Skip to main content

Index Geophysics

InterServer Web Hosting and VPS
InterServer Web Hosting and VPS

Items

Advanced search
  • Effects of dust storms on microwave radiation based on satellite observation and model simulation over the Taklamakan desert

    Effects of dust particles on microwave radiation over the Taklamakan desert are studied with use of measurements from the Advanced Microwave Scanning Radiometer (AMSR-E) on the EOS Aqua satellite and a microwave radiation transfer model. Eight observed cases show that the signal from atmospheric dust can be separated from the surface radiation by the fact that the dust particles produce stronger scattering at high frequencies and depolarize the background desert signature. This result of satellite data is consistent with the model simulation.
  • Twelve years of global observations of formaldehyde in the troposphere using GOME and SCIAMACHY sensors

    This work presents global tropospheric formaldehyde columns retrieved from near-UV radiance measurements performed by the GOME instrument onboard ERS-2 since 1995, and by SCIAMACHY, in operation on ENVISAT since the end of 2002. A special effort has been made to ensure the coherence and quality of the CH<sub>2</sub>O dataset covering the period 1996–2007. Optimised DOAS settings are proposed in order to reduce the impact of two important sources of error in the derivation of slant columns, namely, the polarisation anomaly affecting the SCIAMACHY spectra around 350 nm, and a major absorption band of the O<sub>4</sub> collision complex centred near 360 nm. The air mass factors are determined from scattering weights generated using radiative transfer calculations taking into account the cloud fraction, the cloud height and the ground albedo. Vertical profile shapes of CH<sub>2</sub>O are provided by the global CTM IMAGES based on an up-to-date representation of emissions, atmospheric transport and photochemistry. A comprehensive error analysis is presented. This includes errors on the slant columns retrieval and errors on the air mass factors which are mainly due to uncertainties in the a priori profile and in the cloud properties. The major features of the retrieved formaldehyde column distribution are discussed and compared with previous CH<sub>2</sub>O datasets over the major emission regions.
  • Aerosol direct radiative effect in the Po Valley region derived from AERONET measurements

    The aerosol direct radiative effect (ADRE) affecting the Po Valley and the adjacent North Adriatic Sea is studied using 10-year series of measurements collected at two AERONET sites located in the western part of the Valley (Ispra), and on a platform (AAOT) offshore Venice. This region is characterized by a high, mostly continental, aerosol load with comparable average aerosol optical thickness &tau;<sub>a</sub> at both locations (0.21 at 500 nm) and more absorbing aerosols at Ispra. A dynamic aerosol model accounting for the changes in scattering phase function with &tau;<sub>a</sub> is used for radiative transfer calculations, together with boundary conditions representative of terrestrial and marine surfaces. A sensitivity analysis allows the construction of an error budget for the daily ADRE estimates, found to be of the order of 20% and mostly due to uncertainties on aerosol single scattering albedo and &tau;<sub>a</sub>. The daily radiative efficiencies, normalized by &tau;<sub>a</sub> at 500 nm, increase from December to June, from &minus;17 to &minus;24 W m<sup>&minus;2</sup> &tau;<sub>a</sub><sup>&minus;1</sup> at top-of-atmosphere (TOA) and &minus;33 to &minus;72 W m<sup>&minus;2</sup> &tau;<sub>a</sub><sup>&minus;1</sup> at surface for the Po Valley, and from &minus;15 to &minus;32 (TOA) and &minus;35 to &minus;65 W m<sup>&minus;2</sup> &tau;<sub>a</sub><sup>&minus;1</sup> (surface) for the AAOT site. The average of log-transformed ADRE for TOA, surface and atmosphere are &minus;5.2, &minus;12.2 and +6.8 W m<sup>&minus;2</sup> for the Po Valley case, and &minus;6.5, &minus;13.0 and +6.5 W m<sup>&minus;2</sup> for the AAOT site but these values can be much higher for individual days. Concurrent clear-sky days give indications on the regional atmospheric heating spatial gradients. Differences between the atmospheric ADRE at the two locations average 6.3 W m<sup>&minus;2</sup> with a gradient positive towards the inner valley in 65% of the cases. This study confirms the importance of duly considering the radiative impact of aerosols on the regional climate.
  • The influence of natural and anthropogenic secondary sources on the glyoxal global distribution

