net/5/225/2012/</link><description>&lt;b&gt;Development and characterization of a single particle laser ablation mass spectrometer (SPLAM) for organic aerosol studies&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 225-241, 2012&lt;br /&gt;&lt;br /&gt;Author(s): F. Gaie-Levrel, S. Perrier, E. Perraudin, C. Stoll, N. Grand, and M. Schwell&lt;br /&gt;&lt;br /&gt;A single particle instrument was developed for real-time analysis of organic
aerosol. This instrument, named Single Particle Laser Ablation Mass
Spectrometry (SPLAM), samples particles using an aerodynamic lens system for
which the theoretical performances were calculated. At the outlet of this
system, particle detection and sizing are realized by using two continuous
diode lasers operating at &amp;lambda; = 403 nm. Polystyrene Latex (PSL),
sodium chloride (NaCl) and dioctylphtalate (DOP) particles were used to
characterize and calibrate optical detection of SPLAM. The optical detection
limit (DL) and detection efficiency (DE) were determined using size-selected
DOP particles. The DE ranges from 0.1 to 90% for 100 and 350 nm DOP
particles respectively and the SPLAM instrument is able to detect and
size-resolve particles as small as 110–120 nm. During optical detection,
particle scattered light from the two diode lasers, is detected by two
photomultipliers and the detected signals are used to trigger UV excimer
laser (&amp;lambda; = 248 nm) used for one-step laser desorption ionization
(LDI) of individual aerosol particles. The formed ions are analyzed by a 1 m
linear time-of-flight mass spectrometer in order to access to the chemical
composition of individual particles. The TOF-MS detection limit for gaseous
aromatic compounds was determined to be 0.85 × 10&lt;sup&gt;&amp;minus;15&lt;/sup&gt; kg
(&amp;sim;4 × 10&lt;sup&gt;3&lt;/sup&gt; molecules). DOP particles were also used to test the overall operation of
the instrument. The analysis of a secondary organic aerosol, formed in a
smog chamber by the ozonolysis of indene, is presented as a first
application of the instrument. Single particle mass spectra were obtained
with an effective hit rate of 8%. Some of these mass spectra were found
to be very different from one particle to another possibly reflecting
chemical differences within the investigated indene SOA particles. Our study
shows that an exhaustive statistical analysis, over hundreds of particles,
and adapted reference mass spectra are further needed to understand the
chemical meaning of single particle mass spectra of chemically complex
submicrometer-sized organic aerosols.</description><dc:date>2012-01-26T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/195/2012/"><title>Three-dimensional factorization of size-resolved organic aerosol mass spectra from Mexico City</title><link>http://www.atmos-meas-tech.net/5/195/2012/</link><description>&lt;b&gt;Three-dimensional factorization of size-resolved organic aerosol mass spectra from Mexico City&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 195-224, 2012&lt;br /&gt;&lt;br /&gt;Author(s): I. M. Ulbrich, M. R. Canagaratna, M. J. Cubison, Q. Zhang, N. L. Ng, A. C. Aiken, and J. L. Jimenez&lt;br /&gt;&lt;br /&gt;A size-resolved submicron organic aerosol composition dataset from a
high-resolution time-of-flight mass spectrometer (HR-ToF-AMS) collected in
Mexico City during the MILAGRO campaign in March 2006 is analyzed using
3-dimensional (3-D) factorization models. A method for estimating the
precision of the size-resolved composition data for use with the
factorization models is presented here for the first time. Two 3-D models are
applied to the dataset. One model is a 3-vector decomposition (PARAFAC
model), which assumes that each chemical component has a constant size
distribution over all time steps. The second model is a vector-matrix
decomposition (Tucker 1 model) that allows a chemical component to have a
size distribution that varies in time. To our knowledge, this is the first
report of an application of 3-D factorization models to data from fast
aerosol instrumentation, and the first application of this vector-matrix
model to any ambient aerosol dataset. A larger number of degrees of freedom
in the vector-matrix model enable fitting real variations in factor size
distributions, but also make the model susceptible to fitting noise in the
dataset, giving some unphysical results. For this dataset and model, more
physically meaningful results were obtained by partially constraining the factor mass
spectra using a priori information and a new regularization method. We find
four factors with each model: hydrocarbon-like organic aerosol (HOA),
biomass-burning organic aerosol (BBOA), oxidized organic aerosol (OOA), and
a locally occurring organic aerosol (LOA). These four factors have
previously been reported from 2-dimensional factor analysis of the
high-resolution mass spectral dataset from this study. The size
distributions of these four factors are consistent with previous reports for
these particle types. Both 3-D models produce useful results, but the
vector-matrix model captures real variability in the size distributions that
cannot be captured by the 3-vector model. A tracer &lt;i&gt;m/z&lt;/i&gt;-based method provides a
useful approximation for the component size distributions in this study.
