Finger rafting

Last updated

Aerial photograph showing two thin ice sheets (made of nilas) that are moving toward each other. Along the length of the contact between the two sheets, segments where one sheet climbs onto the other alternate with others where it is the other way around. The lighter areas are where the ice thickness has doubled due to the overlapping process. This pattern is known as finger rafting. In many cases, it is highly systematic. Nilas sea ice 2.jpg
Aerial photograph showing two thin ice sheets (made of nilas) that are moving toward each other. Along the length of the contact between the two sheets, segments where one sheet climbs onto the other alternate with others where it is the other way around. The lighter areas are where the ice thickness has doubled due to the overlapping process. This pattern is known as finger rafting. In many cases, it is highly systematic.
Finger rafting in the Weddell Sea, Operation IceBridge photo, 2017. Finger rafting Weddell Sea.jpeg
Finger rafting in the Weddell Sea, Operation IceBridge photo, 2017.
Idealized three-dimensional representation of finger rafting, It occurs when two thin ice sheets converge toward each other. Drawing of rafted ice.svg
Idealized three-dimensional representation of finger rafting, It occurs when two thin ice sheets converge toward each other.
Finger rafting derives its name from its resemblance to the interlocking of fingers. Note that the fingers shown here are not interlaced normally (with all ten fingers showing from the top), but interlaced as in finger rafting (with only five fingers visible from either the top or bottom). Finger rafting (sea ice) with real hands.JPG
Finger rafting derives its name from its resemblance to the interlocking of fingers. Note that the fingers shown here are not interlaced normally (with all ten fingers showing from the top), but interlaced as in finger rafting (with only five fingers visible from either the top or bottom).
Rafted ice observed during MOSAiC Expedition in June 2020. Rafted sea ice.jpg
Rafted ice observed during MOSAiC Expedition in June 2020.

Finger rafting develops in an ice cover as a result of a compression regime established within the plane of the ice. As two expanses of sea ice converge toward another, one of them slides smoothly on top of the other (it is overthrusted) along a given distance, resulting in a local increase in ice thickness. The term finger rafting refers to the systematic alternation of interlocking overthrusts and underthrusts involved in this process. [1] [2] [3] Such a pattern derives its name from its resemblance to the interlocking of fingers. [note 1]

Contents

The process

Rafting, also called telescoped ice, [3] is most noticeable when it involves new and young ice, but also occurs in ice of all thicknesses. [4] The process of finger rafting as such is commonly observed inside a lead, once a thin layer of ice (at the nilas stage) has formed. Although this ice is typically very weak (it is unable to support its own weight outside the water), it contains a lot of brine and is also relatively warm, since being that thin, its temperature is near that of the water. Rafting is accompanied with rapid draining of the brine inside the overlying ice sheet. This brine acts as a lubricant, significantly reducing the friction between the two sheets during overthrusting. Such a mechanism, and the fact that the upper surface of nilas is already slippery, account for overthrust distances in excess of 100 metres (330 ft) (a length-to-thickness ratio of 1000 to one). [4] [note 2]

Rafting versus ridging

Rafting and ridging are two possible responses expected from the interaction between two converging ice sheets or floes. [4] [5] The term 'ridging' refers to the process of ridge formation, involving the breaking up of the ice sheet into distinct blocks (which does not happen during rafting). [1] [2] [3] The reason why breaking happens is that, as the ice thickness increases, the bending moment exerted on the upper surface of the ice exceeds its tensile strength. [5] In other words, the ice is no longer flexible enough to withstand the overthrust event without breaking.

Maximum thickness for rafting

A theoretical formula has been used to estimate the maximum thickness an ice sheet can have in order to be able to raft. [5] This thickness () is

where is Poisson's ratio, is the tensile strength of the ice, is water density, Y is the Young's modulus of sea ice and g is the gravitational acceleration. What this equation shows is that, assuming a representative tensile strength of 0.65 MPa, the maximum thickness for rafting to occur is in the range of 0.2 metres (7.9 in). [5]

See also

Notes

  1. 1 2 Whereby the first finger in one hand overlies the same finger in the other hand), the second finger in one hand underlies the second finger in the other hand, the third fingers do as the first fingers, etc.
  2. According to this source, finger rafting is also possible in lakes and rivers even though this ice is non saline, but only if it is very thin, i.e. less than 2 centimetres (0.79 in).

