<?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-discuss.net/xml/rss1_0.xml"><title>AMTD - Latest Articles</title><link>http://www.atmos-meas-tech-discuss.net/</link><description>Atmospheric Measurement Techniques Discussions Latest Articles</description><items><rdf:Seq><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3987/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3971/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3925/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3907/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3877/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3851/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3803/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3747/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3725/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3675/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3643/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3601/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3535/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3489/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3455/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3425/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3383/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3345/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3319/2010/" /><rdf:li resource="http://www.atmos-meas-tech-discuss.net/3/3293/2010/" /></rdf:Seq></items></channel><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3987/2010/"><title>Remote sensing of water vapour profiles in the framework of the Total Carbon Column Observing Network (TCCON)</title><link>http://www.atmos-meas-tech-discuss.net/3/3987/2010/</link><description>&lt;b&gt;Remote sensing of water vapour profiles in the framework of the Total Carbon Column Observing Network (TCCON)&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3987-4007, 2010&lt;br /&gt;&lt;br /&gt;Author(s): M. Schneider, E. Sepúlveda, O. García, F. Hase, and T. Blumenstock&lt;br /&gt;&lt;br /&gt;We show that the near infrared solar absorption spectra recorded in the framework of
the Total Carbon Column Observing Network (TCCON) can be used to derive the vertical distribution
of tropospheric water vapour. Using spectral H&lt;sub&gt;2&lt;/sub&gt;O signatures in the 4500–4700 cm&lt;sup&gt;−1&lt;/sup&gt;
region one can well distinguish lower from middle/upper tropospheric water vapour concentrations.
The vertical resolution is about 3 and 6 km, for the lower and middle/upper troposphere,
respectively. We document the quality of the remotely-sensed profiles by comparisons with
coincident in-situ Vaisala RS92 radiosonde measurements. The agreement of both techniques
is very satisfactory. Due to the long-term strategy of the network and the high measurement
frequency, the TCCON water vapour profile data offer novel opportunities for estimating
the water vapour variability at different time scales and altitudes.</description><dc:date>2010-08-31T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3971/2010/"><title>Observation of the exhaust plume from the space shuttle main engine using the Microwave Limb Sounder</title><link>http://www.atmos-meas-tech-discuss.net/3/3971/2010/</link><description>&lt;b&gt;Observation of the exhaust plume from the space shuttle main engine using the Microwave Limb Sounder&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3971-3986, 2010&lt;br /&gt;&lt;br /&gt;Author(s): H. C. Pumphrey, A. Lambert, and N. J. Livesey&lt;br /&gt;&lt;br /&gt;A space shuttle launch deposits 700 t of water in the
atmosphere. Some of this water is released into the upper mesosphere
and lower thermosphere where it may be directly detected by a limb
sounding satellite instrument. We report measurements of water vapour
plumes from shuttle launches made by the Microwave Limb Sounder (MLS)
on the Aura satellite. Approximately 50% of shuttle launches are
detected by MLS. The signal appears at a similar level across the
upper 10 km of the MLS limb scan, suggesting that the bulk of the
observed water is above the top of the scan. Only a small fraction at
best of smaller launches (Ariane, Proton) are detected. We conclude
that the sensitivity of MLS is only just great enough to detect a
shuttle sized launch, but that a suitably designed instrument of the
same general type could detect the exhausts from a large proportion of
heavy-lift launches.</description><dc:date>2010-08-30T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3925/2010/"><title>Airborne DOAS limb measurements of tropospheric trace gas profiles: case study on the profile retrieval of O&lt;sub&gt;4&lt;/sub&gt; and BrO</title><link>http://www.atmos-meas-tech-discuss.net/3/3925/2010/</link><description>&lt;b&gt;Airborne DOAS limb measurements of tropospheric trace gas profiles: case study on the profile retrieval of O&lt;sub&gt;4&lt;/sub&gt; and BrO&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3925-3969, 2010&lt;br /&gt;&lt;br /&gt;Author(s): C. Prados-Roman, A. Butz, T. Deutschmann, M. Dorf, L. Kritten, A. Minikin, U. Platt, H. Schlager, H. Sihler, N. Theys, M. Van Roozendael, T. Wagner, and K. Pfeilsticker&lt;br /&gt;&lt;br /&gt;A novel limb scanning mini-DOAS spectrometer for the detection
      of UV/vis absorbing radicals (e.g., O&lt;sub&gt;3&lt;/sub&gt;, BrO, IO, HONO)
      was deployed on the DLR-Falcon (Deutsches Zentrum für Luft-
      und Raumfahrt) aircraft and tested during the ASTAR 2007
      campaign (Arctic Study of Tropospheric Aerosol, Clouds and
      Radiation) that took place at Svalbard (78° N) in
      spring 2007. Our main objectives during this campaign were to
      test the instrument, and to perform spectral and profile
      retrievals of tropospheric trace gases, with particular
      interest on investigating the distribution of halogen
      compounds (e.g., BrO) during the so-called ozone depletion
      events (ODEs). In the present work, a new method for the
      retrieval of vertical profiles of tropospheric trace gases
      from tropospheric DOAS limb observations is presented. Major
      challenges arise from modeling the radiative transfer in an
      aerosol and cloud particle loaded atmosphere, and from
      overcoming the lack of a priori knowledge of the targeted
      trace gas vertical distribution (e.g., unknown tropospheric
      BrO vertical distribution). Here, those challenges are tackled
      by a mathematical inversion of tropospheric trace gas profiles
      using a regularization approach constrained by a retrieved
      vertical profile of the aerosols extinction coefficient
      &lt;i&gt;&amp;epsilon;&lt;/i&gt;&lt;sub&gt;&lt;i&gt;M&lt;/i&gt;&lt;/sub&gt;. The validity and limitations of the algorithm
      are tested with in situ measured  &lt;i&gt;ε&lt;/i&gt;&lt;sub&gt;&lt;i&gt;M&lt;/i&gt;&lt;/sub&gt;, and with an
      absorber of known vertical profile (O&lt;sub&gt;4&lt;/sub&gt;). The method is
      then used for retrieving vertical profiles of tropospheric
      BrO. Results indicate that, for aircraft ascent/descent
      observations, the limit for the BrO detection is roughly
      1.5 pptv (pmol/mol), and the BrO profiles inferred from the
      boundary layer up to the upper troposphere and lower
      stratosphere have around 10 degrees of freedom.
