Supplementary material to “Quantifying mineral dust mass budgets: Systematic
terminology, constraints, and current estimates”
C. S. Zender, University of California, Irvine; R. L. Miller, NASA Goddard Institute for Space Studies, New York, New York; I. Tegen, Institute for Tropospheric Research, Leipzig, Germany.
Citation:
Zender, C. S., R. L. Miller, and I. Tegen (2004),
Quantifying mineral dust mass budgets: Systematic terminology, constraints, and current estimates,
Eos Trans. AGU, 85(48), 509.
[Full Article (pdf)]
Mineral dust mass budget estimates in the current literature exist in sufficient numbers
to summarize only for anthropogenic and natural sources in combination. The wide range of
current estimates of global dust emission and loading highlights the disparity between models
and observations, and among models. Table A1 surveys recent models estimates of mineral dust
mass budgets. Few studies provide quantitative estimates of uncertainties such as natural
variability and model error. Including these would more completely represent, and further
widen, the estimated range of mass budgets. Since 2001, published dust emission estimates for
the present climate range from 1000 to 2150 Tg yr1.
Atmospheric burden estimates range from 8 to 36 Tg, however, an uncertainty factor
exceeding 4. The surprising discrepancy calls into question whether observations could be
better used to constrain dust mass budgets.
Acknowledgments
We gratefully acknowledge all authors of cited studies. N. Mahowald provided insightful
comments. C.S.Z. was supported by NASA grants NAG5-10147 and NAG5-10546. R.L.M. was supported
by the U.S. National Science Foundation’s Climate Dynamics Program ATM-01-24258.
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