Core OL-92 from Owens Lake, southeast California
Continental-marine correlation of Late Pleistocene climate change: Census of palynomorphs from core OL-92, Owens Lake, California
- Ronald J. Litwin
- Norman O. Frederiksen
- U.S. Geological Survey, Reston, VA
- David P. Adam
- U.S. Geological Survey, Menlo Park, CA
- Victoria A.S. Andrle
- Thomas P. Sheehan
- U.S. Geological Survey, Reston, VA
Contents:
Introduction
The initial palynomorph census obtained from core OL-92 indicates the
presence of a nearly continuous record of pollen assemblages through
approximately 320 meters of lake sediments from Owens Lake, Inyo County,
southeastern California. The sediments recovered range in age from
present day to approximately 0.8 Ma, i.e., the entire Brunhes polarity
chron and the uppermost portion of the Matuyama polarity chron (Smith,
this volume; Glen et al., this volume). Preliminary palynological results
suggest a high correlation of the terrestrial fossil record to d18O
isotope curves derived from marine core analyses. Core OL-92 therefore
has potential to become an important baseline record for correlating
climate change in terrestrial and marine environments through the Late
Cenozoic.
This study had four purposes:
- to assess the quality and continuity of the palynomorph record in core OL-92,
- to determine the core's potential for providing a high resolution signal of climate change for the southern California Basin and Range through the Late Cenozoic, on the basis of its fossil pollen,
- to correlate this terrestrial climate change record with high resolution marine cores through the same temporal interval, and
- to create a statistically significant pollen database for comparison with coeval Late Cenozoic long terrestrial records across the western U.S..
Preliminary conclusions are discussed here; detailed analyses of the
pollen assemblages from these core samples will be presented at a later
date.
Location
The field location and a detailed core log of OL-92 are noted in Smith
(this volume). The core was sited at approximately 36° 22'50"N, 117° 57'
40" W, in Owens Valley, at the southwestern end of Owens Lake (Figure 1A).
Provenance
The palynological record preserved in the core sediments represents a
regional vegetational record of the Owens Valley watershed, derived in
large part from the eastern flank of the southern Sierra Nevada (John Muir
Wilderness Area and Inyo National Forests) and the western flank of the
Inyo Mountains (including part of the Inyo National Forest)(Figure 1A).
Drainages from these two areas combine in the valley to form the south-
flowing Owens River that presently terminates in Owens Lake at the
southern end of the valley. To the southwest of the core site Ash Creek
drains approximately 7400 ft. of vertical relief above lake level on the
eastern flank of Muah Mountain. To the northwest of the core
siteCottonwood Creek drains nearly 9300 ft. of vertical relief above lake
level on the eastern flank of Cirque Peak and the southern flank of Wonoga
Peak.
Age calibration
The pollen record of Owens Lake core OL-92 is especially valuable for
climate change research because it can be calibrated for age by several
independent means. First, coring at 309.1-308.5 m depth penetrated a
tephra marker bed, the Bishop Ash (primary ashfall). This tephra unit is
geographically widespread from California to Kansas (Izett et al., 1988;
Figure 1B) and has been dated radiometrically at an absolute age of
0.78±0.02 Ma (Izett and Obradovich, 1991), on the basis of 40Ar-39Ar laser
fusion analysis of the sanidine component of the tuff. Second, the
Brunhes-Matuyama polarity chron boundary likely was penetrated just below
the tuff, in our sample depth interval 309.1-312.33 m (see discussion,
below). Izett and Obradovich (1991) back-calculated the Brunhes-Matuyama
chron boundary at approximately 0.79 Ma, on the basis of inferred
deposition rates for other lake cores in the western region that also
recorded the tuff and polarity datums. They noted that their age estimate
corroborated ages that were previously derived independently by oxygen
isotope analyses (Shackleton et al., 1990) and astronomical calculations
(Johnson, 1982). Third, Bischoff et al. (this volume) calculated age/depth
relationships for the core on the basis of 14C isotope ages (upper part of
core) and on 40Ar-39Ar laser fusion analyses of the Bishop Ash (Izett and
Obradovich, 1991) in the lower part of the core.