&lt;br&gt;&lt;/br&gt;
      For the ASTAR 2007 deployments during ODEs, the retrieved BrO
      vertical profiles consistently indicate high BrO mixing ratios
      (~15 pptv) within the boundary layer, low BrO mixing
      ratios (&amp;le;1.5 pptv) in the free troposphere, occasionally
      enhanced BrO mixing ratios (~1.5 pptv) in the upper
      troposphere, and increasing BrO mixing ratios with altitude in
      the lowermost stratosphere. These findings are well in
      agreement with satellite and balloon-borne soundings of total
      and partial BrO atmospheric column densities.</description><dc:date>2010-08-30T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3907/2010/"><title>Ceilometer-lidar inter-comparison: backscatter coefficient retrieval and  signal-to-noise ratio determination</title><link>http://www.atmos-meas-tech-discuss.net/3/3907/2010/</link><description>&lt;b&gt;Ceilometer-lidar inter-comparison: backscatter coefficient retrieval and  signal-to-noise ratio determination&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3907-3924, 2010&lt;br /&gt;&lt;br /&gt;Author(s): B. Heese, H. Flentje, D. Althausen, A. Ansmann, and S. Frey&lt;br /&gt;&lt;br /&gt;The potential of a new generation of ceilometer
instruments for aerosol monitoring has been studied in the
Ceilometer-Lidar Inter- Comparison (CLIC) study. The ceilometer is
of type CHM15k from Jenoptik, Germany, which uses a solid state
laser at the wavelength of 1064 nm and an avalanche photodiode for
photon counting detection. The German Meteorological Service is in
progress of setting up a ceilometer network for aerosol monitoring
in Germany. The intercomparison study was performed to determine
whether the ceilometers are capable to deliver quality assured
particle backscatter coefficient profiles. For this, the derived
ceilometer profiles were compared to simultaneously measured lidar
profiles at the same wavelength. The lidar used for this
intercomparison was IfTs multi-wavelengths Raman lidar Polly&lt;sup&gt;&lt;i&gt;XT&lt;/i&gt;&lt;/sup&gt;.
During the EARLINET lidar intercomparison campaign EARLI 09 in
Leipzig, Germany, a new type of the Jenoptik ceilometer, the
CHM15k-X, took part. This new ceilometer has a new optical setup
resulting in a complete overlap at 150 m. The derived particle
backscatter profiles were compared to profiles derived from
Polly&lt;sup&gt;&lt;i&gt;XT&lt;/i&gt;&lt;/sup&gt;s measurements, too. The elastic daytime particle
backscatter profiles as well as the less noisy night-time Raman
particle backscatter profiles compare well with the ceilometers
profiles in atmospheric structures like aerosol layers or the
boundary layer top height. The calibration of the ceilometer
profiles by an independent measurement of the aerosol optical depth
(AOD) by a sun photometer is necessary to determine the correct
magnitude of the particle backscatter coefficient profiles. A
comprehensive signal-to-noise ratio study was carried out to
characterize the ceilometers signal performance with increasing
altitude.</description><dc:date>2010-08-30T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3877/2010/"><title>Retrieval of macrophysical cloud parameters from MIPAS: algorithm description and preliminary validation</title><link>http://www.atmos-meas-tech-discuss.net/3/3877/2010/</link><description>&lt;b&gt;Retrieval of macrophysical cloud parameters from MIPAS: algorithm description and preliminary validation&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3877-3906, 2010&lt;br /&gt;&lt;br /&gt;Author(s): J. Hurley, A. Dudhia, and R. G. Grainger&lt;br /&gt;&lt;br /&gt;The Michelson Interferometer for Passive Atmospheric Sounding
      (MIPAS) onboard ENVISAT has the potential to be particularly
      useful for studying high, thin clouds, which have been
      difficult to observe in the past. This paper details the
      development, implementation and testing of an
      optimal-estimation-type retrieval for three macrophysical
      cloud parameters (cloud top height, cloud top temperature and
      cloud extinction coefficient) from infrared spectra measured
      by MIPAS, employing additional information derived to improve
      the choice of a priori. The retrieval is applied and initially
      validated on MIPAS data. From application to MIPAS data, the
      retrieved cloud top heights are assessed to be accurate to
      within 50 m, the cloud top temperatures to within 0.5 K and
      extinction coefficients to within a factor of 15%. This
      algorithm has been adopted by the European Space Agency's
      ''MIPclouds'' project, which itself recognises the
      potential of MIPAS beyond monitoring atmospheric chemistry and
      seeks to study clouds themselves rigorously using MIPAS.</description><dc:date>2010-08-26T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3851/2010/"><title>Dry deposition of NaCl aerosols: theory and method for a modified leaf-washing technique</title><link>http://www.atmos-meas-tech-discuss.net/3/3851/2010/</link><description>&lt;b&gt;Dry deposition of NaCl aerosols: theory and method for a modified leaf-washing technique&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3851-3876, 2010&lt;br /&gt;&lt;br /&gt;Author(s): A. Reinap, B. L. B. Wiman, S. Gunnarsson, and B. Svenningsson&lt;br /&gt;&lt;br /&gt;Within the framework of aerosol deposition to vegetation we present
      a specially designed leaf wash-off method used in a wind-tunnel based
      study, where leaves of &lt;i&gt;Quercus robur&lt;/i&gt; L. were exposed to NaCl
      aerosols. We summarise the principles and illustrate the method for
      two types of substances, the chloride ion and the sodium ion, and for
      two levels of aerosol exposure prior to leaf washing. On the average,
      in the low-exposure experiments (S1), the 1st (2nd) wash-off step
      provided 90% (96%) of the amount of Cl&lt;sup&gt;&amp;minus;&lt;/sup&gt; on the leaves. In
      the high-exposure experiments (S2) the corresponding values were
      96% and 99%. For sodium, the general dynamics resembles that of
