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  • 1
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2000
    In:  Journal of Geophysical Research: Atmospheres Vol. 105, No. D24 ( 2000-12-27), p. 29379-29386
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 105, No. D24 ( 2000-12-27), p. 29379-29386
    Abstract: To predict the environmental impacts of commercial aviation, intensive studies have been launched to measure the properties and effects of aircraft emissions. These observations have revealed an extremely wide variance with respect to the number and sizes of the particles produced in the exhaust plumes. An analytic parameterization is presented that explains most of the observational variance. It is shown that the observed scatter in emission indices of volatile particles is due mainly to variations of plume age, the detection threshold size of the particle counters, and condensable organic emissions. The principle trend of the volatile particle concentrations with fuel sulfur content can be explained with conversion fractions of sulfur into particulate sulfuric acid at emission within the range 0.5 to 5%. A novel assessment of the perturbation of the stratospheric aerosol layer by a future supersonic aircraft fleet confirms previous estimates and puts these simulations on a sounder physical basis.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2000
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  • 2
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2000
    In:  Journal of Geophysical Research: Atmospheres Vol. 105, No. D15 ( 2000-08-16), p. 19941-19954
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 105, No. D15 ( 2000-08-16), p. 19941-19954
    Abstract: In situ measurements of ultrafine aerosol particle emissions were performed at cruise altitudes behind the Deutsches Zentrum für Luft‐und Raumfahrt ATTAS research jet (Rolls‐Royce/Snecma M45H M501 engines) and a B737‐300 aircraft (CFM International 56‐3B1 engines). Measurements were made 0.15–20 s after emission as the source aircraft burned fuel with sulfur contents (FSC) of 2.6, 56, or 118mg kg −1 . Particle size distributions of from 3‐ to 60‐nm diameter were determined by using condensationnuclei‐counters with varying lower size detection limits. Volatile particle concentrations in the aircraft plumes strongly increased as diameter decreased toward the sizes of large molecular clusters, illustrating that apparent particle emissions are extremely sensitive to the smallest particle size detectable by the instrument used. Environmental conditions and plume age alone could influence the number of detected ultrafine (volatile) aerosols within an order of magnitude, as well. The observed volatile particle emissions decreased nonlinearly as FSC decreased to 60mg kg −1 , reaching minimum values of about 2×10 17 kg −1 and 2×10 16 kg −1 for particles 〉 3nm and 〉 5nm, respectively. Volatile particle emissions did not change significantly as FSCs were further reduced below 60mg kg −1 . Volatile particle emissions did not differ significantly between the two studied engine types. In contrast, soot particle emissions from the modern CFM56‐3B1 engines were 4–5 times less (4×10 14 kg −1 ) than from the older RR M45H M501 engines (1.8×10 15 kg −1 ). Contrail processing has been identified as an efficient sink/quenching parameter for ultrafine particles and reduces the remaining interstitial aerosol by factors of 2–10 depending on particle size. These and previously published data are consistent with volatile particle emissions of 2.4×10 17 kg −1 independent of environmental conditions, engine type and FSCs ranging between 2.6 and 2700mg kg −1 . There are clear experimental indications that nonsulfate compounds (probably nonmethane hydrocarbons) begin to dominate the volatile particle composition as FSC decreases below ∼l00mg kg −1 .
