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Forcing radiative efficiency

Gss 2011 Atmospheric Mixing Ratio " 2011 Radiative Forcing (W/m ) 2011 Radiative Efficiency (W/ (m ppb(v))) Atmospheric Residence Time (years) Change in Mixing Ratio from 2005 to 2011... [Pg.421]

Weaver C.P. (2003). Efficiency of storm tracks an important climate parameter The role of cloud radiative forcing in poleward heat transport. J. Geophys. Res., 108(D1), 5/1-5/6. [Pg.556]

Many astrophysical textbooks accept the hypothesis of Michaud [14] of efficient stratification in the photosphere of selected elements, and even isotopes, by a delicate balance between the radiative pressure on the atoms and monatomic cations absorbing the ambient photons, and the fall due to gravitational attraction. This theory still needs to be refined in many elaborate details. If it applies to the He stars (Sect. 5) with the elusive helium isotope enriched by a factor 5000, the discrimination originates in the gravitational force being 25... [Pg.214]

Aerosol Radiative Forcing Efficiency The radiative forcing of an aerosol species can be normalized by its column mass burden to produce a radiative forcing efficiency per unit mass AG. For sulfate aerosol, for example, one obtains... [Pg.1070]

One may also define a related measure, the radiative forcing efficiency per unit optical depth, for example... [Pg.1070]

FIGURE 24.13 Radiative effects of East Asian aerosol during the period April S-1S, 2001 (Conant et al. 2003) Optical depth surface forcing efficiency (W m"2 t i ) TOA forcing efficiency (Wm 2 1) surface forcing (Wm-2) and TOA forcing (Wm ). Values are for clear skies assuming that the aerosol components are externally mixed. [Pg.1076]

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See also in sourсe #XX -- [ Pg.1070 ]



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Radiative efficiency

Radiative forcing

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