Variation in the size distributions is demonstrated in a case study day with
a large secondary aerosol formation event, in which there is evidence for
the coating of HOA-containing particles with secondary species, shifting the
HOA size distribution to larger particle sizes. These 3-D factorizations
could be used to extract size-resolved aerosol composition data for
correlation with aerosol hygroscopicity, cloud condensation nuclei (CCN),
and other aerosol impacts. Furthermore, other fast and chemically complex 3-D
datasets, including those from thermal desorption or chromatographic
separation, could be analyzed with these 3-D factorization models.
Applications of these models to new datasets requires careful construction
of error estimates and appropriate choice of models that match the
underlying structure of those data. Factorization studies with these 3-D
datasets have the potential to provide further insights into organic aerosol
sources and processing.</description><dc:date>2012-01-25T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/193/2012/"><title>Corrigendum to &quot;The ACOS CO&lt;sub&gt;2&lt;/sub&gt; retrieval algorithm – Part 1: Description and validation against synthetic observations&quot; published in Atmos. Meas. Tech., 5, 99–121, 2012</title><link>http://www.atmos-meas-tech.net/5/193/2012/</link><description>&lt;b&gt;Corrigendum to &quot;The ACOS CO&lt;sub&gt;2&lt;/sub&gt; retrieval algorithm – Part 1: Description and validation against synthetic observations&quot; published in Atmos. Meas. Tech., 5, 99–121, 2012&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 193-193, 2012&lt;br /&gt;&lt;br /&gt;Author(s): C. W. O'Dell, B. Connor, H. Bösch, D. O'Brien, C. Frankenberg, R. Castano, M. Christi, D. Crisp, A. Eldering, B. Fisher, M. Gunson, J. McDuffie, C. E. Miller, V. Natraj, F. Oyafuso, I. Polonsky, M. Smyth, T. Taylor, G. C. Toon, P. O. Wennberg, and D. Wunch&lt;br /&gt;&lt;br /&gt;No abstract available.</description><dc:date>2012-01-24T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/181/2012/"><title>Quantification of gas-phase glyoxal and methylglyoxal via the Laser-Induced Phosphorescence of (methyl)GLyOxal Spectrometry (LIPGLOS) Method</title><link>http://www.atmos-meas-tech.net/5/181/2012/</link><description>&lt;b&gt;Quantification of gas-phase glyoxal and methylglyoxal via the Laser-Induced Phosphorescence of (methyl)GLyOxal Spectrometry (LIPGLOS) Method&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 181-192, 2012&lt;br /&gt;&lt;br /&gt;Author(s): S. B. Henry, A. Kammrath, and F. N. Keutsch&lt;br /&gt;&lt;br /&gt;Glyoxal and methylglyoxal are key products of oxidative photochemistry in the
lower troposphere. Reliable measurements of such compounds are critical for
testing our understanding of volatile organic compound (VOC) processing in
this region. We present a new method for obtaining sensitive, high time
resolution, in situ measurements of these compounds via laser-induced
phosphorescent decays. By exploiting the unique phosphorescent lifetimes for
each molecule, this method achieves speciation and high-sensitivity
quantification of both molecules. With two different light sources at
different wavelengths, the lowest 3&amp;sigma; limits of detection observed
during calibration with this method are 11 pptv in 5 min for
glyoxal and 243 pptv in 5 min for methylglyoxal. During ambient
measurements of glyoxal, a 3&amp;sigma; limit of detection of
&lt;4.4 pptv in 5 min was observed. Additionally, this method
enables the simultaneous measurement of both glyoxal and methylglyoxal using
a single, non-wavelength-tunable light source, which will allow for the
development of inexpensive (~$40 k) and turnkey instrumentation. The
simplicity and affordability of this new instrumentation would enable the
construction of a long-term, spatially distributed database of these two key
species. This chemical map can be used to constrain or drive regional or
