Emissions from ships with respect to their effects on clouds

Citation
Pv. Hobbs et al., Emissions from ships with respect to their effects on clouds, J ATMOS SCI, 57(16), 2000, pp. 2570-2590
Citations number
34
Categorie Soggetti
Earth Sciences
Journal title
JOURNAL OF THE ATMOSPHERIC SCIENCES
ISSN journal
00224928 → ACNP
Volume
57
Issue
16
Year of publication
2000
Pages
2570 - 2590
Database
ISI
SICI code
0022-4928(20000815)57:16<2570:EFSWRT>2.0.ZU;2-F
Abstract
Emissions of particles, gases, heat, and water vapor from ships are discuss ed with respect to their potential for changing the microstructure of marin e stratiform clouds and producing the phenomenon known as "ship tracks." Ai rborne measurements are used to derive emission factors of SO, and NO from diesel-powered and steam turbine-powered ships, burning low-grade marine fu el oil (MFO); they were similar to 15-89 and similar to 2-25 g kg(-1) of fu el burned, respectively. By contrast a steam turbine-powered ship burning h igh-grade navy distillate fuel had an SO2 emission factor of similar to 6 g kg(-1). Various typos of ships, burning both MFO and navy distillate fuel, emitted from similar to 4 x 10(15) to 2 x 10(16) total particles per kilogram of fu el burned (similar to 4 x 10(15)-1.5 x 10(16) particles per secondi. Howeve r, diesel-powered ships burning MFO emitted particles with a larger mode ra dius (similar to 0.02-0.05 mu m) and larger maximum sizes than those powere d by steam turbines burning navy distillate fuel (mode radius similar to 0. 02 mu m). Consequently, if the particles have similar chemical compositions , those emitted by diesel ships burning MFO will serve as cloud condensatio n nuclei (CCN) at lower supersaturations land 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 em it particles with a mode radius similar to that of diesel-powered ships fue led 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 determi ning whether or not a ship will produce a ship track. However, more measure ments 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. Me asurements of the total particles entering marine stratiform clouds from di esel-powered ships fueled by MFO, and increases in droplet concentrations p roduced by these particles, show that only about 12% of the particles serve as CCN. The fluxes of beat and water vapor from ships are estimated to be similar t o 2-22 MW and similar to 0.5-1.5 kg s(-1), respectively. These emissions ra rely produced measurable temperature perturbations, and never produced dete ctable perturbations in water vapor, in the plumes from ships. Nuclear-powe red ships, which emit heat but negligible particles. do not produce ship tr acks. Therefore, it is concluded that heat and water vapor emissions do nor play a significant role in ship track formation and that particle emission s, particularly from those burning low-grade fuel oil, are responsible for ship track formation. Subsequent papers in this special issue discuss and t est these hypotheses.