Materials and methods
This study was a reconnaisance-scale palynological census of the OL-92
interval 21.09-323.28 m depth. Fine resolution pollen analysis of the core
interval 0-60 m is in progress by researchers at the University of
Arizona (Woolfenden, this volume), and the pollen assemblage dataset
through the 0-20 m depth interval is not included in this report. Both
reconnaissance and fine scale sampling were done through the depth
interval 20-60 m, to permit comparison of results of the two sampling
scales. The sampling interval for the pollen assemblages presented in
this report (138 samples) is noted in Figure 2 and Tables 2-3, and
correlates directly with samples obtained for diatom analyses (Bradbury,
this volume). For pollen extraction, approximately 2-5 grams of sediment
were decalcified with 20% HCl and demineralized with 52% HF (in a fume
hood) until the mineral fraction was disaggregated. Strew slides of
neutral pH residue were made to identify incompletely disaggregated
samples. Samples of silt-sand then were acidified in 2% HCl and
centrifuged in an aqueous solution of zinc chloride (s.g. 2.0) for
specific gravity separation. Undigested or clay-rich samples were
retreated in HCl, HF, or were winnowed of clay before specific gravity
separation. Clay removal was accomplished by centrifugation of mud in a
dilute low-sudsing detergent (surfactant). (For specific procedures see
Litwin and Andrle, 1992). The residual organic fraction was isolated by
the specific gravity separation mentioned above. Palynomorphs also were
recaptured from the clay-rich supernatant fraction by vacuum-filtering
with an 8 _m nylon filter. These were rinsed in HCl and combined with the
other palynomorph fraction. Melted glycerine jelly was added to the
recombined palynomorph fraction for permanent microscope slide preparation.
Tabulation
Minimum census counts of 200 specimens were made from each sample where
possible (total dataset of ~28,600 specimens). Forty two taxa and census
categories (combinations of taxa) were identified. Pollen identifications
mostly were made to generic level and in several cases to family level.
Conifer pollen frequently was encountered as broken specimens in these
preparations. To correct this we counted isolated sacci as half-specimens
and did not count isolated corpi. The subtotal of broken grains was added
to counts of complete conifer pollen grains for a final sum. All
identifiable taxa were codedfor census (Table 1). Census figures are
presented in Tables 2a and 2b. All counts below 208 m depth were
normalized to 200 specimens (Table 2b) before preliminary climatic trends
were interpreted. Original preparations from which these census data were
compiled are reposited at the U.S. Geological Survey (Reston, VA).
Discussion
The initial pollen analyses indicate that the Owens Lake core OL-92
preserves a high quality, nearly continuous terrestrial vegetational
record from the Owens Valley watershed that spans the past 0.8 Ma. A high
rate of change was noted for individual taxon frequencies and for
assemblage diversities. We attribute this in part to our relatively low
sampling density, and in part to the presence of a high resolution climate
signal. Figure 3A illustrates the curve for pines (genus Pinus, including
all species) plotted against core depth (unit depth), with ages assigned
on the basis of the age/depth values calculated by Bischoff et al. (this
volume). We used Pinus relative frequency to test for response to changes
in temperature and precipitation associated with glacial and interglacial
events because it was the dominant element in our long terrestrial record,
because the genus is known to be a prodigous producer of pollen, and
because its relative frequency had a high rate of change. Relative
frequencies below 50% and above 90% were chosen for initial comparison
(minima M1-M8 and peak abundances P1-P7, Figure 3A) to known climatic
shifts. The deep sea _18O isotope curve of Ruddiman et al. (1989) from
Site 607 (North Atlantic Ocean) was chosen as a good approximate glacial/
interglacial record for comparison to the Pinus curve of Core OL-92. The
age/depth values in Figure 3A then were transposed and the Pinus curve was
replotted (Figure 3B) so that preliminary comparison could be made between
the Pinus and _18O curves at the same scale (as a tentative estimate of
unit time).
The initial results indicate that the pollen record for the pines shows a
strong positive correlation with each of the marine oxygen-isotope Stages
for this time interval. The stratigraphic interval examined for this
report probably correlates with _18O isotope Stages 2 (base of 1?) to 22
(23?). The Pinus minima M8-M1 appear to correspond to isotope stages 2, 4,
6 (~M6 + M5), 8, 10, 14, and 22?, respectively. The Pinus peak abundances
P7-P1 appear to coincide with isotope stages 3, 9, 11, 13 (~P4 + P3), 18?,
and 21?, respectively. With the exception of P2, peak abundances of Pinus
appeared to be coincident with interglacial intervals, and minima appeared
to be coincident with glacial intervals. Additionally, there is
preliminary evidence that the pollen curves at least in some cases have
the capability to resolve substage equivalents within the isotopic record
(Figure 3B, compare the isotopic and pollen excursions for isotope Stage
7). Both convergent and divergent intervals are present in the pollen
curve, with respect to the isotopic trends. Presently we suspect that
convergent trends ("in phase" intervals) may represent larger scale
vegetational response to climatic change, and that divergent trends
("out of phase" intervals) may represent geographically localized
terrestrial response, forest disequilibrium, or artifacts of our sampling
interval and/or density. Some response lag may be present in parts of the
pollen curve (Figure 3B); this may be real or an artifact. Vegetational
leads or lags, with respect to glacial and interglacial trends, will be
able to be established more conclusively once radiometric and
paleomagnetic studies are finished, and calibration of core Ol-92 is
finalized.