global models as well as provide verification of satellite observations.</description><dc:date>2012-01-23T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/161/2012/"><title>Information operator approach applied to the retrieval of the vertical distribution of atmospheric constituents from ground-based high-resolution FTIR measurements</title><link>http://www.atmos-meas-tech.net/5/161/2012/</link><description>&lt;b&gt;Information operator approach applied to the retrieval of the vertical distribution of atmospheric constituents from ground-based high-resolution FTIR measurements&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 161-180, 2012&lt;br /&gt;&lt;br /&gt;Author(s): C. Senten, M. De Mazière, G. Vanhaelewyn, and C. Vigouroux&lt;br /&gt;&lt;br /&gt;The analysis of high spectral resolution Fourier Transform infrared (FTIR)
solar absorption spectra is an important issue in remote sensing. If this is
done carefully, one can obtain information, not only about the total column
abundances, but also about the vertical distribution of various constituents
in the atmosphere. This work introduces the application of the information
operator approach for extracting vertical profile information from
ground-based FTIR measurements. The algorithm is implemented and tested
within the well-known retrieval code SFIT2, adapting the optimal estimation
method such as to take into account only the significant contributions to
the solution. In particular, we demonstrate the feasibility of the method in
an application to ground-based FTIR spectra taken in the framework of the
Network for the Detection of Atmospheric Composition Change (NDACC) at Ile
de La Réunion (21&amp;deg; S, 55&amp;deg; E). A thorough comparison is made
between the original optimal estimation method, Tikhonov regularization and
this alternative retrieval algorithm, regarding information content,
retrieval robustness and corresponding full error budget evaluation for the
target species ozone (O&lt;sub&gt;3&lt;/sub&gt;), nitrous oxide (N&lt;sub&gt;2&lt;/sub&gt;O), methane
(CH&lt;sub&gt;4&lt;/sub&gt;), and carbon monoxide (CO). It is shown that the information
operator approach performs well and in most cases yields both a better
accuracy and stability than the optimal estimation method. Additionally, the
information operator approach has the advantage of being less sensitive to
the choice of a priori information than the optimal estimation method and
Tikhonov regularization. On the other hand, in general the Tikhonov
regularization results seem to be slightly better than the optimal
estimation method and information operator approach results when it comes to
error budgets and column stability.</description><dc:date>2012-01-16T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/149/2012/"><title>Interferences of commercial NO&lt;sub&gt;2&lt;/sub&gt; instruments in the urban atmosphere and in a smog chamber</title><link>http://www.atmos-meas-tech.net/5/149/2012/</link><description>&lt;b&gt;Interferences of commercial NO&lt;sub&gt;2&lt;/sub&gt; instruments in the urban atmosphere and in a smog chamber&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 149-159, 2012&lt;br /&gt;&lt;br /&gt;Author(s): G. Villena, I. Bejan, R. Kurtenbach, P. Wiesen, and J. Kleffmann&lt;br /&gt;&lt;br /&gt;Reliable measurements of atmospheric trace gases are necessary for both, a
better understanding of the chemical processes occurring in the atmosphere,
and for the validation of model predictions. Nitrogen dioxide (NO&lt;sub&gt;2&lt;/sub&gt;) is
a toxic gas and is thus a regulated air pollutant. Besides, it is of major
importance for the oxidation capacity of the atmosphere and plays a pivotal
role in the formation of ozone and acid precipitation. Detection of NO&lt;sub&gt;2&lt;/sub&gt;
is a difficult task since many of the different commercial techniques used
are affected by interferences. The chemiluminescence instruments that are
used for indirect NO&lt;sub&gt;2&lt;/sub&gt; detection in monitoring networks and smog
chambers use either molybdenum or photolytic converters and are affected by
either positive (NO&lt;sub&gt;y&lt;/sub&gt;) or negative interferences (radical formation in
the photolytic converter). Erroneous conclusions on NO&lt;sub&gt;2&lt;/sub&gt; can be drawn if
these interferences are not taken into consideration. In the present study,
NO&lt;sub&gt;2&lt;/sub&gt; measurements in the urban atmosphere, in a road traffic tunnel and