    Glyoxal, the smallest dicarbonyl, which has recently been observed from space, is expected to provide indications on volatile organic compounds (VOC) oxidation and secondary aerosol formation in the troposphere. Glyoxal (CHOCHO) is known to be mostly of natural origin and is produced during biogenic VOC oxidation. However, a number of anthropogenically emitted hydrocarbons, like acetylene and aromatics, have been positively identified as CHOCHO precursors. The present study investigates the contribution of pollution to the CHOCHO levels by taking into account the secondary chemical formation of CHOCHO from precursors emitted from biogenic, anthropogenic and biomass burning sources. The impact of potential primary land emissions of CHOCHO is also investigated. A global 3-dimensional chemistry transport model of the troposphere (TM4-ECPL) able to simulate the gas phase chemistry coupled with all major aerosol components is used. <br><br> The secondary anthropogenic contribution from fossil fuel and industrial VOCs emissions oxidation to the CHOCHO columns is found to reach 20–70% in the industrialized areas of the Northern Hemisphere and 3–20% in the tropics. This secondary CHOCHO source is on average three times larger than that from oxidation of VOCs from biomass burning sources. The chemical production of CHOCHO is calculated to equal to about 56 Tg y<sup>&minus;1</sup> with 70% being produced from biogenic hydrocarbons oxidation, 17% from acetylene, 11% from aromatic chemistry and 2% from ethene and propene. CHOCHO is destroyed in the troposphere primarily by reaction with OH radicals (23%) and by photolysis (63%), but it is also removed from the atmosphere through wet (8%) and dry deposition (6%). Potential formation of secondary organic aerosol through CHOCHO losses on/in aerosols and clouds is neglected here due to the significant uncertainties associated with the underlying chemistry. The global annual mean CHOCHO burden and lifetime in the model domain are estimated to be 0.02 Tg (equal to the global burden seen by SCIAMACHY over land for the year 2005) and about 3 h, respectively. The model results are compared with satellite observations of CHOCHO columns. When accounting only for the secondary sources of CHOCHO in the model, the model underestimates CHOCHO columns observed by satellites. This is attributed to an overestimate of CHOCHO sinks or a missing global source of about 20 Tg y<sup>&minus;1</sup>. Using the current primary emissions of CHOCHO from biomass burning together with the anthropogenic combustion sources of about 7 Tg y<sup>&minus;1</sup> leads to an overestimate by the model over hot spot areas.
  • Laboratory studies of H2SO4/H2O binary homogeneous nucleation from the SO2+OH reaction: evaluation of the experimental setup and preliminary results

    Binary homogeneous nucleation (BHN) of sulphuric acid and water (H<sub>2</sub>SO<sub>4</sub>/H<sub>2</sub>O) is one of the most important atmospheric nucleation processes, but laboratory observations of this nucleation process are very limited and there are also large discrepancies between different laboratory studies. The difficulties associated with these experiments include wall loss of H<sub>2</sub>SO<sub>4</sub> and uncertainties in estimation of H<sub>2</sub>SO<sub>4</sub> concentration ([H<sub>2</sub>SO<sub>4</sub>]) involved in nucleation. We have developed a new laboratory nucleation setup to study H<sub>2</sub>SO<sub>4</sub>/H<sub>2</sub>O BHN kinetics and provide relatively constrained [H<sub>2</sub>SO<sub>4</sub>] needed for nucleation. H<sub>2</sub>SO<sub>4</sub> is produced from the SO<sub>2</sub>+OH→HSO<sub>3</sub> reaction and OH radicals are produced from water vapor UV absorption. The residual [H<sub>2</sub>SO<sub>4</sub>] were measured at the end of the nucleation reactor with a chemical ionization mass spectrometer (CIMS). Wall loss factors (WLFs) of H<sub>2</sub>SO<sub>4</sub> were estimated by assuming that wall loss is diffusion limited and these calculated WLFs were in good agreement with simultaneous measurements of the initial and residual [H<sub>2</sub>SO<sub>4</sub>] with two CIMSs. The nucleation zone was estimated from numerical simulations based on the measured aerosol sizes (particle diameter, <i>D</i><sub><i>p</i></sub>) and [H<sub>2</sub>SO<sub>4</sub>]. The measured BHN rates (<i>J</i>) ranged from 0.01–220 cm<sup>&minus;3</sup> s<sup>&minus;1</sup> at the initial and residual [H<sub>2</sub>SO<sub>4</sub>] from 10<sup>8</sup>&minus;10<sup>10</sup> cm<sup>&minus;3</sup>, a temperature of 288 K and relative humidity (RH) from 11–23%; <i>J</i> increased with increasing [H<sub>2</sub>SO<sub>4</sub>] and RH. <i>J</i> also showed a power dependence on [H<sub>2</sub>SO<sub>4</sub>] with the exponential power of 3–8. These power dependences are consistent with other laboratory studies under similar [H<sub>2</sub>SO<sub>4</sub>] and RH, but different from atmospheric field observations which showed that particle number concentrations are often linearly dependent on [H<sub>2</sub>SO<sub>4</sub>]. These results, together with a higher [H<sub>2</sub>SO<sub>4</sub>] threshold (10<sup>8</sup>–10<sup>9</sup> cm<sup>&minus;3</sup>) needed to produce the unit <i>J</i> measured from the laboratory studies compared to the atmospheric conditions (10<sup>6</sup>–10<sup>7</sup> cm<sup>&minus;3</sup>), imply that H<sub>2</sub>SO<sub>4</sub>/H<sub>2</sub>O BHN alone is insufficient to explain atmospheric aerosol formation and growth. Particle growth rates estimated from the measured aerosol size distributions, residence times (<i>t</i><sub><i>r</i></sub>), and [H<sub>2</sub>SO<sub>4</sub>] were 100–500 nm h<sup>&minus;1</sup>, much higher than those seen from atmospheric field observations, because of the higher [H<sub>2</sub>SO<sub>4</sub>] used in our study.
  • Source characteristics of volatile organic compounds during high ozone episodes in Hong Kong, Southern China