      chloride, but the amounts washed off were, in both series, on the
      average below what would be expected if the equivalent ratio in the
      tunnel aerosol were to be preserved. Na&lt;sup&gt;+&lt;/sup&gt; showed adsorption
      and/or absorption at the leaf surfaces. The difference between the
      mean values of the amounts of chloride and of sodium washed off in S1
      was not statistically significant, the mean Na&lt;sup&gt;+&lt;/sup&gt; to Cl&lt;sup&gt;&amp;minus;&lt;/sup&gt;
      difference as a fraction of Cl&lt;sup&gt;&amp;minus;&lt;/sup&gt; being minus 18%±27%;
      corresponding values for S2 were minus 16%±9%, however
      (&lt;i&gt;p&lt;/i&gt;&lt;0.05). In the latter case, 101±57 μequiv
      Na&lt;sup&gt;+&lt;/sup&gt; per m&lt;sup&gt;2&lt;/sup&gt; of leaf area were missing for the equivalent
      relationship 1:1 with Cl&lt;sup&gt;&amp;minus;&lt;/sup&gt; to be met. Although uncertainties are
      thus large, this indicates the magnitude of the
      Na&lt;sup&gt;+&lt;/sup&gt;-retention. The method is suitable not only for chloride,
      an inexpensive and easy-to-handle tracer, but also for sodium under
      exposure at high aerosol concentrations. Our findings will help design
      further studies of aerosol/forest interactions.</description><dc:date>2010-08-25T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3803/2010/"><title>In situ detection of atomic and molecular iodine using resonance and off-resonance fluorescence by lamp excitation: ROFLEX</title><link>http://www.atmos-meas-tech-discuss.net/3/3803/2010/</link><description>&lt;b&gt;In situ detection of atomic and molecular iodine using resonance and off-resonance fluorescence by lamp excitation: ROFLEX&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3803-3849, 2010&lt;br /&gt;&lt;br /&gt;Author(s): J. C. Gómez Martín, J. Blahins, U. Gross, T. Ingham, A. Goddard, A. S. Mahajan, A. Ubelis, and A. Saiz-Lopez&lt;br /&gt;&lt;br /&gt;We demonstrate a new instrument for in situ detection of atmospheric
      iodine atoms and molecules based on atomic and molecular resonance and
      off-resonance ultraviolet fluorescence excited by lamp emission. The
      instrument combines the robustness, light weight, low power
      consumption and efficient excitation of radio-frequency discharge
      light sources with the high sensitivity of the photon counting
      technique. Calibration of I&lt;sub&gt;2&lt;/sub&gt; fluorescence is achieved via
      quantitative detection of the molecule by incoherent broad band
      cavity-enhanced absorption spectroscopy. Atomic iodine fluorescence
      signal is calibrated by controlled broad band photolysis of known
      I&lt;sub&gt;2&lt;/sub&gt; concentrations in the visible spectral range at atmospheric
      pressure. The instrument has been optimised in laboratory experiments
      to reach detection limits of 1.2 pptv for I atoms and 20 pptv for
      I&lt;sub&gt;2&lt;/sub&gt;, for S/N=1 and 10 min of integration time. The ROFLEX
      system has been deployed in a field campaign in Northern Spain,
      representing the first concurrent observation of ambient mixing ratios
      of iodine atoms and molecules in the 1–350 pptv range.</description><dc:date>2010-08-25T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3747/2010/"><title>A new optimal estimation retrieval scheme for carbon monoxide using IASI  spectral radiances – Part 1: Sensitivity analysis, error budget and simulations</title><link>http://www.atmos-meas-tech-discuss.net/3/3747/2010/</link><description>&lt;b&gt;A new optimal estimation retrieval scheme for carbon monoxide using IASI  spectral radiances – Part 1: Sensitivity analysis, error budget and simulations&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3747-3802, 2010&lt;br /&gt;&lt;br /&gt;Author(s): S. M. Illingworth, J. J. Remedios, H. Boesch, D. P. Moore, H. Sembhi, A. Dudhia, and J. C. Walker&lt;br /&gt;&lt;br /&gt;This paper presents a new retrieval scheme for tropospheric
      carbon monoxide (CO), using measured radiances from the
      Infrared Atmospheric Sounding Interferometer (IASI) onboard
      the MetOp-A  satellite. The University of Leicester IASI
      Retrieval Scheme (ULIRS) is an optimal estimation retrieval
      scheme, which utilises equidistant pressure levels and
      a floating pressure grid based on topography. It makes use of
      explicit digital elevation and emissivity information, and
      incorporates a correction for solar surface reflection in the
      daytime with a high resolution solar spectrum. The retrieval
      scheme has been assessed through a formal error analysis, via
      the simulation of surface effects and by an application to
      real IASI data over a region in Southern Africa. The ULIRS
      enables the retrieval of between 1 and 2 pieces of
      information about the tropospheric CO vertical profiles, with
      peaks in the sensitivity at approximately 5 and
      12 km. Typical errors for the African region relating to the
      profiles are found to be ~20% at 5 and 12 km, and on
      the total columns to range from 18 to 34%. Finally the
      performance of the ULIRS is shown for a range of simulated
      geophysical conditions.</description><dc:date>2010-08-24T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3725/2010/"><title>Laboratory evaluation of the effect of nitric acid uptake on frost  point hygrometer performance</title><link>http://www.atmos-meas-tech-discuss.net/3/3725/2010/</link><description>&lt;b&gt;Laboratory evaluation of the effect of nitric acid uptake on frost  point hygrometer performance&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3725-3745, 2010&lt;br /&gt;&lt;br /&gt;Author(s): T. Thornberry, T. Gierczak, R. S. Gao, H. Vömel, L. A. Watts, J. B. Burkholder, and D. W. Fahey&lt;br /&gt;&lt;br /&gt;Chilled mirror hygrometers (CMH) are widely used to measure water
      vapour in the troposphere and lower stratosphere from balloon-borne
      sondes. Systematic discrepancies among in situ water vapour
      instruments have been observed at low water vapour mixing ratios
