letters to nature
310 NATURE | VOL 416 | 21 MARCH 2002 | www.nature.com
¯ow line, reaching a minimum of 0.7 cm yr
-1
at Vostok station.
Along the eastern shoreline a signi®cant increase in accretion rate to
2.9 cm yr
-1
is necessary to produce the grounded accreted ice. It is
possible that some of the accreted ice thickening along the eastern
shoreline is the result of compressive ¯ow and not accretion. The
lower layers in the ice sheet (3,300±2,800 m) undergo a 7%
thickening, in contrast to the shallower layers of the ice sheet
(2,400±1,900 m) which thin by 5±13% when grounding. The
accretion process is most evident along the lake shorelines.
In the grounded ice adjacent to the southeastern Lake Vostok
shoreline, we observe an average of 295 m of accreted ice in 21 radar
pro®les (Fig. 1, inset). No accretion ice is imaged adjacent to the
eastern grounding line in the northern 15 radar pro®les. We
estimate the ice ¯ux out of the lake, projected onto a 165-km line
downslope of the lake, parallel to local contours. Assuming an
average thickness of 295 m of accretion ice and a mean velocity of
3myr
-1
, we estimate an annual accreted ice volume ¯ux of
0.146 km
3
yr
-1
along this line. For a lake volume
14
of 1,800 km
3
,
the residence time is 13,300 years. Previous estimates of residence
time range from 4,500 years (ref. 6) to 125,000 years (ref. 1). The
lower estimate (4,500 years), derived from the He
4
/He
3
ratio
6
, may
be related to the formation of the accreted ice samples along the
western shoreline in regions isolated from the main lake circula-
tionÐthat is, the shallow embayment or the western grounding
line. Deeper samples of accreted ice should be more representative
of the open lake.
In the southern portion of Lake Vostok, the interaction between
the lake and the overlying ice sheet is dominated by accretion.
Earlier evidence for melting in this region
4
was based on radar data
oblique to the ice ¯ow ®eld, and is, we believe, incorrect. Ice ¯ow
over southern Lake Vostok has a strong along-lake component, and
has had a consistent orientation for the past 16,000 yearsÐassum-
ing that the velocity has been constant over this time period. The
accretion process dominates at the lake shorelines, although some
accretion continues over the middle of the lake. The accretion ice is
generally transported out of the lake along the southeastern lake
margin. Most samples of accretion ice analysed to date are derived
either from the shallow embayment or from the western grounding
line, environments that are not representative of the open lake
system. M
Received 29 August 2001; accepted 11 February 2002.
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Acknowledgements
The ice-penetrating radar data were acquired by the US National Science Foundation's
Support Of®ce for Aerogeophysical Research (SOAR) located at the University of Texas.
We acknowledge the contributions of the Vostok ®eld team, including the SOAR team, the
Kenn Borek ¯ight crews and the Raytheon East Camp crew. Comments from C. Bentley,
R. Alley, E. Waddington and M. Siegert were appreciated. RADARSATsatellite data was
provided by the Canadian Space Agency. This work was supported by the US National
Science Foundation.
Competing interests statement
The authors declare that they have no competing ®nancial interests.
Correspondence and requests for materials should be addressed to R.E.B.
(e-mail: robinb@ldeo.columbia.edu).
.................................................................
Development of anisotropic structure
in the Earth's lower mantle by
solid-state convection
Allen K. McNamara*, Peter E. van Keken* & Shun-Ichiro Karato²
* Department of Geological Sciences, University of Michigan, Ann Arbor,
Michigan 48109-1063, USA
² Departmentof Geology and Geophysics, Yale University, New Haven,
Connecticut 06520-8109, USA
..............................................................................................................................................
Seismological observations reveal highly anisotropic patches at
the bottom of the Earth's lower mantle, whereas the bulk of the
mantle has been observed to be largely isotropic
1±4
. These patches
have been interpreted to correspond to areas where subduction
has taken place in the past or to areas where mantle plumes are
upwelling, but the underlying cause for the anisotropy is
unknownÐboth shape-preferred orientation of elastically hetero-
genous materials
5
and lattice-preferred orientation of a homo-
geneous material
6±8
have been proposed. Both of these
mechanisms imply that large-strain deformation occurs within
the anisotropic regions, but the geodynamic implications of the
mechanisms differ. Shape-preferred orientation would imply the
presence of large elastic (and hence chemical) heterogeneity
whereas lattice-preferred orientation requires deformation at
high stresses. Here we show, on the basis of numerical modelling
incorporating mineral physics of elasticity and development of
lattice-preferred orientation, that slab deformation in the deep
lower mantle can account for the presence of strong anisotropy in
the circum-Paci®c region. In this modelÐwhere development of
the mineral fabric (the alignment of mineral grains) is caused
solely by solid-state deformation of chemically homogeneous
mantle materialÐanisotropy is caused by large-strain deforma-
tion at high stresses, due to the collision of subducted slabs with
the core±mantle boundary.
Lattice-preferred orientation (LPO) leads to the development of a
mineral fabric in material that deforms primarily by dislocation
creep. Previous work
9
has shown that slabs cause high-stress regions
in the lower mantle, which leads to localized regions of dislocation
creep within a lower mantle dominated by diffusion creep under a
wide range of rheological parameters. It has also been shown that
hot, upwelling regions are low stress, and are therefore dominated
by diffusion creep. The presence of dislocation creep is not in itself a
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