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Consolidated pancake ice forms when pancake ice packs, rafts and freezes together with interstitial frazil ice. Its heterogeneous granular structure can retain stacked layers and acquire later columnar basal growth.

// Target: geophysics.bigb

In a uniformly wind-forced polynya with normalized heat loss $f$, let $H=L+c_{p}m{C}_{\infty }$, $K=f/H$, $J=3S/(4\rho )$ and $r=\rho -{\rho }_s$. The dilute equilibrium model gives $b{u}^2=Jx$, $\varphi bu=Kx$ and $rg\varphi b{b}^{\prime }=S/4$. Hence $u=(rgKx/\rho {)}^{1/3}$, $b=Jx/u^2$ and $\varphi =(K/J)u$. This similarity solution is valid only while the frazil ice volume fraction is small and no exported crystal flux has been neglected improperly.

The Odden ice tongue is an intermittent extension of young sea ice into the Greenland Sea. Repeated formation and export of frazil ice and pancake ice can produce brine rejection without a steadily thickening local ice cover, increasing the salinity of the water left behind.

Pancake ice consists of approximately disk-shaped young ice floes, often with raised edges formed by collisions. Wave-driven collisions and motion in the surrounding frazil ice can dissipate energy.

In seawater, freezing produces nearly salt-free solid and leaves salt in the interstitial liquid. The growing cover is therefore a mushy layer, with sea-ice crystal fabric determined by both crystal growth and the mechanical history. Crystallographic c-axes are perpendicular to the plates' basal planes; grain elongation and c-axis orientation must not be confused.

For first-year sea ice growing by congelation, heat loss first brings the surface water to its salinity-dependent freezing point. Small frazil ice crystals may form and collect into a thin continuous sheet, or a quiet surface can freeze directly; the resulting nilas provides the initial cover. Once the water surface is protected from strong agitation, heat transported by heat conduction upward through the sheet permits freezing onto its underside. Competitive growth favors grains with fast basal-plane growth directed downward, so grains with approximately horizontal c-axes crowd out less favorably oriented grains. The mature congelation ice consists predominantly of long vertical columns beneath a finer initial surface layer. Within and between these grains, the advancing cellular interface traps brine-bearing spaces. The growth sequence and crystallographic selection explain why the resulting texture is columnar rather than a random aggregate of floating crystals.

For pancake ice, wind and surface gravity waves prevent an uninterrupted ice sheet. Supercooled surface water produces suspended frazil ice; crystals accumulate into grease ice and then small coherent cakes. Wave-induced convergence, collisions and repeated accumulation of frazil increase cake size and thickness. Collisions and overwash deposit slush around the margins, building the characteristic raised rims. The crystal aggregate is predominantly granular, with much less systematic orientation than in congelation ice. A calmer interval can add a columnar basal layer, so a pancake need not be purely granular throughout. Observed pancake structures include frazil layers, basal congelation growth and rafted cakes.

In Antarctic consolidated pancake ice, the active edge initially follows this frazil-pancake route. As concentration rises and waves are attenuated, pancakes jam, raft and become frozen together, with interstitial frazil filling the gaps. The consolidated sheet retains overlapping cake outlines, stacked granular layers and an irregular underside, rather than acquiring the simple fabric of a single quiet-water-grown sheet. Later basal freezing can add congelation ice, but the granular fraction often remains large. Snow loading or overwash can flood the top; freezing this slush adds granular snow ice, a separate contribution from seawater-derived frazil. These mechanisms produce the heterogeneous sea-ice crystal fabric documented in cores from the Antarctic marginal ice zone. Quiet basal growth produces columnar ice; wave-driven aggregation and consolidation produce predominantly granular, layered ice.

The main efficient net desalination mechanisms require transport through the ice boundary. In gravity drainage of sea-ice brine, cold saline liquid is denser than the water below, so a connected permeable pore network permits downward flow and compensating entry of less saline seawater. Dense brine can collect into channels and convective drainage pathways. For a layer of depth $H$, a Darcy law estimate of drainage speed is $u_D\sim K\Delta \rho g/\mu$, giving a drainage time $H/u_D$ and showing directly why permeability of a porous medium and buoyancy matter. Warm, brine-rich ice drains much more readily than cold ice whose pores have become poorly connected. This is important during growth and can intensify as warming reconnects channels; an isolated sealed brine pocket cannot drain merely because its liquid is dense. The connectivity constraint is supported by sea-ice permeability measurements.