      (&lt;5 ppm) in the upper troposphere and lower stratosphere
      (UT/LS). Understanding the source of the measurement discrepancies is
      important for a more accurate and reliable determination of water
      vapour abundance in this region. We have conducted a laboratory study
      to investigate the potential interference of gas-phase nitric acid
      (HNO&lt;sub&gt;3&lt;/sub&gt;) with the measurement of frost point temperature, and
      consequently the water vapour mixing ratio, determined by CMH under
      conditions representative of operation in the UT/LS. No detectable
      interference in the measured frost point temperature was found for
      HNO&lt;sub&gt;3&lt;/sub&gt; mixing ratios of up to 4 ppb for exposure times
      up to 150 min. HNO&lt;sub&gt;3&lt;/sub&gt; was observed to co-condense on
      the mirror frost, with the adsorbed mass increasing linearly with time
      at constant exposure levels. Over the duration of a typical balloon
      sonde ascent (90–120 min), the maximum accumulated
      HNO&lt;sub&gt;3&lt;/sub&gt; amounts were comparable to monolayer coverage of the
      geometric mirror surface area, which corresponds to only a small
      fraction of the actual frost layer surface area. This small amount of
      co-condensed HNO&lt;sub&gt;3&lt;/sub&gt; is consistent with the observed lack of
      HNO&lt;sub&gt;3&lt;/sub&gt; interference in the frost point measurement because the
      CMH utilizes significant reductions (&gt;10%) in surface
      reflectivity by the condensate to determine H&lt;sub&gt;2&lt;/sub&gt;O.</description><dc:date>2010-08-24T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3675/2010/"><title>Absolute accuracy and sensitivity analysis of OP-FTIR retrievals of CO&lt;sub&gt;2&lt;/sub&gt;, CH&lt;sub&gt;4&lt;/sub&gt; and CO over concentrations representative of ''clean air'' and ''polluted plumes''</title><link>http://www.atmos-meas-tech-discuss.net/3/3675/2010/</link><description>&lt;b&gt;Absolute accuracy and sensitivity analysis of OP-FTIR retrievals of CO&lt;sub&gt;2&lt;/sub&gt;, CH&lt;sub&gt;4&lt;/sub&gt; and CO over concentrations representative of ''clean air'' and ''polluted plumes''&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3675-3723, 2010&lt;br /&gt;&lt;br /&gt;Author(s): T. E. L. Smith, M. J. Wooster, M. Tattaris, and D. W. T. Griffith&lt;br /&gt;&lt;br /&gt;When compared to established point-sampling methods, Open-Path Fourier
      Transform Infrared (OP-FTIR) spectroscopy can provide path-integrated
      concentrations of multiple gases simultaneously, in situ and
      near-continuously. Concentrations can be retrieved from the measured
      IR spectra using a forward model coupled to a non-linear least squares
      fitting procedure, without requiring ''background'' spectral
      measurements unaffected by the gases of interest. However, few studies
      have investigated the accuracy of such retrievals for CO&lt;sub&gt;2&lt;/sub&gt;,
      CH&lt;sub&gt;4&lt;/sub&gt; and CO, particularly across a broad concentration range
      covering ambient to highly polluted air (e.g. from biomass burning or
      industrial plumes). Here we perform such an assessment using data
      collected by a field-portable FTIR spectrometer. The FTIR was
      positioned to view a fixed IR source placed at the other end of an
      IR-transparent cell filled with the gases of interest, whose target
      concentrations were varied by up to two orders of
      magnitude. Retrievals made using the forward model are complicated by
      absorption line pressure broadening, the effects of temperature on
      absorption band shape and by convolution of the gas absorption lines
      and the instrument line shape (ILS). Despite this, with optimal
      forward model parameterisation (i.e. the wavenumber range used in the
      retrieval, gas temperature, pressure and ILS), concentration
      retrievals for all gases were able to be made to within 5% of the
      true value. Sensitivity to the aforementioned model inputs was also
      investigated. CO retrievals were shown to be most sensitive to the ILS
      (a function of the assumed instrument FOV), which is due to the
      narrow nature of CO absorption lines and their consequent sensitivity
      to convolution with the ILS. Conversely, CO&lt;sub&gt;2&lt;/sub&gt; retrievals were
      most sensitive to assumed atmospheric parameters, particularly
      temperature. The analysis suggests that trace gas concentration
      retrieval errors can remain well below 10%, even with the
      uncertainties in atmospheric pressure and temperature that might arise
      when studying plumes in field situations (e.g. at uncertain altitudes
      or temperatures). Our findings provide confidence that FTIR-derived
      trace gas retrievals of CO&lt;sub&gt;2&lt;/sub&gt;, CH&lt;sub&gt;4&lt;/sub&gt; and CO based on
      forward modeling can yield accurate results, even over very large
      concentration ranges that can prove difficult to retrieve via standard
      classical least squares (CLS) techniques.</description><dc:date>2010-08-23T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3643/2010/"><title>Aerosol profiling using the ceilometer network of the German Meteorological Service</title><link>http://www.atmos-meas-tech-discuss.net/3/3643/2010/</link><description>&lt;b&gt;Aerosol profiling using the ceilometer network of the German Meteorological Service&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3643-3673, 2010&lt;br /&gt;&lt;br /&gt;Author(s): H. Flentje, B. Heese, J. Reichardt, and W. Thomas&lt;br /&gt;&lt;br /&gt;The German Meteorological Service (DWD) operates about 52 lidar ceilometers
within its synoptic observations network, covering Germany. These affordable
low-power lidar systems provide spatially and temporally high resolved
aerosol backscatter profiles which can operationally provide quasi 3-D
distributions of particle backscatter intensity. Intentionally designed for
cloud height detection, recent significant improvements allow following the