In both plots (Figure 3A and Figure 3B) the pollen curve appears to
exhibit two general signal frequencies. The shorter of these frequencies
may correspond to a 41,000 year orbital cycle, and the longer of these to
a 100,000 year orbital cycle. If this is true, the Pinus curve (in
particular) may provide terrestrial evidence that the periodicity shift
from the Matuyama chron (dominantly a 41,000 year frequency) to the
Brunhes chron (dominantly a 100,000 year frequency) may not have occurred
before the beginning of the Brunhes chron. This polarity shift was noted
in marine records by Ruddiman et al. (1989). Additionally, the pollen
records may suggest some overprinting of the shorter cycle on the longer
through much of the Late Cenozoic.
Once the OL-92 pollen dataset is resolved more finely (i.e., with a closer
sampling interval), it may permit a direct comparison to other
exceptionally long terrestrial records such as those at Clear Lake (Adam
et al., 1981; Adam, 1988a, 1988b) and at Tule Lake (Adam et al., 1989),
and direct comparison to Pacific marine records, such as those by Heusser
and Shackleton (1979), Adam (1988b), Gardner et al. (1988), and Heusser
and Heusser (1990). Although these results are preliminary, they do
suggest that the terrestrial vegetational record preserved in the
sediments of Core Ol-92 shows marked response to climatic shifts, and has
the ability to be correlated to the deep sea d18O isotopic record.
Current work
Our current studies focus on testing the response of our other census
categories (and combinations of them) for the OL-92 record. Ultimately,
we hope to correlate our pollen record with other long terrestrial
records, such as the Tule Lake and Clear Lake records, and to test the
practical limits of resolution in several depth intervals of core OL-92,
in order to determine the resolution level of climatic response in the
fossil floral record. We would like to determine the heterogeneity in
resolution potential through core OL-92, as we do not expect glacial and
interglacial resolution potentials necessarily to be equivalent. Results
of these studies will be presented elsewhere, but initial results of
testing this model to the Brunhes chron pollen record at Tule Lake
tentatively suggest that we can resolve each of the equivalent isotope
stages where sampling density and pollen recovery were sufficient.
Conclusions
Initial analyses of the long terrestrial pollen record of Owens Lake core
OL-92 suggest the following conclusions. First, the potential for
examining high resolution climate change through the Late Cenozoic appears
to be excellent, as recorded in the fossil palynomorph record in sediments
of Owens Lake and previously studied western U.S. long terrestrial
records. This potential for the Owens Lake pollen record is enhanced by
independent age controls (radiometric and paleomagnetic datums) that exist
in parts of the cored interval and which permit a high quality age
calibration for its fossil vegetational record. Second, correlation of the
OL-92 pollen record with high resolution deep sea cores as far back as the
Brunhes-Matuyama chron boundary appears to be feasible, and oxygen-isotope
Stages 2(1?)-22(23?) tentatively were identified in this core.
Fluctuations in floral diversity were noted through the sample interval,
but probable causative factors were not established. We only note that
diversity in any sample was in part inversely correlated with Pinus
frequency, and that our studies on this topic are in progress. Lastly, we
believe the palynomorph record at Owens Lake appears to have high
potential for calibrating geographically separated Late Cenozoic long
terrestrial records and for correlating marine and terrestrial Late
Cenozoic climate change in the western U.S., through the Brunhes-Matuyama
chron boundary.
Acknowledgements
This study is part of the U.S. Geological Survey's Global Change and
Climate History Program. The authors acknowledge with gratitude the
following: G.I. Smith (USGS, Menlo Park) for sample splits from core OL-92
and helpful discussion, J.L. Bischoff (USGS, Menlo Park) for sharing age/
depth calibration values, Thomas M. Cronin, Scott E. Ishman, and Jurate
Landwehr (USGS, Reston) for helpful discussion, R.Z. Poore (USGS, Reston)
and Thomas M.Cronin for critical review of this manuscript, and Nancy J.
Durika (USGS, Reston) for preparation of tables and technical support.
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