6 Magnetic Record of Catfish Pond - Institute for Rock ... · 0 2E-5 4E-5 6E-5 Ferrimagnetic...

17
126 6 Magnetic Record of Catfish Pond 6.1 Introduction The Holocene and Late-Wisconsinan record of Pittsburg Basin are severely damaged by oxidation due to the drainage of the lake in the early 20 th century. Catfish Pond is a small lake, approximately 5 km NE of Pittsburg Basin (Figure 3.1), and it was cored to fill in the gaps of the paleoenvironmental record of Pittsburg Basin. The lithology of the cores CFP-1 and CFP-2 has already been discussed in chapter 3 (Figure 3.8). Detailed study of the cores revealed that many of the sediments are disturbed either by wave action or (bovine) bioturbation. At present Catfish Pond has a water depth between 0.5 - 1 m and a smaller watershed than Pittsburg Basin. Its sedimentary record is likely to contain many hiatuses and some dry periods are probably not recorded. Section 6.2 gives a detailed overview of the magnetic properties of Catfish Pond sediments and their interpretation in terms of magnetic mineralogy, concentration and grain-size. A paleoenvironmental interpretation of the magnetic and palynological findings is presented in section 6.3. This section is quite brief, since most of the interpretation is presented in chapter 7. 6.2 Magnetic Properties 6.2.1 Magnetic Mineralogy The magnetic mineralogy has been characterized by a combination of magnetic analyses, including Curie temperature and low-temperature magnetic measurements, hysteresis loops and the determination of S-ratios. Figure 6.1 shows several Curie temperature measurements. All samples have final Curie temperatures between 570 and 580(C, indicating the presence of (titano)magnetite or maghemite, but several samples show additional drops in magnetic moment near 320(C (indicated by arrows in Figure 6.1), which may be due to small amounts of pyrrhotite. All samples have higher magnetic moments after being heated to 650/700(C, which is due to the conversion of a weakly magnetic phase into magnetite.

Transcript of 6 Magnetic Record of Catfish Pond - Institute for Rock ... · 0 2E-5 4E-5 6E-5 Ferrimagnetic...

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126

6 Magnetic Record of Catfish Pond

6.1 Introduction

The Holocene and Late-Wisconsinan record of Pittsburg Basin are severely

damaged by oxidation due to the drainage of the lake in the early 20th century. Catfish

Pond is a small lake, approximately 5 km NE of Pittsburg Basin (Figure 3.1), and it was

cored to fill in the gaps of the paleoenvironmental record of Pittsburg Basin. The

lithology of the cores CFP-1 and CFP-2 has already been discussed in chapter 3 (Figure

3.8). Detailed study of the cores revealed that many of the sediments are disturbed either

by wave action or (bovine) bioturbation. At present Catfish Pond has a water depth

between 0.5 - 1 m and a smaller watershed than Pittsburg Basin. Its sedimentary record

is likely to contain many hiatuses and some dry periods are probably not recorded.

Section 6.2 gives a detailed overview of the magnetic properties of Catfish Pond

sediments and their interpretation in terms of magnetic mineralogy, concentration and

grain-size. A paleoenvironmental interpretation of the magnetic and palynological

findings is presented in section 6.3. This section is quite brief, since most of the

interpretation is presented in chapter 7.

6.2 Magnetic Properties

6.2.1 Magnetic Mineralogy

The magnetic mineralogy has been characterized by a combination of magnetic

analyses, including Curie temperature and low-temperature magnetic measurements,

hysteresis loops and the determination of S-ratios. Figure 6.1 shows several Curie

temperature measurements. All samples have final Curie temperatures between 570 and

580(C, indicating the presence of (titano)magnetite or maghemite, but several samples

show additional drops in magnetic moment near 320(C (indicated by arrows in Figure

6.1), which may be due to small amounts of pyrrhotite. All samples have higher magnetic

moments after being heated to 650/700(C, which is due to the conversion of a weakly

magnetic phase into magnetite.

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0 10 0 20 0 3 00 40 0 50 0 60 0 70 0

T empera tu re (°C )

1E -7

3E -7

5E -7

Mag

netic

Mom

ent (

Am2 )

C F P -1 , 8 1 cmT C = 5 70°C

0 10 0 2 00 3 00 40 0 50 0 60 0 70 0

0

2E -6

4E -6 C F P -1 , 2 56 cmT C = 5 70°C

0 10 0 20 0 3 00 40 0 50 0 60 0 70 0

0

8E -8 C F P -1 , 4 83 cmT C = 5 80°C

0 10 0 20 0 3 00 40 0 50 0 60 0 70 0

0

1E -7

2E -7

3E -7

H eating C u rv e

C o o ling C u rv e

C F P -1 , 5 77 cmT C = 5 8 0°C

Fig. 6.1: Curie temperature measurements for samples from Catfish Pond. Arrowsindicate slight drops in magnetic moment that might be due to the presence of pyrrhotite.