in a smog-chamber using different commercial techniques, i.e. chemiluminescence instruments with molybdenum or photolytic converters, a
Luminol based instrument and a new NO&lt;sub&gt;2&lt;/sub&gt;-LOPAP, were compared with
spectroscopic techniques, i.e. DOAS and FTIR. Interferences of the different
instruments observed during atmospheric measurements were partly
characterised in more detail in the smog chamber experiments. Whereas all
the commercial instruments showed strong interferences, excellent agreement
was obtained between a new NO&lt;sub&gt;2&lt;/sub&gt;-LOPAP instrument and the FTIR technique
for the measurements performed in the smog chamber.</description><dc:date>2012-01-13T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/141/2012/"><title>Quantification of levoglucosan and its isomers by High Performance Liquid Chromatography &amp;ndash; Electrospray Ionization tandem Mass Spectrometry and its applications to atmospheric and soil samples</title><link>http://www.atmos-meas-tech.net/5/141/2012/</link><description>&lt;b&gt;Quantification of levoglucosan and its isomers by High Performance Liquid Chromatography &amp;ndash; Electrospray Ionization tandem Mass Spectrometry and its applications to atmospheric and soil samples&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 141-148, 2012&lt;br /&gt;&lt;br /&gt;Author(s): C. Piot, J.-L. Jaffrezo, J. Cozic, N. Pissot, I. El Haddad, N. Marchand, and J.-L. Besombes&lt;br /&gt;&lt;br /&gt;The determination of atmospheric concentrations of levoglucosan and its two
isomers, unambiguous tracers of biomass burning emissions, became even more
important with the development of wood as renewable energy for domestic
heating. Many researches demonstrated the increase during recent years of
atmospheric particulate matter load due to domestic biomass combustion in
developed countries. Analysis of biomass burning tracers is traditionally
performed with Gas Chromatography-Mass Spectrometry (GC-MS) technique after
derivatization and requires an organic solvent extraction. A simpler and
faster technique using Liquid Chromatography &amp;ndash; Electrospray Ionisation &amp;ndash;
tandem Mass Spectrometry (LC-ESI-MS/MS) was optimized for the analysis of
levoglucosan, mannosan and galactosan isomers after an aqueous extraction.
This technique allows a good separation between the three compounds in a
very reduced time (runtime ~5 min). LOD and LOQ of this method are 30 μg l&lt;sup&gt;&amp;minus;1&lt;/sup&gt;
and 100 μg l&lt;sup&gt;&amp;minus;1&lt;/sup&gt; respectively, allowing the use of
filters from low-volume sampler (as commonly used in routine campaigns). A
comparison of simultaneous levoglucosan measurements by GC-MS and
LC-ESI-MS/MS for about 50 samples coming from different types of sampling
sites and seasons was realized and shows very good agreement between the two
methods. Therefore LC-ESI-MS/MS method can be used as an alternative to
GC-MS particularly for measurement campaigns in routine where analysis time
is important and detection limit is reduced. This paper shows that this
method is also applicable to other environmental sample types like soil.</description><dc:date>2012-01-12T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/123/2012/"><title>Antarctic ozone hole as observed by IASI/MetOp for 2008–2010</title><link>http://www.atmos-meas-tech.net/5/123/2012/</link><description>&lt;b&gt;Antarctic ozone hole as observed by IASI/MetOp for 2008–2010&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 123-139, 2012&lt;br /&gt;&lt;br /&gt;Author(s): C. Scannell, D. Hurtmans, A. Boynard, J. Hadji-Lazaro, M. George, A. Delcloo, O. Tuinder, P.-F. Coheur, and C. Clerbaux&lt;br /&gt;&lt;br /&gt;In this paper we present a study of the ozone hole as observed by the
Infrared Atmospheric Sounding Interferometer (IASI) on-board the MetOp-A
European satellite platform from the beginning of data dissemination, August
2008, to the end of December 2010. Here we demonstrate IASI's ability to
capture the seasonal characteristics of the ozone hole, in particular during
polar night. We compare IASI ozone total columns and vertical profiles with