development of the boundary layer and to detect denser particle plumes in the
free tropospere like volcanic ash, Saharan dust or fire smoke. Thus the
network builds a powerful aerosol plume alerting and tracking system. If
auxiliary aerosol information is available, the particle backscatter
coefficient, the extinction coefficient and even particle mass concentrations
may be estimated, with however large uncertainties. Therefore, large
synergistic benefit is achieved if the ceilometers are linked to existing
lidar networks like EARLINET or integrated into WMO's envisioined Global
Aerosol Lidar Observation Network GALION. To this end, we demonstrate the
potential and limitations of ceilometer networks by means of three
representative aerosol episodes over Europe, namely Sahara dust,
Mediterranean fire smoke and, more detailed, the Icelandic Eyjafjoll volcano
eruption from mid April 2010 onwards. The DWD (Jenoptik CHM15k) lidar
ceilometer network tracked the Eyjafjoll ash layers over Germany and roughly
estimated peak extinction coefficients and mass concentrations on 17 April of
4–6(± 2) 10&lt;sup&gt;-4&lt;/sup&gt; m&lt;sup&gt;−1&lt;/sup&gt; and
500–750(± 300) μg/m&lt;sup&gt;−3&lt;/sup&gt;, respectively, based on co-located
aerosol optical depth, nephelometer (scattering coefficient) and particle
mass concentration measurements. Though large, the uncertainties are small
enough to let the network suit for example as aviation advisory tool,
indicating whether the legal flight ban threshold of presently 2 mg/m&lt;sup&gt;3&lt;/sup&gt;
is imminent to be exceeded.</description><dc:date>2010-08-23T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3601/2010/"><title>Synergetic cloud fraction determination for SCIAMACHY using MERIS</title><link>http://www.atmos-meas-tech-discuss.net/3/3601/2010/</link><description>&lt;b&gt;Synergetic cloud fraction determination for SCIAMACHY using MERIS&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3601-3642, 2010&lt;br /&gt;&lt;br /&gt;Author(s): C. Schlundt, A. A. Kokhanovsky, W. von Hoyningen-Huene, T. Dinter, L. Istomina, and J. P. Burrows&lt;br /&gt;&lt;br /&gt;Since clouds play an essential role in the Earth's climate system,
it is important to understand the cloud characteristics as well as
their distribution on a global scale using satellite observations.
The main scientific objective of SCIAMACHY
(SCanning Imaging Absorption spectroMeter for Atmospheric CHartographY)
onboard the ENVISAT satellite is the retrieval of vertical columns of
trace gases.



&lt;br&gt;&lt;br&gt;

On the one hand, SCIAMACHY has to be sensitive to low variations in
trace gas concentrations which means the ground pixel size has to be large enough.
On the other hand, such a large pixel size leads to the problem that
SCIAMACHY spectra are often contaminated by clouds. SCIAMACHY spectral
measurements are not well suitable to derive a reliable sub-pixel cloud fraction
that can be used as input parameter for subsequent retrievals of cloud
properties or vertical trace gas columns.
Therefore, we use MERIS/ENVISAT spectral measurements
with its high spatial resolution
as sub-pixel information for the determination of
MerIs Cloud fRation fOr Sciamachy (MICROS).
Since MERIS covers an even broader swath width than SCIAMACHY,
no problems in spatial and temporal collocation of measurements occur.
This enables the derivation of a SCIAMACHY cloud fraction with an accuracy
much higher as compared with other current cloud fractions that are based
on SCIAMACHY's PMD (Polarization Measurement Device) data.



&lt;br&gt;&lt;br&gt;

We present our new developed MICROS algorithm, based on the threshold approach,
as well as a qualitative validation of our results
with MERIS satellite images for different locations, especially
with respect to bright surfaces such as snow/ice and sands.
In addition, the SCIAMACHY cloud fractions derived from MICROS are intercompared
with other current SCIAMACHY cloud fractions based on different approaches
demonstrating a considerable improvement regarding
geometric cloud fraction determination using the MICROS algorithm.</description><dc:date>2010-08-19T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3535/2010/"><title>Determination of aerosol properties from satellite observations of the Ring effect</title><link>http://www.atmos-meas-tech-discuss.net/3/3535/2010/</link><description>&lt;b&gt;Determination of aerosol properties from satellite observations of the Ring effect&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3535-3599, 2010&lt;br /&gt;&lt;br /&gt;Author(s): T. Wagner, S. Beirle, T. Deutschmann, and M. P. de Vries&lt;br /&gt;&lt;br /&gt;In this study we explore the potential of satellite observations of the Ring effect (at
      various wavelengths) for the retrieval of atmospheric aerosol properties. Compared to
      clouds, aerosols have a rather weak influence on the Ring effect, thus the requirements on
      the accuracy of the measurements and the radiative transfer simulations are high. In this
      study, we show that for moderate and high aerosol optical depth (AOD), Ring effect
      observations are sensitive enough to yield information not only on the AOD, but also on the
      absorbing properties of aerosols and the aerosol layer height. The latter two quantities are
      especially important for the determination of the radiative effects of aerosols.
&lt;br&gt;&lt;br&gt;
      Our investigations are based on observations by the satellite instrument SCIAMACHY on
      ENVISAT (2004–2008) and on model simulations using the Monte-Carlo radiative transfer model
      McArtim. In addition to the Ring effect we investigate the impact of aerosols on the
      absorptions of the oxygen molecule (O&lt;sub&gt;2&lt;/sub&gt;) and dimer (O&lt;sub&gt;4&lt;/sub&gt;) as well as the
      radiance. In general good consistency between measured and simulated quantities is found. In
      some cases also systematic differences occurred, which are probably mainly related to the
      strong polarisation sensitivity of the SCIAMACHY instrument.