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128

0 100 200 300

T emperature (Κ)

0

1E -6

2E -6

Mag

netic

Mom

ent (

Am2

)

1E -10

1E -9

1E -8

1E -7

Gradient -dM

/dT (A

m2/K

)

C F P -1 , 81 cm

0 100 200 300

0

1E -6

2E -6

3E -6

1E -10

1E -9

1E -8

1E -7

1E -6 C F P -1 , 256 cm

0 100 200 300

0

4E -7

8E -7

1.2E -6

1E -11

1E -10

1E -9

1E -8

1E -7 C F P -1 , 483 cm

0 100 200 300

0

4E -7

8E -7

1.2E -6

1.6E -6

2E -6

1E -11

1E -10

1E -9

1E -8

1E -7

M agnetic M om en t

G rad ien t -dM /dT

C F P -1 , 564 cm

a)

b )

c)

d )

Fig. 6.2: Thermal demagnetization curves of low-temperature SIRM. Only a) shows adistinct Verwey ttransition, but a slight transition is present in all samples as can be seenfrom the gradient of the demagnetization curve. The change in gradient above 270 K maybe related to the thawing of the wet sample.

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129

Thermal demagnetization curves of low-temperature SIRM (Figure 6.2) show a distinct

Verwey transition between 100K and 120K only for the uppermost samples (above 100

cm depth). All other samples show only a slight change in magnetic remanence, which

is revealed in the first derivative of the demagnetization curve (open symbols in Figure

6.2). Gradient curves for samples above 100cm show transitions that are smeared out

towards lower temperatures, while the samples below 100cm have Verwey transitions

close to 120K.

Most samples from Catfish Pond have S-ratios below 1.0 (Figure 6.3), suggesting

the presence of an additional magnetically harder mineral besides magnetite or

maghemite. A plot of remanence ratios (Mrs/Ms) vs. coercivity ratios (Hcr/Hc) (Figure 6.4)

shows that many samples are shifted toward the right side of the diagram, which can also

be due to the presence of a magnetically hard (higher Hcr ) component. A scatter plot of

remanence ratio vs. S-ratio (Figure 6.5) shows a negative correlation between the two

parameters. Samples that have low S-ratios tend to have high remanence ratios. In this

case Hcr/Hc is therefore not necessarily an indicator for grain-size changes or a proxy for

the presence of coarse multi-domain grains. No X-ray or SEM-analyses have been

performed on samples from Catfish Pond. It is therefore difficult to confirm the

mineralogy of this magnetically hard component. The smeared out Verwey transitions

in the upper part of the core can be caused by the combined presence of magnetite and

maghemite [Özdemir et al., 1993], and the relatively sharp transitions in the lower

samples (as indicated by the well localized peaks in the gradient curve) could be

explained by the preferential reductive dissolution of pre-existing maghemite in the core.

If this is the case it is unlikely that the low S-ratios observed in Figure 6.3 are due to the

presence of hematite or goethite, which should also be readily dissolved. It is possible,

however, that the high concentrations of maghemite and magnetite in the top 100 cm of

the core are mainly caused by an increased input of iron oxide minerals due to

anthropogenic influences. The absence of maghemite in the lower layers can then be

explained by changes in erosional behavior, and the magnetically hard iron oxides might

be more or less stable throughout the entire record.

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130

0 .8 1

S -R a tio

6 0 0

5 0 0

4 0 0

3 0 0

2 0 0

1 0 0

0

Dep

th (

cm)

S -ra t io s,C F P -1

S -ra t io s,C F P -2

Fig. 6.3: S-ratios for samples from Catfish Pond. S-ratios close to 1 are due tomagnetically soft minerals such as magnetite or maghemite, while magnetically hardminerals such as hematite or goethite shift the S-ratio towards lower values.