those of the Global Ozone Monitoring Experiment 2 (GOME-2, also on-board
MetOp-A) and electrochemical concentration cell (ECC) ozone sonde
measurements. Total ozone column from IASI and GOME-2 were found to be in
excellent agreement for this region with a correlation coefficient of 0.97,
for September, October and November 2009. On average IASI exhibits a
positive bias of approximately 7% compared to the GOME-2 measurements
over the entire ozone hole period. Comparisons between IASI and ozone sonde
measurements were also found to be in good agreement with the difference
between both ozone profile measurements being less than &amp;plusmn;30% over
the altitude range of 0–40 km. The vertical structure of the ozone profile
inside the ozone hole is captured remarkably well by IASI.</description><dc:date>2012-01-12T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/99/2012/"><title>The ACOS CO&lt;sub&gt;2&lt;/sub&gt; retrieval algorithm – Part 1: Description and validation against synthetic observations</title><link>http://www.atmos-meas-tech.net/5/99/2012/</link><description>&lt;b&gt;The ACOS CO&lt;sub&gt;2&lt;/sub&gt; retrieval algorithm – Part 1: Description and validation against synthetic observations&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 99-121, 2012&lt;br /&gt;&lt;br /&gt;Author(s): C. W. O'Dell, B. Connor, H. Bösch, D. O'Brien, C. Frankenberg, R. Castano, M. Christi, D. Eldering, B. Fisher, M. Gunson, J. McDuffie, C. E. Miller, V. Natraj, F. Oyafuso, I. Polonsky, M. Smyth, T. Taylor, G. C. Toon, P. O. Wennberg, and D. Wunch&lt;br /&gt;&lt;br /&gt;This work describes the NASA Atmospheric CO&lt;sub&gt;2&lt;/sub&gt; Observations
from Space (ACOS) &lt;i&gt;X&lt;/i&gt;&lt;sub&gt;CO&lt;sub&gt;2&lt;/sub&gt;&lt;/sub&gt; retrieval algorithm, and its
performance on highly realistic, simulated observations. These
tests, restricted to observations over land, are used to
evaluate retrieval errors in the face of realistic clouds and
aerosols, polarized non-Lambertian surfaces, imperfect
meteorology, and uncorrelated instrument noise. We find that
post-retrieval filters are essential to eliminate the poorest
retrievals, which arise primarily due to imperfect cloud
screening. The remaining retrievals have RMS errors of
approximately 1 ppm. Modeled instrument noise, based on the
Greenhouse Gases Observing SATellite (GOSAT) in-flight
performance, accounts for less than half the total error in
these retrievals. A small fraction of unfiltered clouds,
particularly thin cirrus, lead to a small positive bias of
~0.3 ppm. Overall, systematic errors due to imperfect
characterization of clouds and aerosols dominate the error
budget, while errors due to other simplifying assumptions, in
particular those related to the prior meteorological fields,
appear small.</description><dc:date>2012-01-11T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/73/2012/"><title>Aerosol classification using airborne High Spectral Resolution Lidar measurements – methodology and examples</title><link>http://www.atmos-meas-tech.net/5/73/2012/</link><description>&lt;b&gt;Aerosol classification using airborne High Spectral Resolution Lidar measurements – methodology and examples&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 73-98, 2012&lt;br /&gt;&lt;br /&gt;Author(s): S. P. Burton, R. A. Ferrare, C. A. Hostetler, J. W. Hair, R. R. Rogers, M. D. Obland, C. F. Butler, A. L. Cook, D. B. Harper, and K. D. Froyd&lt;br /&gt;&lt;br /&gt;The NASA Langley Research Center (LaRC) airborne High Spectral Resolution
Lidar (HSRL) on the NASA B200 aircraft has acquired extensive datasets of
aerosol extinction (532 nm), aerosol optical depth (AOD) (532 nm),
backscatter (532 and 1064 nm), and depolarization (532 and 1064 nm) profiles
during 18 field missions that have been conducted over North America since
2006. The lidar measurements of aerosol intensive parameters (lidar ratio,
depolarization, backscatter color ratio, and spectral depolarization ratio)
are shown to vary with location and aerosol type. A methodology based on
observations of known aerosol types is used to qualitatively classify the
extensive set of HSRL aerosol measurements into eight separate types.