Related Research Articles

<span class="mw-page-title-main">Optical depth</span>

In physics, optical depth or optical thickness is the natural logarithm of the ratio of incident to transmitted radiant power through a material. Thus, the larger the optical depth, the smaller the amount of transmitted radiant power through the material. Spectral optical depth or spectral optical thickness is the natural logarithm of the ratio of incident to transmitted spectral radiant power through a material. Optical depth is dimensionless, and in particular is not a length, though it is a monotonically increasing function of optical path length, and approaches zero as the path length approaches zero. The use of the term "optical density" for optical depth is discouraged.

<span class="mw-page-title-main">Hydrostatic equilibrium</span> State of balance between external forces on a fluid and internal pressure gradient

In fluid mechanics, hydrostatic equilibrium is the condition of a fluid or plastic solid at rest, which occurs when external forces, such as gravity, are balanced by a pressure-gradient force. In the planetary physics of Earth, the pressure-gradient force prevents gravity from collapsing the planetary atmosphere into a thin, dense shell, whereas gravity prevents the pressure-gradient force from diffusing the atmosphere into outer space.

Isostasy or isostatic equilibrium is the state of gravitational equilibrium between Earth's crust and mantle such that the crust "floats" at an elevation that depends on its thickness and density. This concept is invoked to explain how different topographic heights can exist at Earth's surface. Although originally defined in terms of continental crust and mantle, it has subsequently been interpreted in terms of lithosphere and asthenosphere, particularly with respect to oceanic island volcanoes, such as the Hawaiian Islands.

<span class="mw-page-title-main">Einstein–Hilbert action</span>

The Einstein–Hilbert action in general relativity is the action that yields the Einstein field equations through the stationary-action principle. With the (− + + +) metric signature, the gravitational part of the action is given as

<span class="mw-page-title-main">Bending</span>

In applied mechanics, bending characterizes the behavior of a slender structural element subjected to an external load applied perpendicularly to a longitudinal axis of the element.

<span class="mw-page-title-main">Soil mechanics</span> Branch of soil physics and applied mechanics that describes the behavior of soils

Soil mechanics is a branch of soil physics and applied mechanics that describes the behavior of soils. It differs from fluid mechanics and solid mechanics in the sense that soils consist of a heterogeneous mixture of fluids and particles but soil may also contain organic solids and other matter. Along with rock mechanics, soil mechanics provides the theoretical basis for analysis in geotechnical engineering, a subdiscipline of civil engineering, and engineering geology, a subdiscipline of geology. Soil mechanics is used to analyze the deformations of and flow of fluids within natural and man-made structures that are supported on or made of soil, or structures that are buried in soils. Example applications are building and bridge foundations, retaining walls, dams, and buried pipeline systems. Principles of soil mechanics are also used in related disciplines such as geophysical engineering, coastal engineering, agricultural engineering, hydrology and soil physics.

<span class="mw-page-title-main">Sheet resistance</span> Electrical resistance of a thin film

Sheet resistance, is the resistance of a square piece of a thin material with contacts made to two opposite sides of the square. It is usually a measurement of electrical resistance of thin films that are uniform in thickness. It is commonly used to characterize materials made by semiconductor doping, metal deposition, resistive paste printing, and glass coating. Examples of these processes are: doped semiconductor regions, and the resistors that are screen printed onto the substrates of thick-film hybrid microcircuits.

<span class="mw-page-title-main">Scale height</span>

In atmospheric, earth, and planetary sciences, a scale height, usually denoted by the capital letter H, is a distance over which a physical quantity decreases by a factor of e.

In theoretical physics, the superconformal algebra is a graded Lie algebra or superalgebra that combines the conformal algebra and supersymmetry. In two dimensions, the superconformal algebra is infinite-dimensional. In higher dimensions, superconformal algebras are finite-dimensional and generate the superconformal group.

In physics and fluid mechanics, a Blasius boundary layer describes the steady two-dimensional laminar boundary layer that forms on a semi-infinite plate which is held parallel to a constant unidirectional flow. Falkner and Skan later generalized Blasius' solution to wedge flow, i.e. flows in which the plate is not parallel to the flow.