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131

0 1 2 3 4 5 6 7

H cr / Hc

0

0 .1

0 .2

0 .3

0 .4

0 .5

0 .6

Mrs

/ M

s

Fig. 6.4: Plot of remanence ratio Mrs/Ms vs. coercivity ratio Hcr/Hc. Grain-size labels onplot after Day et al. [1977]. Shaded area represents Mrs/Ms vs. Hcr/Hc combinationsobtained from synthetic sample sets of known grain-size [modified after Dunlop andÖzdemir, 1997]. Many samples are shifted to the right of the plot due to the presence ofmagnetically hard minerals.

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132

0 .8 0 .8 4 0 .8 8 0 .9 2 0 .9 6 1

S -R atio

2

4

6

Hcr

/ H

c

Fig. 6.5: Scatter plot of coercivity ratio Hcr/Hc vs. S-ratio. Samples with low S-ratiostend to have higher remanence ratios, indicating that Hcr/Hc is not just a function ofparticle size but also reflects changes in magnetic mineralogy.

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133

Iron-sulfides are another possibility to explain the low S-ratios in Figure 4.3.

IRM-acquisition curves for pyrrhotite [Dekkers, 1988b] and greigite [Krs et al., 1992]

show that both minerals are not fully saturated at 300 mT and can cause low S-ratios.

Greigite-bearing lake sediments from Sweden, on the other hand, show relatively high

S-ratios, close to 1.0, in the greigite-containing horizon [Snowball, 1991]. Curie

measurements for the Catfish Pond samples show no thermally unstable behavior

characteristic for the presence of iron sulfides, except for the slight decrease in magnetic

moment near 320(C. Pyrrhotite may be present in some samples, but it is unclear

whether it is present in sufficient amounts to explain the observed behavior in S-ratios

and remanence ratios.

6.2.2 Concentration of Magnetic Minerals

Figure 6.6 shows the variation of concentration-dependent parameters with depth.

Sediments above 100 cm depth are strongly magnetic, and many of the records are

truncated in order to show the more subtle variations in the lower part of the core. The

magnetic concentration of magnetic minerals roughly correlates with core lithology,

which is sketched in Figure 6.6a. Organic sediments tend to have lower concentrations

of magnetic minerals than silty clays that have a low organic matter content. Figure 6.6b

shows the influence of para- and diamagnetic minerals on magnetic susceptibility.

Crosses (9,+) show bulk susceptibility values for cores C.P.-1 and C.P.-2. High field

susceptibility has been calculated from hysteresis measurements, and the ferrimagnetic

susceptibility 3ferri = 3total-3hf is shown as solid circles (q) in Figure 6.6.b. Both bulk

susceptibility and ferrimagnetic susceptibility are higher in the silty clays. The contrast

between clays and organic horizons is lower for ferrimagnetic susceptibility because it

has been corrected for the presence of paramagnetic minerals in the silty clays and

diamagnetic contributions, which tend to occur in the more organic rich layers. Scatter

plots of SIRM (Figure 6.7a) and ARM (Figure 6.7b) vs. magnetic susceptibility also show

the influence of para- and diamagnetic minerals on magnetic susceptibility.

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134

08E

-81.

6E-7

Mag

netic

Sus

cept

ibili

ty(m

3/k

g)

600

500

400

300

200

1000

Depth (cm)

tota

l mag

netic

susc

eptib

ility

ferr

imag

netic

su

scep

tibili

ty

gray

silt

y cl

ay

gytt

ja

Lith

olog

y1E

-52E

-53E

-5A

RM

(A

m2/k

g)0.

0002

0.00

04S

IRM

(A

m2/k

g)

a)b

)c)

d)

ma

x A

RM

at

0.00

025

Am2 /k

g

ma

x S

IRM

at

0.00

6 A

m2 /k

g

ma

x χ

at

5 *

10-7

m3 /k

g

Fig.6.6: Variation of concentration-dependent parameters with depth for Catfish Pond.

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135

0 2E -5 4E -5 6E -5

F err im agnetic S usceptib ilit y (m3/m 3)

0

0.1

0.2

0.3

0.4

0.5

0.6

SIR

M

0 2E -5 4E -5 6E -5 8E -5 0.0001

T ota l S usceptib ilit y (m3/m 3)

0

0.2

0.4

0.6

T o ta lS u scept ib il it y

F err im agn eticS u sceptib il it y

a)

0 2E -5 4E -5 6E -5

F err im agnetic S usceptib ilit y (m3/m 3)

0

0.004

0.008

0.012

0.016

0.02

AR

M

0 2E -5 4E -5 6E -5 8E -5 0.0001

T ota l S usceptib ilit y (m3/m 3)

0

0.004

0.008

0.012

0.016

0.02

b )

Fig.6.7: Scatter plots of ARM and SIRM vs. susceptibility 3. The correlation betweenremanence parameters and susceptibility increases when 3 is corrected for para- anddiamagnetic contributions.