In meltwater flushing of sea ice, water supplied by surface snow melt or melt ponds has a hydraulic head above sea level and percolates down connected pores and cracks, displacing brine. It can remove salt rapidly in warm summer ice. Its limits are the supply and head of meltwater and pore connectivity; lateral runoff may reduce the amount available for vertical flushing. Gravity-driven drainage can act without surface melting, whereas flushing cannot.

Brine expulsion occurs when additional freezing and solid expansion pressurize an inclusion and force liquid into nearby passages. This is often internal redistribution: expelling brine from one inclusion does not desalinate the entire floe unless that liquid reaches the ocean. Migration of brine inclusions involves melting on a warmer wall and refreezing on the colder wall; molecular salt diffusion through liquid connections is also possible. These slow processes are far less effective at exporting bulk salt than connected advective drainage. Diffusion through the ice lattice itself is extremely slow. Likewise, excluding salt from each growing crystal is not by itself proof of salt loss from a whole ice-brine mixture. Desalination experiments and transport calculations distinguish net salt export from internal redistribution. Gravity drainage dominates desalination of permeable growing ice; meltwater flushing can dominate summer desalination; expulsion, inclusion migration and diffusion are comparatively ineffective without a boundary-crossing flow.

Assume small-amplitude motion, a thin uniform elastic plate, no prestress, and inviscid, irrotational deep water. Write the upward displacement as $\eta (x,t)$, the ice mass per unit area as $m={\rho }_{i}h$, and its flexural rigidity aswhere $E$ is Young's modulus and $\nu$ is Poisson's ratio. The plate equation is $m{\eta }_{tt}+D{\eta }_{xxxx}=p$, where $p$ is the perturbation of upward water pressure.

Let the water velocity potential be $\varphi =A{e}^{kz}{e}^{i(kx-\omega t)}$ below the mean surface $z=0$, with $k>0$. This solves the Laplace equation and decays at depth. For $\eta ={\eta }_0{e}^{i(kx-\omega t)}$, the kinematic boundary condition ${\eta }_t={\varphi }_z$ gives $A=-i\omega {\eta }_0/k$. The linear Bernoulli equation givesEliminating $p$ proves the dispersion relation of a floating elastic plate:Thus the desired wavenumber is the positive root ofFor positive $D$ and $\omega$, this root is unique: the polynomial is negative at zero and positive eventually; if its derivative starts negative, that derivative crosses zero only once, at a negative-valued minimum before the positive root. If a finite water depth $d$ is required, the corresponding relation is ${\omega }^2=(gk+D{k}^5/{\rho }_w)\tanh (kd)/[1+({\rho }_{i}h/{\rho }_w)k\tanh (kd)]$.

Put $\beta =D/{\rho }_w$ and $\alpha ={\rho }_{i}h/{\rho }_w$. Differentiation gives the group velocityFor long periods, the surface gravity wave limit gives $c_g\sim gT/(4\pi )$. At sufficiently short periods, plate inertia and bending dominate, $\omega \sim \sqrt{D/m}{k}^2$ and $c_g\sim 2\sqrt{D/m}k$. Consequently the curve has a group-velocity minimum of a flexural-gravity wave between branches that rise toward both long and short periods, within the formal deep-water plate model. Very short waves eventually fall outside the thin-plate approximation.

The plot is an original model illustration with $h=1\mathrm{m}$, $E=5\mathrm{GPa}$, $\nu =0.3$, ${\rho }_i=917\mathrm{kg}{\mathrm{m}}^{-3}$, ${\rho }_w=1025\mathrm{kg}{\mathrm{m}}^{-3}$, and $g=9.81\mathrm{m}{\mathrm{s}}^{-2}$. Its two minima occur at different periods.

