The role of marine sediments in understanding the...
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The role of marine sediments in understanding the dust cycle
David McGee
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Determining “modern” (Late Holocene) dust fluxes
Modern dust fluxes
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Reconstructing LGM dust fluxes
LGM dust fluxes
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Time series
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Spatial gradients
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Determining dust fluxes in marine sediments
IRD
OIB sediments
Hemipelagic sediments
Challenge: Distinguishing dust from other components of the detrital fraction
Dust
Ash
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is dominantly dust
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North Pacific (East Asian dust)
0 100 200 Age (ka)
VM21-146 (Shatsky Rise)
H3571 (Hess Rise)
Operationally-defined eolian fraction
Aluminum-based fluxes
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But in low dust regions...
Equatorial Pacific sediments: a mixture of material similar to Chinese loess and other material (mafic volcanics?)
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Andesitic ash and long-travelled equatorial undercurrent detritus may be significant contributors as well.
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Equatorial Pacific Examples: 232Th, 4He
Strategy 2: Distinguish between dust and other detrital components using geochemical differences
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232Th as a dust proxy
Equatorial Pacific
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detrital components using grain size differences
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Moving from concentrations to fluxes
Challenge 2: Determining sedimentary fluxes
Increase in dust flux or decrease in biogenic sediment flux?
Dust MAR = Total MAR x [dust]
MAR = mass accumulation rate [ ] = concentration
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Calculating mass accumulation rates (MARs)
1. Age model approach
t1
t2
t1 t2
Δz
Δz
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Calculating MARs:
Largely insensitive to age model errors
“Instantaneous” fluxes at each sample depth
2. Constant flux proxy normalization
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3He
Delivered by interplanetary dust particles (IDPs)
IDP 3He flux ~constant in the late Quaternary
Constant flux proxies
230Th
Produced by 234U decay in the water column
Short residence time in the ocean (decades)
Flux to seafloor ~ production rate in overlying water column
Halflife = 75.7 kyr
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Bioturbation limits resolution
Average open-ocean sedimentation rate: 1-2 cm/kyr.
Average bioturbation depth: 5-10 cm.
In average sediments, bioturbation thus smooths signal over 2-10 kyr intervals.
Without bioturbation
With bioturbation
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Bioturbation can:
-limit our ability to observe abrupt or short-lived dust flux changes
-decrease dust flux differences in time (e.g., LGM-Holocene differences)
-produce mixes of modern and older sediments at the core top (if it is preserved during coring)
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Prospects for higher-resolution marine records
Continental margin cores in places where eolian and fluvial sediments differ by grain size or geochemistry (e.g., North African margin, northwest Pacific).
Open-ocean cores with good carbonate preservation (usually seamounts) (e.g., Shatsky Rise, Hess Rise)
Drift deposits probably not an option.
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Questions to ask about marine dust records
How was dust distinguished from other detrital components?
How were fluxes calculated?
What are errors on absolute ages in the age model?
What effects does bioturbation have on the record?
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232Th offers quantitative dust flux estimates
232Th concentrations near UCC average in most dust source areas, but may be up to 50% higher in fine fraction
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Effects of lateral sediment advection (“focusing”)
• Age model-based MARs reflect all sediment additions (vertical and lateral)
• CFP-based MARs dominantly reflect vertical sedimentation (“rain rates”)
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Arabian Sea (Arabian peninsula, Central Asia)
0 10 20 30 40 50 60 70 80 90 100 110 20
30
40
50
60
70
80
90
Age (ka)
232 T
h flu
x (μ
g cm
-2 k
yr-1
)
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Equatorial and North Tropical Atlantic (North Africa)
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Tasman Sea (Australia)
Kumar et al., 1995
South Atlantic (Southern South America)
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Determining dust fluxes in marine sediments
Challenge 1: Distinguishing dust from other components of the detrital fraction
Hemipelagic sediments
Ice-rafted detritus
Strategy 1: Open-ocean settings outside IRD belt"
• Use geochemical proxies that are minimal in volcanic contaminants
Volcanic ash and sediments Eolian dust
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Equatorial Pacific
232Th concentrations: ~10 ppm in UCC, loess ≤1 ppm in basalts
Strategy 2: Distinguish between dust and other detrital components using geochemical differences