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2000
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  • 3
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1997
    In:  Journal of Geophysical Research: Atmospheres Vol. 102, No. D25 ( 1997-12-27), p. 29867-29880
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 102, No. D25 ( 1997-12-27), p. 29867-29880
    Abstract: Microphysical properties of jet exhaust aerosol and contrails were studied in the near field of the emitting aircraft for different fuel sulfur contents. Measurements were performed behind two different aircraft (ATTAS test aircraft of type VFW 614 and Airbus A310‐300) using fuels with sulfur contents of 6 ppm and 2700 ppm, respectively. At closest approach (plume age 〈 1 s), the total number concentrations exceeded the measuring range of the condensation particle counter, i.e., N 〉 10 5 cm −3 . The concentration of the dry accumulation mode aerosol, i.e., predominantly soot particles, was not affected by the fuel sulfur content. At a plume age of 10 s, an increase in total number concentration ( D p 〉 0.01 µm) by a factor of 3.5 in the high sulfur case compared to the low sulfur case was observed. The ultrafine condensation nuclei fraction (0.007 µm 〈 D p 〈 0.018 µm) contributed at maximum 70% to the total aerosol in the plume while this fraction was much less outside the plume. The high fuel sulfur content also caused an increase in the typical number concentrations of contrail particles by about one third with respect to low sulfur fuel, while the effective diameter of the size distribution was lowered at a fuel sulfur independent ice water content. The major differences in accumulation mode aerosol and microphysical contrail properties between the used aircraft were an increased number concentration of both the accumulation mode aerosol and the contrail particles in the Airbus A310‐300 plume relative to the ATTAS plume. Part of the difference in contrail particles may be caused by different ambient conditions, but the major differences are assumed to be caused by different engine and wake properties.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1997
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    detail.hit.zdb_id: 3094268-8
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  • 4
    In: Journal of Aerosol Science, Elsevier BV, Vol. 32 ( 2001-09), p. 1043-1044
    Type of Medium: Online Resource
    ISSN: 0021-8502
    Language: English
    Publisher: Elsevier BV
    Publication Date: 2001
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  • 5
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1998
    In:  Geophysical Research Letters Vol. 25, No. 15 ( 1998-08-01), p. 2789-2792
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 25, No. 15 ( 1998-08-01), p. 2789-2792
    Type of Medium: Online Resource
    ISSN: 0094-8276
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1998
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  • 6
    Online Resource
    Online Resource
    American Meteorological Society ; 1994
    In:  Journal of Atmospheric and Oceanic Technology Vol. 11, No. 5 ( 1994-10), p. 1392-1399
    In: Journal of Atmospheric and Oceanic Technology, American Meteorological Society, Vol. 11, No. 5 ( 1994-10), p. 1392-1399
    Type of Medium: Online Resource
    ISSN: 0739-0572 , 1520-0426
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 1994
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    detail.hit.zdb_id: 48441-6
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  • 7
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2002
    In:  Journal of Geophysical Research: Atmospheres Vol. 107, No. D23 ( 2002-12-16), p. ACL 12-1-ACL 12-14
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 107, No. D23 ( 2002-12-16), p. ACL 12-1-ACL 12-14
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2002
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    SSG: 16,13
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  • 8
    Online Resource
    Online Resource
    Copernicus GmbH ; 2004
    In:  Atmospheric Chemistry and Physics Vol. 4, No. 5 ( 2004-08-27), p. 1407-1417
    In: Atmospheric Chemistry and Physics, Copernicus GmbH, Vol. 4, No. 5 ( 2004-08-27), p. 1407-1417
    Abstract: Abstract. A unique halocarbon dataset has been obtained using the Australian high altitude research aircraft, the Grob G520T Egrett, during May-June 2000 with GC instrument (DIRAC), which has been previously deployed on balloon platforms. The halocarbon data generally shows a good anticorrelation with ozone data obtained simultaneously from commercial sensors. On 5 June 2000, at 380K, the Egrett entered a high latitude tongue of air over the U.K. CFC-11 and O3 data obtained on the flight show evidence of this feature. The dataset has been used, in conjunction with a 3D chemical transport model, to infer ozone depletion encountered in the midlatitude lower stratosphere during the flight. We calculate that ozone is depleted by 20% relative to its winter value in the higher latitude airmass. A suite of ozone loss tracers in the model have been used to track ozone depletion according to location relative to the vortex and chemical cycle responsible. The model, initialised on 9 December, indicates that 50% of the total chemical ozone destruction encountered in June in the middle latitudes occurred in the 90-70°N equivalent latitude band and that 70% was due to halogen chemistry.