A wave packet near the group-speed minimum carries energy away relatively slowly, so sustained forcing can concentrate energy in that period band. However, wind generation cannot be decided from $c_g$ alone. A steadily translating pressure pattern resonates through its phase velocity $c_p=\omega /k$; it must reach the minimum phase speed of a flexural-gravity wave. Actual wind-wave growth also requires suitable pressure coupling and enough energy input to overcome damping. A coherent cover suppresses ordinary free-surface wave generation, while incoming ocean swell can still excite bending and break the cover.

For disconnected pancake ice or frazil ice, remove the assumption of coherent elastic bending and retain the effective mass loading as a first conservative approximation. Setting $D=0$ gives ${\omega }^2=gk/[1+({\rho }_{i}h/{\rho }_w)k]$. To describe damping as well, replace the elastic layer by a viscous suspension and match velocity and stress to the water beneath: the resulting viscous layer model of frazil-pancake ice has complex $k$, whose real part gives dispersion and imaginary part gives attenuation. Keller's 1998 two-layer model implements this replacement. Effective viscosity and connectedness must reflect the particular cover; zero rigidity alone does not model attenuation.

A polynya is a persistent or recurrent area of open water or relatively thin ice within an otherwise ice-covered region. Persistence of the opening does not mean absence of ice formation: a latent-heat polynya can continuously make ice and export it. In contrast, a sensible-heat polynya remains open because ocean heat inhibits freezing. Both processes may occur at the same site.

At an Antarctic coast, cold air descending from the elevated continent produces strong katabatic winds. Their offshore component drives sea ice away from a fixed coastline, fast-ice edge or grounded-iceberg barrier. Open water exposed to the cold atmosphere loses heat rapidly; frazil ice forms, aggregates into pancake ice or consolidated new ice, and is exported offshore. The opening continues as long as export balances production. Headlands, the shelter provided by fast ice and the direction of the prevailing winds determine the location and size. Terra Nova Bay is a characteristic coastal example. Such latent-heat polynyas are ice factories rather than permanently warm holes in the ice pack.

At an ice shelf front the fixed boundary is floating shelf ice instead of land. Offshore winds blowing across the shelf can similarly remove newly formed sea ice, so an ice-front polynya need not have a different thermodynamic mechanism from a coastal one; the Ross Ice Shelf front provides an important wind-driven example. Shelf-front geometry, ice tongues, grounded icebergs and changes in calving alter the shelter and the supply of drifting pack ice. Some ice-front openings also receive significant sensible heat from currents, tidal mixing or upwelling, and heat carried out of an ice-shelf cavity can affect freezing. A sensible-heat polynya requires a sufficiently warm ocean supply, whereas the latent-heat mechanism requires continuing removal of the ice that does form. Consequently a strict identification of all coastal openings with one mechanism and all ice-shelf openings with the other would be incorrect.

The oceanic roles are substantial. Rapid heat loss and freezing produce brine rejection, raising shelf-water salinity and mass density. The resulting convection and circulation can carry dense shelf water into ice-shelf cavities; melting beneath an ice shelf modifies it into colder, fresher ice-shelf water. Dense shelf and cavity-modified waters can subsequently descend the continental slope, mix with adjacent waters and contribute to Antarctic bottom water. The outcome depends on bathymetry and the density after mixing: not all rejected brine reaches the abyss.

These localized regions can therefore have a disproportionate effect on deep-ocean ventilation, oxygen supply, carbon transport and the large-scale ocean circulation. They are also intense sites of ocean-to-atmosphere heat and moisture transfer. Seasonal sunlight arriving in open water supports high biological production where nutrients are available, with consequences for marine food webs and carbon cycling. Antarctic polynyas connect wind-driven ice export, concentrated ice production and dense-water formation; ice-shelf fronts add a floating boundary and possible cavity-related heat and freshwater exchanges.

