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    Emissions from Ships with respect to Their Effects on Clouds

    Source: Journal of the Atmospheric Sciences:;2000:;Volume( 057 ):;issue: 016::page 2570
    Author:
    Hobbs, Peter V.
    ,
    Garrett, Timothy J.
    ,
    Ferek, Ronald J.
    ,
    Strader, Scott R.
    ,
    Hegg, Dean A.
    ,
    Frick, Glendon M.
    ,
    Hoppel, William A.
    ,
    Gasparovic, Richard F.
    ,
    Russell, Lynn M.
    ,
    Johnson, Douglas W.
    ,
    O’Dowd, Colin
    ,
    Durkee, Philip A.
    ,
    Nielsen, Kurt E.
    ,
    Innis, George
    DOI: 10.1175/1520-0469(2000)057<2570:EFSWRT>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Emissions of particles, gases, heat, and water vapor from ships are discussed with respect to their potential for changing the microstructure of marine stratiform clouds and producing the phenomenon known as ?ship tracks.? Airborne measurements are used to derive emission factors of SO2 and NO from diesel-powered and steam turbine-powered ships, burning low-grade marine fuel oil (MFO); they were ?15?89 and ?2?25 g kg?1 of fuel burned, respectively. By contrast a steam turbine?powered ship burning high-grade navy distillate fuel had an SO2 emission factor of ?6 g kg?1. Various types of ships, burning both MFO and navy distillate fuel, emitted from ?4 ? 1015 to 2 ? 1016 total particles per kilogram of fuel burned (?4 ? 1015?1.5 ? 1016 particles per second). However, diesel-powered ships burning MFO emitted particles with a larger mode radius (?0.03?0.05 ?m) and larger maximum sizes than those powered by steam turbines burning navy distillate fuel (mode radius ?0.02 ?m). Consequently, if the particles have similar chemical compositions, those emitted by diesel ships burning MFO will serve as cloud condensation nuclei (CCN) at lower supersaturations (and will therefore be more likely to produce ship tracks) than the particles emitted by steam turbine ships burning distillate fuel. Since steam turbine?powered ships fueled by MFO emit particles with a mode radius similar to that of diesel-powered ships fueled by MFO, it appears that, for given ambient conditions, the type of fuel burned by a ship is more important than the type of ship engine in determining whether or not a ship will produce a ship track. However, more measurements are needed to test this hypothesis. The particles emitted from ships appear to be primarily organics, possibly combined with sulfuric acid produced by gas-to-particle conversion of SO2. Comparison of model results with measurements in ship tracks suggests that the particles from ships contain only about 10% water-soluble materials. Measurements of the total particles entering marine stratiform clouds from diesel-powered ships fueled by MFO, and increases in droplet concentrations produced by these particles, show that only about 12% of the particles serve as CCN. The fluxes of heat and water vapor from ships are estimated to be ?2?22 MW and ?0.5?1.5 kg s?1, respectively. These emissions rarely produced measurable temperature perturbations, and never produced detectable perturbations in water vapor, in the plumes from ships. Nuclear-powered ships, which emit heat but negligible particles, do not produce ship tracks. Therefore, it is concluded that heat and water vapor emissions do not play a significant role in ship track formation and that particle emissions, particularly from those burning low-grade fuel oil, are responsible for ship track formation. Subsequent papers in this special issue discuss and test these hypotheses.
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      Emissions from Ships with respect to Their Effects on Clouds

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4159143
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    contributor authorHobbs, Peter V.
    contributor authorGarrett, Timothy J.
    contributor authorFerek, Ronald J.
    contributor authorStrader, Scott R.
    contributor authorHegg, Dean A.
    contributor authorFrick, Glendon M.
    contributor authorHoppel, William A.
    contributor authorGasparovic, Richard F.
    contributor authorRussell, Lynn M.
    contributor authorJohnson, Douglas W.
    contributor authorO’Dowd, Colin
    contributor authorDurkee, Philip A.
    contributor authorNielsen, Kurt E.
    contributor authorInnis, George
    date accessioned2017-06-09T14:36:24Z
    date available2017-06-09T14:36:24Z
    date copyright2000/08/01
    date issued2000
    identifier issn0022-4928
    identifier otherams-22668.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4159143
    description abstractEmissions of particles, gases, heat, and water vapor from ships are discussed with respect to their potential for changing the microstructure of marine stratiform clouds and producing the phenomenon known as ?ship tracks.? Airborne measurements are used to derive emission factors of SO2 and NO from diesel-powered and steam turbine-powered ships, burning low-grade marine fuel oil (MFO); they were ?15?89 and ?2?25 g kg?1 of fuel burned, respectively. By contrast a steam turbine?powered ship burning high-grade navy distillate fuel had an SO2 emission factor of ?6 g kg?1. Various types of ships, burning both MFO and navy distillate fuel, emitted from ?4 ? 1015 to 2 ? 1016 total particles per kilogram of fuel burned (?4 ? 1015?1.5 ? 1016 particles per second). However, diesel-powered ships burning MFO emitted particles with a larger mode radius (?0.03?0.05 ?m) and larger maximum sizes than those powered by steam turbines burning navy distillate fuel (mode radius ?0.02 ?m). Consequently, if the particles have similar chemical compositions, those emitted by diesel ships burning MFO will serve as cloud condensation nuclei (CCN) at lower supersaturations (and will therefore be more likely to produce ship tracks) than the particles emitted by steam turbine ships burning distillate fuel. Since steam turbine?powered ships fueled by MFO emit particles with a mode radius similar to that of diesel-powered ships fueled by MFO, it appears that, for given ambient conditions, the type of fuel burned by a ship is more important than the type of ship engine in determining whether or not a ship will produce a ship track. However, more measurements are needed to test this hypothesis. The particles emitted from ships appear to be primarily organics, possibly combined with sulfuric acid produced by gas-to-particle conversion of SO2. Comparison of model results with measurements in ship tracks suggests that the particles from ships contain only about 10% water-soluble materials. Measurements of the total particles entering marine stratiform clouds from diesel-powered ships fueled by MFO, and increases in droplet concentrations produced by these particles, show that only about 12% of the particles serve as CCN. The fluxes of heat and water vapor from ships are estimated to be ?2?22 MW and ?0.5?1.5 kg s?1, respectively. These emissions rarely produced measurable temperature perturbations, and never produced detectable perturbations in water vapor, in the plumes from ships. Nuclear-powered ships, which emit heat but negligible particles, do not produce ship tracks. Therefore, it is concluded that heat and water vapor emissions do not play a significant role in ship track formation and that particle emissions, particularly from those burning low-grade fuel oil, are responsible for ship track formation. Subsequent papers in this special issue discuss and test these hypotheses.
    publisherAmerican Meteorological Society
    titleEmissions from Ships with respect to Their Effects on Clouds
    typeJournal Paper
    journal volume57
    journal issue16
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(2000)057<2570:EFSWRT>2.0.CO;2
    journal fristpage2570
    journal lastpage2590
    treeJournal of the Atmospheric Sciences:;2000:;Volume( 057 ):;issue: 016
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
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