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136

Neither SIRM nor ARM depend on para- or diamagnetic contributions, and the scatter

in Figure 6.7 can be reduced by plotting both remanence parameters vs. ferrimagnetic

susceptibility (solid symbols) rather than bulk susceptibility (open symbols). Remanence

parameters such as ARM (Figure 6.6c) and SIRM (Figure 6.6.d) show variations with

depth similar to those in ferrimagnetic susceptibility. Since all magnetic parameters

correlate with lithology it is possible that the variations in concentration-dependent

parameters are due to the dilution of a uniform detrital source by non-magnetic organic

material. Figure 6.8 shows a plot of ferrimagnetic susceptibility and ARM vs. total

organic carbon (TOC) content. A good correlation between magnetic susceptibility and

TOC suggests that variations in bulk concentration of magnetic minerals, which is

dominated by large particles, is due to the dilution of a detrital source by organic matter.

The correlation between ARM and TOC, however, is much worse. ARM does not only

depend on the abundance of magnetic minerals, but is also strongly influenced by the

presence of small single-domain grains, which are easily affected by dissolution

processes. The good correlation between magnetic susceptibility and TOC, combined

with the poor correlation between ARM and TOC, indicates that dissolution began to

remove fine-grained particles from the sediments, but failed to affect the coarse-grained

susceptibility-contributing fraction to a large degree.

6.2.3 Magnetic Granulometry

The variation of several grain-size dependent parameters is shown in Figure 6.9.

ARM/3 (Figure 6.9.b) and ARM/SIRM (Figure 6.9.c) are both indicators of the relative

abundance of single-domain particles, while frequency-dependent susceptibility (3FD) can

be used as a proxy for the presence of super-paramagnetic grains. Both ARM/3 and

ARM/SIRM suggest the presence of fine-grained magnetic particles in the uppermost part

of the core (< 100 cm), while the rest of the record is relatively coarse-grained, as

indicated by low ratios of ARM/3 and ARM/SIRM.

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137

0 4 8 12 16 20

T o ta l O rgan ic C arbo n (% )

0

4E -8

8E -8

1 .2E -7

Fer

rim

agne

tic S

usce

ptib

ility

(m3 /

kg)

6E -6

8E -6

1E -5

1 .2E -5

1 .4E -5

AR

M (A

/m)

m ag. susceptib ilit y

A R M

fit fo r χ ,r2 = 0 .72

f it fo r A R M ,r2 = 0 .11

Fig. 6.8: Scatter plot of ferrimagnetic susceptibility and ARM vs. total organic carbon(TOC). The good correlation between susceptibility and TOC suggests that the bulkconcentration of magnetic minerals is dominated by the dilution effects of organic matter.The absence of any correlation between ARM and TOC is probably due to dissolution offine grains in some horizons, which is not connected to the presence of organic matter.

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3 Since dia- and paramagnetic minerals cannot be neglected for the susceptibilitymeasurements 3FD has been corrected for dia- and paramagnetic contributions as outlined inchapter 2.

138

The interval between 100 cm and 140 cm depth is characterized by large variations in

ARM/3total (which disappear when corrected for dia- and paramagnetic components) and

ARM/SIRM, which is only affected by ferrimagnetic minerals. The lithology of this part

of the core consists of organic rich gyttja without any internal structure. It is therefore

hard to tell whether the large variations in this part of the core are due to disturbance of

the core or some other unidentified process. Figure 6.9b and 6.9c show slight differences

below 140 cm depth which may be due to the effects of paramagnetic minerals that were

not entirely compensated for. Figure 6.9d shows variations of frequency-dependent

susceptibility (solid symbols, q) and variations of ARM/SIRM (same as Figure 6.9c, but

at expanded scale). 3FD3 values are generally quite low (the error associated with 3FD

measurements is between 2 and 3%) and do not show a good correlation with

ARM/SIRM, except for the interval between 220 and 260 cm, where both parameters

show low values. The low values of 3FD throughout the lower part of the core (> 100 cm)

agree with the low ARM/3 and ARM/SIRM ratios and indicate a mostly coarse-grained

magnetic component that is little influenced by superparamagnetic grains.