In the Pease polynya model, take a straight fixed coast at $x=0$ and an offshore polynya edge at $x=L(t)$. Let consolidated pack ice move offshore at speed $U>0$, let new ice be produced throughout the opening at equivalent thickness rate $F>0$, and let the collected ice at the edge have a prescribed thickness $H$. All fluxes below are per unit length of coastline. The new-ice volume production is $FL$, while the consolidated-ice export relative to the moving edge is $H(U-\dot{L})$. Neglect storage of drifting frazil ice inside the opening, so conservation givesThis is the simplest Pease closure: newly formed ice is collected at the edge rapidly enough that production can be equated to the instantaneous edge flux. A model retaining frazil storage would instead include the local balance ${\partial }_{t}h+{\partial }_x(uh)=F$, with frazil thickness $h$ and transport velocity $u$, together with an edge condition; it should not silently be identified with the instantaneous-collection approximation.

For constant $U,F,H$, the stable equilibrium and relaxation time areIn particular, an initially closed opening has $L(t)=L_{\infty }(1-e^{-t/\tau })$. It initially opens at speed $U$, then slows as its larger area produces more ice. It reaches $63\%$ of its ultimate width after $\tau$ and $95\%$ after $-\tau \log 0.05\simeq 3\tau$; the exact equilibrium is approached asymptotically, not reached at a finite opening time.

The production rate is determined by the energy budget. With $Q_{\mathrm{surf}}$ positive for net upward surface heat loss and $Q_o$ the heat supplied from the underlying ocean, water at its local freezing temperature givesThe surface loss includes sensible and latent turbulent transfers and net radiation. For example, the sensible component is approximately ${\rho }_a{c}_{p,a}{C}_{H}V(T_f-T_a)$, where $V$ is wind speed and $C_H$ an exchange coefficient. Ice motion is commonly parameterized as a small fraction of the offshore wind speed, but currents and the direction relative to the coast also matter. Thus colder air and stronger net cooling increase $F$ and narrow the opening; faster export increases $U$ and widens it; thicker collected ice increases both $L_{\infty }$ and $\tau$. Stronger winds can increase both export and heat loss, so the width's dependence on wind can be much weaker than the formula with artificially fixed $F$ would suggest.

The assumptions are steady spatially uniform forcing; a one-dimensional straight coast; fixed collection thickness and drift speed; no alongshore import of pack ice; water already at freezing rather than an appreciable sensible-heat reservoir; and negligible residence time of newly formed ice. Real coastlines, time-dependent winds, ocean currents, atmospheric adjustment over warm open water and variable ice accumulation can all violate these assumptions. The model describes a latent-heat polynya, not an opening maintained principally by a warm deep-ocean heat supply.

If air temperature rises while wind, $H$ and the other external parameters are unchanged, the smaller air–sea temperature difference reduces net heat loss and hence $F$. For $0<F^{\prime }<F$,The opening becomes wider and takes longer to attain the same fraction of its new equilibrium width. Its initial opening speed remains $U$; the longer equilibration follows from weaker ice production, rather than slower initial export. If warming eliminates net freezing, $F=0$ gives $L=L(0)+Ut$ in the simple kinematic closure, with no finite freezing-balanced width. A negative $F$ represents melt and is outside the positive-production Pease model.

For the shelf-water calculation, a $30$-day month at $0.05\mathrm{m}\mathrm{da}{\mathrm{y}}^{-1}$ produces $h_i=1.5\mathrm{m}$ of ice. Assume a well-mixed $D=100\mathrm{m}$ shelf column, no compensating advection or precipitation, and fixed ice and water densities ${\rho }_i=917$ and ${\rho }_w=1025\mathrm{kg}{\mathrm{m}}^{-3}$. The frozen fraction of its initial liquid mass isLet the liquid initially have salinity $S_0$, and newly formed ice retain $rS$ with $r=0.3$ and $S$ the instantaneous ambient value. For remaining liquid mass $M$, freezing removes salt with the departing ice, so conservation of salt with salt-retaining ice givesThereforeAn initial shelf-water salinity is needed for an absolute answer. Taking $S_0=34$ psu gives $\boxed{\Delta S\simeq 0.32\mathrm{psu}}$. At the accuracy of an equal-density thickness calculation, $f\simeq 1.5/100$ and $\Delta S\simeq 0.7S_{0}f$, giving about $\boxed{0.36\mathrm{psu}}$ for $S_0=34$ psu. These estimates describe the same modest increase. Treating ice as completely fresh would overestimate brine rejection by omitting the factor $0.7$.