Several examples are presented showing how the aerosol intensive parameters
vary with aerosol type and how these aerosols are classified according to
this new methodology. The HSRL-based classification reveals vertical
variability of aerosol types during the NASA ARCTAS field experiment
conducted over Alaska and northwest Canada during 2008. In two examples
derived from flights conducted during ARCTAS, the HSRL classification of
biomass burning smoke is shown to be consistent with aerosol types derived
from coincident airborne in situ measurements of particle size and
composition. The HSRL retrievals of AOD and inferences of aerosol types are
used to apportion AOD to aerosol type; results of this analysis are shown
for several experiments.</description><dc:date>2012-01-10T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/37/2012/"><title>Autofluorescence of atmospheric bioaerosols – fluorescent biomolecules and potential interferences</title><link>http://www.atmos-meas-tech.net/5/37/2012/</link><description>&lt;b&gt;Autofluorescence of atmospheric bioaerosols – fluorescent biomolecules and potential interferences&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 37-71, 2012&lt;br /&gt;&lt;br /&gt;Author(s): C. Pöhlker, J. A. Huffman, and U. Pöschl&lt;br /&gt;&lt;br /&gt;Primary biological aerosol particles (PBAP) are an important subset of air
particulate matter with a substantial contribution to the organic aerosol
fraction and potentially strong effects on public health and climate. Recent
progress has been made in PBAP quantification by utilizing real-time
bioaerosol detectors based on the principle that specific organic molecules
of biological origin such as proteins, coenzymes, cell wall compounds and
pigments exhibit intrinsic fluorescence. The properties of many fluorophores
have been well documented, but it is unclear which are most relevant for
detection of atmospheric PBAP. The present study provides a systematic
synthesis of literature data on potentially relevant biological
fluorophores. We analyze and discuss their relative importance for the
detection of fluorescent biological aerosol particles (FBAP) by online
instrumentation for atmospheric measurements such as the ultraviolet
aerodynamic particle sizer (UV-APS) or the wide issue bioaerosol sensor
(WIBS).
&lt;br&gt;&lt;br&gt;
In addition, we provide new laboratory measurement data for selected
compounds using bench-top fluorescence spectroscopy. Relevant biological
materials were chosen for comparison with existing literature data and to
fill in gaps of understanding. The excitation-emission matrices (EEM)
exhibit pronounced peaks at excitation wavelengths of ~280 nm and
~360 nm, confirming the suitability of light sources used for online
detection of FBAP. They also show, however, that valuable information is
missed by instruments that do not record full emission spectra at multiple
wavelengths of excitation, and co-occurrence of multiple fluorophores within
a detected sample will likely confound detailed molecular analysis. Selected
non-biological materials were also analyzed to assess their possible
influence on FBAP detection and generally exhibit only low levels of
background-corrected fluorescent emission. This study strengthens the
hypothesis that ambient supermicron particle fluorescence in wavelength
ranges used for most FBAP instruments is likely to be dominated by
biological material and that such instrumentation is able to discriminate
between FBAP and non-biological material in many situations. More detailed
follow-up studies on single particle fluorescence are still required to
reduce these uncertainties further, however.</description><dc:date>2012-01-09T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/17/2012/"><title>Ground-based water vapor raman lidar measurements up to the upper troposphere and lower stratosphere for long-term monitoring</title><link>http://www.atmos-meas-tech.net/5/17/2012/</link><description>&lt;b&gt;Ground-based water vapor raman lidar measurements up to the upper troposphere and lower stratosphere for long-term monitoring&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 17-36, 2012&lt;br /&gt;&lt;br /&gt;Author(s): T. Leblanc, I. S. McDermid, and T. D. Walsh&lt;br /&gt;&lt;br /&gt;Recognizing the importance of water vapor in the upper troposphere and lower
stratosphere (UTLS) and the scarcity of high-quality, long-term
measurements, JPL began the development of a powerful Raman lidar in 2005 to
try to meet these needs. This development was endorsed by the Network for
the Detection of Atmospheric Composition Change (NDACC) and the validation
program for the EOS-Aura satellite. In this paper we review the stages in
the instrumental development, data acquisition and analysis, profile
retrieval and calibration procedures of the lidar, as well as selected
results from three validation campaigns: MOHAVE (Measurements of Humidity in
the Atmosphere and Validation Experiments), MOHAVE-II, and MOHAVE 2009.
&lt;br&gt;&lt;br&gt;
In particular, one critical result from this latest campaign is the very
good agreement (well below the reported uncertainties) observed between the
lidar and the Cryogenic Frost-Point Hygrometer in the entire lidar range
3–20 km, with a mean bias not exceeding 2% (lidar dry) in the lower
troposphere, and 3% (lidar moist) in the UTLS. Ultimately the lidar has
demonstrated capability to measure water vapor profiles from &amp;sim;1 km
above the ground to the lower stratosphere with a precision of 10% or
better near 13 km and below, and an estimated accuracy of 5%. Since 2005,
nearly 1000 profiles have been routinely measured, and since 2009, the
profiles have typically reached 14 km for one-hour integration times and 1.5 km vertical resolution, and can reach 21 km for 6-h integration times
using degraded vertical resolutions.