    Measurements of Volatile Organic Compounds (VOC) are analyzed to characterize the sources impacting the Hong Kong area. The ratios of different VOC species, m,p-xylenes-to-ethylbenzene, C<sub>6</sub>H<sub>14</sub>-to-toluene and p-xylene-to-total xylenes are used for diagnostic analyses. Photochemical age analysis shows that the sources of reactive aromatics, the most important contributor to the photochemical reactivity, do not appear to be preferentially located in downtown Hong Kong. In addition, they do not appear to be dominated by mobile emissions based on the analyses of speciated VOC data from an earlier study, but related to industrial, waterfront, and fuel-storage activities. The ratios, p-xylene-to-total xylenes and dSO<sub>2</sub>/dNO<sub>y</sub>, suggest that the anomalously high pollutant concentrations in western Hong Kong in the early morning hours of two episode days appear to have come from transport of urban-type emissions. Comparison of observed ambient ratios of selected VOC and their ratios in the speciated VOC emission inventories for Hong Kong and adjacent Pearl River Delta (PRD) Region gives mixed results. The observed ratio C<sub>6</sub>H<sub>14</sub>-to-toluene is consistent with the speciated version of the VOC emission inventory. The ratios of selected alkanes are not. This may be caused by the inaccuracies in the inventory and/or the speciation method.
  • Repeatability and randomness in heterogeneous freezing nucleation

    This study is aimed at clarifying the relative importance of the specific character of the nuclei and of the duration of supercooling in heterogeneous freezing nucleation by immersed impurities. Laboratory experiments were carried out in which sets of water drops underwent multiple cycles of freezing and melting. The drops contained suspended particles of mixtures of materials; the resulting freezing temperatures ranged from &minus;6&deg;C to &minus;24&deg;C. Rank correlation coefficients between observed freezing temperatures of the drops in successive runs were &gt;0.9 with very high statistical significance, and thus provide strong support for the modified singular model of heterogeneous immersion freezing nucleation. For given drops, changes in freezing temperatures between cycles were relatively small (&lt;1&deg;C) for the majority of the events. These frequent small fluctuations in freezing temperatures are interpreted as reflections of the random nature of embryo growth and are associated with a nucleation rate that is a function of a temperature difference from the characteristic temperatures of nuclei. About a sixth of the changes were larger, up to &plusmn;5&deg;C, and exhibited some systematic patterns. These are thought to arise from alterations of the nuclei, some being permanent and some transitory. The results are used to suggest ways of describing ice initiation in cloud models that account for both the temperature and the time dependence of freezing nucleation.
  • Airborne dust distributions over the Tibetan Plateau and surrounding areas derived from the first year of CALIPSO lidar observations