    Type of Medium: Online Resource
    ISSN: 1680-7324
    Language: English
    Publisher: Copernicus GmbH
    Publication Date: 2004
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  • 9
    In: Atmospheric Chemistry and Physics, Copernicus GmbH, Vol. 3, No. 5 ( 2003-10-27), p. 1807-1816
    Abstract: Abstract. Based on in-situ observations performed during the Interhemispheric differences in cirrus properties from anthropogenic emissions (INCA) experiment, we introduce and discuss the cloud presence fraction (CPF) defined as the ratio between the number of data points determined to represent cloud at a given ambient relative humidity over ice (RHI) divided by the total number of data points at that value of RHI. The CPFs are measured with four different cloud probes. Within similar ranges of detected particle sizes and concentrations, it is shown that different cloud probes yield results that are in good agreement with each other. The CPFs taken at Southern Hemisphere (SH) and Northern Hemisphere (NH) midlatitudes differ from each other. Above ice saturation, clouds occurred more frequently during the NH campaign. Local minima in the CPF as a function of RHI are interpreted as a systematic underestimation of cloud presence when cloud particles become invisible to cloud probes. Based on this interpretation, we find that clouds during the SH campaign formed preferentially at RHIs between 140 and 155%, whereas clouds in the NH campaign formed at RHIs somewhat below 130%. The data show that interstitial aerosol and ice particles coexist down to RHIs of 70-90%, demonstrating that the ability to distinguish between different particle types in cirrus conditions depends on the sensors used to probe the aerosol/cirrus system. Observed distributions of cloud water content differ only slightly between the NH and SH campaigns and seem to be only weakly, if at all, affected by the freezing aerosols.
    Type of Medium: Online Resource
    ISSN: 1680-7324
    Language: English
    Publisher: Copernicus GmbH
    Publication Date: 2003
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  • 10
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1996
    In:  Journal of Geophysical Research: Atmospheres Vol. 101, No. D3 ( 1996-03-20), p. 6853-6869
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 101, No. D3 ( 1996-03-20), p. 6853-6869
    Abstract: The impact of sulfur oxides on particle formation and contrails is investigated in the exhaust plumes of a twin‐engine jet aircraft. Different fuels were used with sulfur mass fractions of 170 and 5500 ppm in the fuel, one lower than average, the other above the specification limit of standard Jet‐Al fuel. During various phases of the same flight, the two engines burnt either high‐ or low‐sulfur fuel or different fuels in the two engines. Besides visual, photographic, and video observations from close distance, in situ measurements were made within the plumes at plume ages of 20 to 30 s, at altitudes between 9 and 9.5 km, and temperatures between −49 and −55°C, when the visible contrail was about 2 km long. The data include particle number densities for particles larger than 7 nm, 18 nm, 120 nm, and 1 μm in diameter, together with wind, temperature and humidity measurements. The observations show visible and measurable differences between contrails caused by the different sulfur levels. At ambient temperatures 5 K below the threshold temperature for contrail onset, the plume became visible about 10 m after the engine exit for high sulfur content, but 15 m after the engine exit for low sulfur content. The higher sulfur emission caused a larger optical thickness of the contrail shortly after onset, with slightly brown‐colored contrail when the Sun was behind the observer, and more contrast when viewed against the Sun. The high‐sulfur contrail grew more quickly but also evaporated earlier than the low‐sulfur contrail. At plume ages of about 20 s, each engine plume was diluted to an effective diameter of 20 m. The plumes contained many subvisible particles. Peak number densities were 30,000 cm −3 for particles of diameter above 7 nm and 15,000 cm −3 above 18 nm. The latter is a little larger than the estimated number of soot particles emitted. The high‐sulfur plume shows more particles than the low‐sulfur plume. The differences are about 25% for particles above 7 nm and about 50% above 18 nm. The results indicate that part of the fuel sulfur is converted to sulfuric acid which nucleates with water vapor heterogeneously on soot or nucleates acid droplets homogeneously which then coagulate partly with soot. During descent through the level of contrail onset, the high‐sulfur contrail remained visible at slightly lower altitude (25 to 50 m) or higher temperature (0.2 to 0.4 K). At least for average to high sulfur contents, aircraft generate an invisible aerosol trail which enhances the background level of condensation nuclei, in particular in regions with dense air traffic at northern latitudes and near the tropopause.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1996
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