&lt;br&gt;&lt;br&gt;
These performance figures show that, with our present target of routinely
running our lidar two hours per night, 4 nights per week, we can achieve
measurements with a precision in the UTLS equivalent to that achieved if
launching one CFH per month.</description><dc:date>2012-01-04T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/5/1/2012/"><title>Identification and localization of layers in the ionosphere using the eikonal and amplitude of radio occultation signals</title><link>http://www.atmos-meas-tech.net/5/1/2012/</link><description>&lt;b&gt;Identification and localization of layers in the ionosphere using the eikonal and amplitude of radio occultation signals&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 5, 1-16, 2012&lt;br /&gt;&lt;br /&gt;Author(s): A. G. Pavelyev, Y. A. Liou, K. Zhang, C. S. Wang, J. Wickert, T. Schmidt, V. N. Gubenko, A. A. Pavelyev, and Y. Kuleshov&lt;br /&gt;&lt;br /&gt;By using the CHAllenge Minisatellite Payload (CHAMP) radio occultation (RO)
data, a description of different types of the ionospheric impacts on the RO
signals at the altitudes 30–90 km of the RO ray perigee is given and
compared with the results of measurements obtained earlier in the
satellite-to-Earth communication link at frequency 1.5415 GHz. An analytical
model is introduced for describing propagation of radio waves in a
stratified medium consisting of sectors with spherically symmetric
refractivity distribution. This model gives analytical expressions for the
phase, bending angle, and refractive attenuation of radio waves and is
applied to the analysis of radio wave propagation phenomena along an
extended path including the atmosphere and two parts of the ionosphere. The
model explains significant amplitude and phase variations at altitudes 30–90 km of the RO ray perigee and attributes them to inclined ionospheric layers.
Based on this analytical model, an innovative technique is introduced to
locate layers in the atmosphere and ionosphere. A necessary and sufficient
criterion is obtained for a layer to be located at the RO ray perigee. This
criterion gives both qualitative and quantitative estimation of the
displacement of an ionospheric and/or atmospheric layer from the RO ray
perigee. This is important, in particular, for determining the location of
wind shears and directions of the internal wave propagation in the lower
ionosphere, and, possibly, in the atmosphere.</description><dc:date>2012-01-04T00:00:00+01:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech.net/4/2851/2011/"><title>Effective density of Aquadag and fullerene soot black carbon reference materials used for SP2 calibration</title><link>http://www.atmos-meas-tech.net/4/2851/2011/</link><description>&lt;b&gt;Effective density of Aquadag and fullerene soot black carbon reference materials used for SP2 calibration&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques, 4, 2851-2858, 2011&lt;br /&gt;&lt;br /&gt;Author(s): M. Gysel, M. Laborde, J. S. Olfert, R. Subramanian, and A. J. Gröhn&lt;br /&gt;&lt;br /&gt;The mass and effective density of black carbon (BC) particles generated from
aqueous suspensions of Aquadag and fullerene soot was measured and
parametrized as a function of their mobility diameter. The measurements were
made by two independent research groups by operating a differential mobility
analyser (DMA) in series with an aerosol particle mass analyser (APM) or a
Couette centrifugal particle mass analyser (CPMA). Consistent and
reproducible results were found in this study for different production lots
of Aquadag, indicating that the effective density of these particles is a
stable quantity and largely unaffected by differences in aerosol generation
procedures and suspension treatments. The effective density of fullerene soot
particles from one production lot was also found to be stable and independent
of suspension treatments. Some differences to previous literature data were
observed for both Aquadag and fullerene soot at larger particle diameters.
Knowledge of the exact relationship between mobility diameter and particle
mass is of great importance, as DMAs are commonly used to size-select
particles from BC reference materials for calibration of single particle soot
photometers (SP2), which quantitatively detect the BC mass in single
particles.</description><dc:date>2011-12-22T00:00:00+01:00</dc:date></item></rdf:RDF>