&lt;br&gt;&lt;br&gt;
      Our study indicates that Ring effect observations have important advantages for aerosol
      retrievals: in contrast to O&lt;sub&gt;2&lt;/sub&gt; and O&lt;sub&gt;4&lt;/sub&gt; absorptions they are only weakly
      affected by the surface albedo; they can be analysed with high accuracy in various
      wavelength ranges; and depending on the wavelength range, they show different sensitivities
      on aerosol properties like single scattering albedo, optical depth or layer height. The
      results of this study are of particular interest for future satellite instruments with
      reduced polarisation sensitivity and smaller ground pixels, capable of measuring the Ring
      effect with higher accuracy.</description><dc:date>2010-08-19T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3489/2010/"><title>A geostationary thermal infrared sensor to monitor the lowermost troposphere: O&lt;sub&gt;3&lt;/sub&gt; and CO retrieval studies</title><link>http://www.atmos-meas-tech-discuss.net/3/3489/2010/</link><description>&lt;b&gt;A geostationary thermal infrared sensor to monitor the lowermost troposphere: O&lt;sub&gt;3&lt;/sub&gt; and CO retrieval studies&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3489-3534, 2010&lt;br /&gt;&lt;br /&gt;Author(s): M. Claeyman, J.-L. Attié, V.-H. Peuch, L. El Amraoui, W. A. Lahoz, B. Josse, P. Ricaud, T. von Clarmann, M. Höpfner, J. Orphal, J.-M. Flaud, D. P. Edwards, K. Chance, X. Liu, F. Pasternak, and R. Cantié&lt;br /&gt;&lt;br /&gt;This paper describes the capabilities of a nadir thermal infrared (TIR)
sensor proposed for embarkation onboard a geostationary platform to monitor
ozone (O&lt;sub&gt;3&lt;/sub&gt;) and carbon monoxide (CO) for air quality (AQ) purposes. To
assess the capabilities of this sensor we perform idealized retrieval studies
considering typical atmospheric profiles of O&lt;sub&gt;3&lt;/sub&gt; and CO over Europe with
different instrument configurations (signal to noise ratio and spectral
sampling interval) using the KOPRA forward model and the KOPRA-fit retrieval
scheme based on the Tikhonov-Phillips regularization. We then select a
configuration, referred to as GEO-TIR, optimized for providing information in
the lowermost troposphere (LmT; 0–3 km in height). For the GEO-TIR
configuration we obtain around 1.5 degrees of freedom for O&lt;sub&gt;3&lt;/sub&gt; and 2 for CO
at altitudes between 0 and 15 km. The error budget of GEO-TIR, calculated
taking account of the principal contributions to the error (namely,
temperature, measurement error, smoothing error) shows that information in
the LmT can be achieved by GEO-TIR. We also retrieve analogous profiles from
another geostationary infrared instrument with characteristics similar to the
Meteosat Third Generation Infrared Sounder (MTG-IRS) which is dedicated to
numerical weather prediction, referred to as GEO-TIR2. Comparison between
GEO-TIR and GEO-TIR2 allows us to quantify the added value of GEO-TIR, a
mission complementing the AQ observing system. To better characterize the
information provided by GEO-TIR and GEO-TIR2 in the LmT, we retrieve two
typical profiles of O&lt;sub&gt;3&lt;/sub&gt; and CO for different thermal contrast ranging from
–10 K to 10 K. The shape of the first averaging kernel (corresponding to
the surface level) confirms that GEO-TIR has good sensitivity to CO in the
LmT and also to O&lt;sub&gt;3&lt;/sub&gt; for high positive thermal contrast. GEO-TIR2 has very
low sensitivity in the LmT to O&lt;sub&gt;3&lt;/sub&gt; but can have sensitivity to CO with high
positive thermal contrast. To quantify these results for a realistic
atmosphere, we simulate it using the chemical transport model MOCAGE
(MOdèle de Chimie Atmospherique à Grande Echelle) – this is the
nature run. We simulate the O&lt;sub&gt;3&lt;/sub&gt; and CO spatial and temporal distributions
from GEO-TIR observations in the LmT in July 2009 over Europe by sampling the
nature run. Results show that GEO-TIR is able to capture well the
spatial and temporal variability in the LmT for both O&lt;sub&gt;3&lt;/sub&gt; and CO,
particularly during periods with high positive thermal contrast near the
ground and high surface temperature, which results in active photochemistry
and a raised planetary boundary layer. These results also provide evidence of
the significant added value in the LmT of GEO-TIR compared to GEO-TIR2 by
showing GEO-TIR is closer to the nature run than GEO-TIR2 for various
statistical parameters (correlation, bias, standard deviation).</description><dc:date>2010-08-18T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3455/2010/"><title>Fine-scale turbulence soundings in the stratosphere with the new balloon-borne instrument LITOS</title><link>http://www.atmos-meas-tech-discuss.net/3/3455/2010/</link><description>&lt;b&gt;Fine-scale turbulence soundings in the stratosphere with the new balloon-borne instrument LITOS&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3455-3487, 2010&lt;br /&gt;&lt;br /&gt;Author(s): A. Theuerkauf, M. Gerding, and F.-J. Lübken&lt;br /&gt;&lt;br /&gt;We have developed a new compact balloon payload called LITOS
(Leibniz-Institute Turbulence Observations in the Stratosphere) for high
resolution wind turbulence soundings up to 35 km altitude. The wind
measurements are performed applying a constant temperature anemometer (CTA)
with a vertical resolution of ~2.5 mm, i.e. 2 kHz sampling rate at
5 m/s ascent speed. Thereby, for the first time, it is possible to study the
entire turbulence spectrum down to the viscous subrange in the stratosphere.