    Using an analysis of the first full year of CALIPSO lidar measurements, this paper derives unprecedented, altitude-resolved seasonal distributions of desert dust transported over the Tibetan Plateau (TP) and the surrounding areas. The CALIPSO lidar observations include numerous large dust plumes over the northern slope and eastern part of the TP, with the largest number of dust events occurring in the spring of 2007, and some layers being lofted to altitudes of 11–12 km. Generation of the Tibetan airborne dusts appears to be largely associated with source regions to the north and on the eastern part of the plateau. Examination of the CALIPSO time history reveals an "airborne dust corridor" due to the eastward transport of dusts originating primarily in these source areas. This corridor extends from west to east and shows a seasonality largely modulated by the TP through its dynamical and thermal forcing on the atmospheric flows. On the southern side, desert dust particles originate predominately in Northwest India and Pakistan. The dust transport occurs primarily in dry seasons around the TP western and southern slopes and dust particles become mixed with local polluted aerosols. No significant amount of dust appears to be transported over the Himalayas. Extensive forward trajectory simulations are also conducted to confirm the dust transport pattern from the nearby sources observed by the CALIPSO lidar. Comparisons with the OMI and MODIS measurements show the unique capability of the CALIPSO lidar to provide unambiguous, altitude-resolved dust measurements.
  • What can 14CO measurements tell us about OH?

    The possible use of <sup>14</sup>CO measurements to constrain hydroxyl radical (OH) concentrations in the atmosphere is investigated. <sup>14</sup>CO is mainly produced in the upper atmosphere from cosmic radiation. Measurements of <sup>14</sup>CO at the surface show lower concentrations compared to the upper atmospheric source region, which is the result of oxidation by OH. In this paper, the sensitivity of <sup>14</sup>CO mixing ratio surface measurements to the 3-D OH distribution is assessed with the TM5 model. Simulated <sup>14</sup>CO mixing ratios agree within a few molecules <sup>14</sup>CO cm<sup>&minus;3</sup> (STP) with existing measurements at five locations worldwide. The simulated cosmogenic <sup>14</sup>CO distribution appears mainly sensitive to the assumed upper atmospheric <sup>14</sup>C source function, and to a lesser extend to model resolution. As a next step, the sensitivity of <sup>14</sup>CO measurements to OH is calculated with the adjoint TM5 model. The results indicate that <sup>14</sup>CO measurements taken in the tropics are sensitive to OH in a spatially confined region that varies strongly over time due to meteorological variability. Given measurements with an accuracy of 0.5 molecules <sup>14</sup>CO cm<sup>&minus;3</sup> STP, a good characterization of the cosmogenic <sup>14</sup>CO fraction, and assuming perfect transport modeling, a single <sup>14</sup>CO measurement may constrain OH to 0.2–0.3&times;10<sup>6</sup> molecules OH cm<sup>&minus;3</sup> on time scales of 6 months and spatial scales of 70&times;70 degrees (latitude&times;longitude) between the surface and 500 hPa. The sensitivity of <sup>14</sup>CO measurements to high latitude OH is about a factor of five higher. This is in contrast with methyl chloroform (MCF) measurements, which show the highest sensitivity to tropical OH, mainly due to the temperature dependent rate constant of the MCF–OH reaction. A logical next step will be the analysis of existing <sup>14</sup>CO measurements in an inverse modeling framework. This paper presents the required mathematical framework for such an analysis.
  • Secondary organic aerosol formation from reaction of tertiary amines with nitrate radical

    Secondary organic aerosol formation from the reaction of tertiary amines with nitrate radical was investigated in an indoor environmental chamber. Particle chemistry was monitored using a high resolution aerosol mass spectrometer while gas-phase species were detected using a proton transfer reaction mass spectrometer. Trimethylamine, triethylamine and tributylamine were studied. Results indicate that tributylamine forms the most aerosol mass followed by trimethylamine and triethylamine respectively. Spectra from the aerosol mass spectrometer indicate the formation of complex non-salt aerosol products. We propose a reaction mechanism that proceeds via abstraction of a proton by nitrate radical followed by RO<sub>2</sub> chemistry. Rearrangement of the aminyl alkoxy radical through hydrogen shift leads to the formation of hydroxylated amides, which explain most of the higher mass ions in the mass spectra. These experiments show that oxidation of tertiary amines by nitrate radical may be an important night-time source of secondary organic aerosol.
InterServer Web Hosting and VPS
InterServer Web Hosting and VPS