6.3 Paleoenvironmental Interpretation

6.3.1 Correlation of Pittsburg Basin and Catfish Pond Records

Two 14C-ages were obtained for Catfish Pond sediments. A macrofossil found at

100 cm depth yielded a date of 170±40 years. The abrupt increase in magnetic mineral

concentrations can therefore be correlated with the onset of agriculture in the watershed.

A radiocarbon date from 200 cm, which corresponds to the onset of Holocene vegetation,

however, yielded only an age of 5970±40 years.

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139

040

080

012

0016

00

AR

M /

κ (Α

/µ)

600

500

400

300

200

1000

Depth (cm)

AR

M/κ

ferr

i

CF

P-1

AR

M/κ

tota

l

CF

P-1

AR

M/κ

tota

l

CF

P-2

gray

silt

y cl

ay

gyttj

a

Lith

olog

y0

0.02

0.04

0.06

0.08

0.1

SIR

M/A

RM

AR

M /

SIR

MC

FP

-1

AR

M /

SIR

M

CF

P-2

a)b)

c)d

)

02

46

8

χ FD (

%)

600

500

400

300

200

1000

χ FD

(%)

CF

P-1

AR

M/S

IRM

CF

P-1

expa

nde

d sc

ale

Fig. 6.9: Variation of grain-size dependent parameters for Catfish Pond. ARM/� andARM/SIRM are proxies for the relative abundance of single domain grains, 3FD can beused as a proxy for the presence of superparamagnetic grains.

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140

For Illinois, Holocene vegetation patterns were established between 14 ka and 10.9 ka BP

[King, 1981]. This late date for the end of glacial vegetation and the absence of the

hypsithermal prairie period confirm the existence of hiatuses in the Catfish Pond record.

Since no dates are available for Pittsburg Basin in this time range the correlation between

the two cores has to rely on variations in the palynological and magnetic record.

Considering the likely presence of hiatuses in both sites only a very crude correlation is

attempted.

Magnetic records for both sites are consistent but are quite homogenous and lack

distinctive features that enable us to use them for detailed correlation purposes.

Pollen assemblages allow us to correlate them on the basis of the onset of Holocene

vegetation patterns and the zone of high spruce concentrations. Table 6.1 lists the

possible correlation markers.

Palynolog. Feature Depth

Pittsburg Basin

Depth Catfish

Pond

Comments

Onset of Holocene

Vegetation

170 cm 260 cm

(200 - 260 cm)

best defined by the

decline in pine at

260 cm, because

spruce peak

between 200 and

260 cm is mainly

due to the absence

of any pollen

Onset of Spruce

and Pine

250 cm 400 cm

Table 6.1: Correlation Between the two sites Based on Palynological Features

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141

Based on all the available information it is possible to say that the glacial record

represented in Catfish Pond represents the late part of the Wisconsinan and does not

extend into the Sangamon interglacial.

6.3.2 Paleoenvironmental Interpretation

Based on their magnetic properties Catfish Pond sediments are very similar to the

corresponding horizons found in Pittsburg Basin. With the exception of the uppermost

100 cm the magnetic fraction is characterized by coarse-grained ferrimagnetic particles

and an additional magnetically hard component (hematite or goethite), which might be

indicative of dry climate with at least some periods when the lake dried out completely.

The absence of the early Holocene and the hypsithermal period from the Catfish

Pond record has already been discussed in section 7.6.2. The onset of agriculture is well

documented in Catfish Pond by an abrupt increase in concentration of magnetic minerals,

leading to very high values of magnetic susceptibility, ARM and SIRM. An increase in

Ambrosia pollen is also observed.

6.4 Summary

The two cores that were retrieved from Catfish Pond consist of silty gray clay and

crumbly gyttja, and are probably disturbed throughout large parts of the record. The

record is likely to contain many hiatuses.

Sediments above 100 cm depth show very high concentrations of magnetite and

maghemite. These high concentrations are due to increased erosion caused by farming

within the watershed of Catfish Pond. Below 100 cm the concentration of magnetic

minerals decreases abruptly. The magnetic minerals have been characterized by Curie

temperature measurements and thermal demagnetization of low-temperature SIRM. They

consist of (titano)magnetite, pyrrhotite and probably hematite. Bulk susceptibility in this

interval is controlled by the dilution of detrital material by organic carbon. Small grain

sizes, however, were also affected by dissolution, leading to a coarse-grained magnetic

assemblage, low in ARM/3 and ARM/SIRM.

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142

The sediments of Catfish Pond record part of the Holocene and the Wisconsinan.

Neither the Holocene hypsithermal nor the Sangamon interglacial are recorded in the

cores retrieved from this site.