<span class="mw-page-title-main">Maxwell's equations in curved spacetime</span> Electromagnetism in general relativity

In physics, Maxwell's equations in curved spacetime govern the dynamics of the electromagnetic field in curved spacetime or where one uses an arbitrary coordinate system. These equations can be viewed as a generalization of the vacuum Maxwell's equations which are normally formulated in the local coordinates of flat spacetime. But because general relativity dictates that the presence of electromagnetic fields induce curvature in spacetime, Maxwell's equations in flat spacetime should be viewed as a convenient approximation.

In the theory of general relativity, a stress–energy–momentum pseudotensor, such as the Landau–Lifshitz pseudotensor, is an extension of the non-gravitational stress–energy tensor that incorporates the energy–momentum of gravity. It allows the energy–momentum of a system of gravitating matter to be defined. In particular it allows the total of matter plus the gravitating energy–momentum to form a conserved current within the framework of general relativity, so that the total energy–momentum crossing the hypersurface of any compact space–time hypervolume vanishes.

<span class="mw-page-title-main">Critical state soil mechanics</span>

Critical state soil mechanics is the area of soil mechanics that encompasses the conceptual models that represent the mechanical behavior of saturated remolded soils based on the Critical State concept.

In statistics, the Matérn covariance, also called the Matérn kernel, is a covariance function used in spatial statistics, geostatistics, machine learning, image analysis, and other applications of multivariate statistical analysis on metric spaces. It is named after the Swedish forestry statistician Bertil Matérn. It specifies the covariance between two measurements as a function of the distance between the points at which they are taken. Since the covariance only depends on distances between points, it is stationary. If the distance is Euclidean distance, the Matérn covariance is also isotropic.

<span class="mw-page-title-main">Kirchhoff–Love plate theory</span>

The Kirchhoff–Love theory of plates is a two-dimensional mathematical model that is used to determine the stresses and deformations in thin plates subjected to forces and moments. This theory is an extension of Euler-Bernoulli beam theory and was developed in 1888 by Love using assumptions proposed by Kirchhoff. The theory assumes that a mid-surface plane can be used to represent a three-dimensional plate in two-dimensional form.

<span class="mw-page-title-main">Sea ice growth processes</span>

Sea ice is a complex composite composed primarily of pure ice in various states of crystallization along with air bubbles and included pockets of brine. Understanding its growth processes is important both for climate scientists for use in simulations as well remote sensing specialists since the composition and microstructural properties of the ice ultimately affect how it interacts with electromagnetic radiation.

<span class="mw-page-title-main">Vibration of plates</span>

The vibration of plates is a special case of the more general problem of mechanical vibrations. The equations governing the motion of plates are simpler than those for general three-dimensional objects because one of the dimensions of a plate is much smaller than the other two. This suggests that a two-dimensional plate theory will give an excellent approximation to the actual three-dimensional motion of a plate-like object, and indeed that is found to be true.

<span class="mw-page-title-main">Reinforced solid</span>

In solid mechanics, a reinforced solid is a brittle material that is reinforced by ductile bars or fibres. A common application is reinforced concrete. When the concrete cracks the tensile force in a crack is not carried any more by the concrete but by the steel reinforcing bars only. The reinforced concrete will continue to carry the load provided that sufficient reinforcement is present. A typical design problem is to find the smallest amount of reinforcement that can carry the stresses on a small cube. This can be formulated as an optimization problem.

<span class="mw-page-title-main">Dirac equation in curved spacetime</span> Generalization of the Dirac equation

In mathematical physics, the Dirac equation in curved spacetime is a generalization of the Dirac equation from flat spacetime to curved spacetime, a general Lorentzian manifold.

In gauge theory, topological Yang–Mills theory, also known as the theta term or -term is a gauge-invariant term which can be added to the action for four-dimensional field theories, first introduced by Edward Witten. It does not change the classical equations of motion, and its effects are only seen at the quantum level, having important consequences for CPT symmetry.

References

  1. 1 2 Wmo Sea-Ice Nomenclature • Terminology
  2. 1 2 Environment Canada – Weather and Meteorology – Ice Glossary
  3. 1 2 3 All About Sea Ice, Introduction :: National Snow and Ice Data Center
  4. 1 2 3 Weeks, W. F. (2010) On sea ice (Chap. 12). University of Alaska Press, Fairbanks, 664 p.
  5. 1 2 3 4 Leppäranta, M. (2005). The Drift of Sea Ice. Springer-Verlag, New York, 266 p.