Including telemetry, housekeeping, batteries and recovery unit the payload
weighs less than 5 kg and can be launched at any radiosonde station. Since
autumn 2007 LITOS has been successfully launched several times from the
Leibniz-Institute of Atmospheric Physics (IAP) in Kühlungsborn, Germany
(54° N, 12° E). Two additional soundings were carried out in
2008 and 2009 at Kiruna, Sweden (67° N, 21° E) as part of the
BEXUS program (Balloon-borne EXperiments for University Students). We
describe here the basic principle of CTA measurements and prove the validity
of this method in the stratosphere. First case studies allow a clear
distinction between non-turbulent layers and turbulent layers with a
thickness of some tens of meters. Since our measurements cover the transition
between the inertial and viscous subrange, energy dissipation rates can be
calculated with high reliability.</description><dc:date>2010-08-18T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3425/2010/"><title>Evaluating the assumptions of surface reflectance and aerosol type selection within the MODIS aerosol retrieval over land: the problem of dust type selection</title><link>http://www.atmos-meas-tech-discuss.net/3/3425/2010/</link><description>&lt;b&gt;Evaluating the assumptions of surface reflectance and aerosol type selection within the MODIS aerosol retrieval over land: the problem of dust type selection&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3425-3453, 2010&lt;br /&gt;&lt;br /&gt;Author(s): T. Mielonen, R. C. Levy, V. Aaltonen, M. Komppula, G. de Leeuw, J. Huttunen, H. Lihavainen, P. Kolmonen, K. E. J. Lehtinen, and A. Arola&lt;br /&gt;&lt;br /&gt;Aerosol Optical Depth (AOD) and Ångström exponent (AE)
      values derived with the MODIS retrieval algorithm over land
      (Collection 5) were compared with ground based sun photometer
      measurements in Europe, Asia, Africa, North America and South
      America.  In Finland (Jokioinen and Sodankylä)
      measurements were done with Precision Filter Radiometer (PFR),
      while in Estonia (Toravere), Italy (Ispra, Rome Tor Vergata),
      India (Kanpur), China (Xianghe), GSFC (USA), Mexico (Mexico
      City), Zambia (Mongu) and Brazil (Alta Floresta) Cimel
      (AERONET, level 2) measurements were used. Comparison results
      for AOD were generally good, although there seems to be room
      for improvement in the MODIS aerosol model selection,
      particularly how dust is taken into account. At all studied
      sites, the MODIS algorithm often selects the dust aerosol
      model even when dust does not seem to be present and the air
      masses are not coming from arid regions. This happens
      especially when AOD values are relatively small (&lt;0.3). The selection of the dust model reduces the correlation
      between ground based and MODIS AOD measurements in dust-free
      situations. Moreover, the current aerosol model selection
      scheme produces unphysical AE values. Our study suggests that
      the aerosol model combining is sensitive to the ratio of
      660 nm and 2130 nm surface reflectances
      (slope(660/2130)). Furthermore, the value of the slope in the
      algorithm is mainly dependent on the Normalized Difference
      Vegetation Index (NDVI). The current relationship of these two
      parameters in the algorithm is not supported by the surface
      albedo climatology derived from MODIS measurements. The use of
      a more physical relationship improves the AE retrieval at the
      studied sites. However, at some sites the AOD correspondence
      deteriorates when the new relationship is used.</description><dc:date>2010-08-17T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3383/2010/"><title>Intercomparison of slant column measurements of NO&lt;sub&gt;2&lt;/sub&gt; and O&lt;sub&gt;4&lt;/sub&gt; by MAX-DOAS and zenith-sky UV and visible  spectrometers</title><link>http://www.atmos-meas-tech-discuss.net/3/3383/2010/</link><description>&lt;b&gt;Intercomparison of slant column measurements of NO&lt;sub&gt;2&lt;/sub&gt; and O&lt;sub&gt;4&lt;/sub&gt; by MAX-DOAS and zenith-sky UV and visible  spectrometers&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3383-3423, 2010&lt;br /&gt;&lt;br /&gt;Author(s): H. K. Roscoe, M. Van Roozendael, C. Fayt, A. du Piesanie, N. Abuhassan, C. Adams, M. Akrami, A. Cede, J. Chong, K. Clémer, U. Friess, M. Gil Ojeda, F. Goutail, R. Graves, A. Griesfeller, K. Grossmann, G. Hemerijckx, F. Hendrick, J. Herman, C. Hermans, H. Irie, P. V. Johnston, Y. Kanaya, K. Kreher, R. Leigh, A. Merlaud, G. H. Mount, M. Navarro, H. Oetjen, A. Pazmino, M. Perez-Camacho, E. Peters, G. Pinardi, O. Puentedura, A. Richter, A. Schönhardt, R. Shaiganfar, E. Spinei, K. Strong, H. Takashima, T. Vlemmix, M. Vrekoussis, T. Wagner, F. Wittrock, M. Yela, S. Yilmaz, F. Boersma, J. Hains, M. Kroon, and A. Piters&lt;br /&gt;&lt;br /&gt;In June 2009, 22 spectrometers from 14 institutes measured
      tropospheric and stratospheric NO&lt;sub&gt;2&lt;/sub&gt; from the ground for more than
      11 days during the Cabauw Intercomparison campaign of Nitrogen Dioxide
      measuring Instruments (CINDI), at Cabauw, NL (51.97° N,
      4.93° E). All visible instruments used a common wavelength
      range and set of cross sections for the spectral analysis. Most of the
      instruments were of the multi-axis design with analysis by
      differential spectroscopy software (MAX-DOAS), whose non-zenith slant
      columns were compared by examining slopes of their least-squares
      straight line fits to mean values of a selection of instruments, after
      taking 30-min averages. Zenith slant columns near twilight were
      compared by fits to interpolated values of a reference instrument,
      then normalised by the mean of the slopes of the best instruments. For
      visible MAX-DOAS instruments, the means of the fitted slopes for
     NO&lt;sub&gt;2&lt;/sub&gt; and O&lt;sub&gt;4&lt;/sub&gt; of all except one instrument were within 10%
      of unity at almost all non-zenith elevations, and most were within
      5%. Values for UV MAX-DOAS instruments were almost as good, being
      12% and 7%, respectively. For visible instruments at zenith near
      twilight, the means of the fitted slopes of all instruments were
      within 5% of unity. This level of agreement is as good as that of previous intercomparisons, despite the site not being ideal for zenith twilight measurements. It bodes well for
      the future of measurements of tropospheric  NO&lt;sub&gt;2&lt;/sub&gt;, as previous
      intercomparisons were only for zenith instruments focussing on
      stratospheric  NO&lt;sub&gt;2&lt;/sub&gt;, with their longer heritage.</description><dc:date>2010-08-13T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3345/2010/"><title>Quantitative and enantioselective analysis of monoterpenes from plant chambers and in ambient air using SPME</title><link>http://www.atmos-meas-tech-discuss.net/3/3345/2010/</link><description>&lt;b&gt;Quantitative and enantioselective analysis of monoterpenes from plant chambers and in ambient air using SPME&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3345-3381, 2010&lt;br /&gt;&lt;br /&gt;Author(s): N. Yassaa, T. Custer, W. Song, F. Pech, J. Kesselmeier, and J. Williams&lt;br /&gt;&lt;br /&gt;A solid-phase microextraction (HS-SPME) and gas chromatography/mass
      spectrometry (GC/MS) system has been developed for quantifying
      enantiomeric and nonenantiomeric monoterpenes in plant chamber studies
      and ambient air. Performance of this system was checked using
      a capillary diffusion system to produce monoterpene standards. The
      adsorption efficiency, competitive adsorption and chromatographic
      peak resolution of monoterpene enantiomer pairs were compared
      for three SPME fibre coatings: 75 μm Carboxen-PDMS
      (CAR-PDMS), 50/30 μm,
      divinylbenzene-carboxen-polydimethylsiloxane (DVB-CAR-PDMS)
      and 65 μm divinylbenzene-polydimethyl-siloxane
      (DVB-PDMS). Key parameters such as the linearity and reproducibility
      of the SPME system have been investigated in this work. The best
      compromise between the enantiomeric separation of monoterpenes and
      competitive adsorption of the isoprenoids on the solid SPME fibre
      coating was found for DVB-PDMS fibres. The optimum conditions using
      DVB-PDMS fibres were applied to measure the exchange rates of
      monoterpenes in the emission of &lt;i&gt;Quercus ilex&lt;/i&gt; using
      a laboratory whole plant enclosure under light and dark conditions, as
      well as in ambient air. With 592 and 223 ng m&lt;sup&gt;−2&lt;/sup&gt; s&lt;sup&gt;−1&lt;/sup&gt;,
      respectively, &amp;beta;-myrcene and limonene were the predominant
      monoterpenes in the emission of &lt;i&gt;Q. ilex&lt;/i&gt;. These values were
      closely comparable to those obtained using a zNose and cartridge
      GC-FID systems.</description><dc:date>2010-08-09T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3319/2010/"><title>Intercomparison of CALIOP and MODIS aerosol optical depth retrievals</title><link>http://www.atmos-meas-tech-discuss.net/3/3319/2010/</link><description>&lt;b&gt;Intercomparison of CALIOP and MODIS aerosol optical depth retrievals&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3319-3344, 2010&lt;br /&gt;&lt;br /&gt;Author(s): C. Kittaka, D. M. Winker, M. A. Vaughan, A. Omar, and L. A. Remer&lt;br /&gt;&lt;br /&gt;The Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) is carried on
the CALIPSO satellite and has acquired global aerosol profiles since June 2006.
CALIPSO is flown in formation with the Aqua satellite as part of the
A-train satellite constellation, so that a large number of coincident
aerosol observations are available from CALIOP and the MODIS-Aqua
instrument. This study compares column aerosol optical depth at 0.532 μm
derived from CALIOP aerosol profiles with MODIS-Aqua 0.55 μm aerosol
optical depth over the period June 2006 through August 2008. The study is
based on the CALIOP Version 2 Aerosol Layer Product and MODIS Collection 5.
While CALIOP is first and foremost a profiling instrument, this comparison
of column aerosol optical depth provides insight into quality of CALIOP
aerosol data. It is found that daytime aerosol optical depth from the CALIOP
Version 2 product has a small global mean bias relative to MODIS Collection
5. Regional biases, of both signs, are larger and biases are seen to vary
somewhat with season. In northern mid-latitudes, aerosol optical depth from
CALIOP is lower, on average, than from MODIS. This may be partly due to a
latitude-dependent calibration error in Version 2 CALIOP Level 1 daytime
0.532 μm profiles. This comparison of CALIOP and MODIS also provides
insight into possible biases in the MODIS aerosol optical depth product due
to cloud masking and errors in modeling land surface reflectance.</description><dc:date>2010-08-09T00:00:00+02:00</dc:date></item><item rdf:about="http://www.atmos-meas-tech-discuss.net/3/3293/2010/"><title>Fast-response high-resolution temperature sonde  aimed at contamination-free profile observations</title><link>http://www.atmos-meas-tech-discuss.net/3/3293/2010/</link><description>&lt;b&gt;Fast-response high-resolution temperature sonde  aimed at contamination-free profile observations&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Measurement Techniques Discussions, 3, 3293-3317, 2010&lt;br /&gt;&lt;br /&gt;Author(s): K. Shimizu and F. Hasebe&lt;br /&gt;&lt;br /&gt;An innovative temperature sonde, equipped with an ultra thin tungsten
      wire, has been developed to meet the scientific requirements suitable
      for climate change research. The response time, shorter than
      40 ms achieved at the altitude of 30 km, enables the
      temperature observations with the radiation correction of less than
      0.4 K in the whole observation range. Test flights during the
      development stage reveal significant artificial perturbations in the
      observed temperature profiles. They are identified as the thermal
      contamination arising primarily from radiosonde package box with some
      additional effect from the launching balloon. The modification of the
      sensor mount successfully removed the contribution from the former
      effect. On the other hand, some filtering procedure need to be
      applied to remove the latter, although the use of a long suspension
      line will be effective to reduce the noise. There remain unavoidable
      small fluctuations (less than 0.4 K) that are brought about by
      the solid angle modulation of the illumination against the sensor body
      in the daytime. While conventional radiation correction may
      unintentionally have taken a part of such contaminations into account,
      they may not be properly corrected in existing radiosonde data, as the
      origin of errors has not been identified. Our tungsten sonde that
      scarcely relies on the ambiguous correction procedures is ideal for
      serving as an international reference.</description><dc:date>2010-08-06T00:00:00+02:00</dc:date></item></rdf:RDF>