The resulting water is denser and can leave the shelf and intrude beneath fresher surface water. It is therefore a physically plausible contribution to the cold halocline. Nevertheless, this one-month column budget yields only a few tenths of a psu, and the salinity contrast across the Arctic halocline can be several psu. If water from a shelf occupying one-third of the area were spread through an equally deep layer over the whole ocean, the average increase would be only about $0.1$ psu. This illustration is not a volume budget for the actual deep Arctic: shelf area fraction is not ocean water-volume fraction, and the exported water can be concentrated within a relatively thin halocline layer.

Consequently this calculation supports a shelf contribution but does not establish its dominance. Repeated seasonal ice production, enhanced production in polynyas, shelf-water export, freshwater dilution, and the thickness and residence time of the receiving layer would all be needed to test dominance. The assumption that the shelf initially becomes ice-free limits the first month's salt production; it does not bound an entire winter's cumulative production if new ice is continually removed.

Another pathway is winter cooling and limited convection of Atlantic-origin water as it enters the Arctic and encounters the ice-covered ocean. Cooling and local freezing can make it near-freezing water without requiring that it first be formed throughout the Siberian shelf. A subsequent fresh surface cap limits further convection; the cooled water is advected into the basin beneath that cap, producing a cold, salinity-stratified lower halocline. Pacific-origin waters also contribute to halocline structure in the western Arctic. Both formation and maintenance depend on circulation and freshwater supply, not simply on the presence of freezing somewhere. The strong stable density stratification then limits upward transfer of heat from the deeper Atlantic layer to sea ice.

A convective chimney is a localized, deeply mixed region within a stratified ocean, formed when surface buoyancy loss allows convection to penetrate far below the surrounding mixed layer. The chimney describes the mixed water column and its circulation; instantaneous downward transfer occurs through many smaller plumes, accompanied by compensating motion and lateral exchange, rather than through one permanently uniform downward pipe. Open-ocean convection occurs in the Labrador and Irminger Seas, the Greenland Sea, the northwestern Mediterranean, and episodically in the open Weddell Sea under a large polynya. Dense-water formation on a continental shelf is related but geometrically distinct from deep open-ocean chimney convection.

Observed Greenland Sea convective chimneys include compact, approximately circular, weakly stratified cores with temperature and salinity much more uniform vertically than in the ambient ocean. A mapped example was about $20\mathrm{km}$ across, extended to about $2500\mathrm{m}$ in winter, and rotated anticyclonically. In summer a fresh, low-density cap and shallower lateral intrusions could isolate the deep core, while winter buoyancy loss removed the cap and renewed deep contact. Such cores could persist through several seasons, so presence of a deep homogeneous core is not proof that vigorous convection is occurring continuously. These particular dimensions and seasonal structure come from successive hydrographic surveys of Greenland Sea chimneys.

Formation is favoured by the cyclonic Greenland gyre, which domes density surfaces and can reduce the depth of the stratified barrier. Cold, dry wind outbreaks produce strong sensible, latent and longwave heat loss. Where frazil ice and pancake ice form in the Odden ice tongue, ice growth removes relatively fresh material while brine rejection increases the density of the remaining water. Ice advection can keep exposing water for further freezing and separate local brine release from later freshwater return. This combination of preconditioning, cooling and sustained salt input can make a formerly buoyant surface layer dense enough to convect.

Conversely, a fresh surface cap supplied by Arctic freshwater and ice melt strengthens density stratification. Warmer atmospheric outbreaks reduce surface heat loss and ice production; circulation changes affecting the cold northwesterly winds and the Odden can reduce the brine source. Atlantic advection supplies both heat and salt, with competing effects on density, so temperature alone is not an adequate diagnostic. The historical decline in Odden ice formation and changes in wind regimes offer a mechanism for less favourable chimney production around the period considered, but ice-driven formation is a physical hypothesis, not evidence that every observed chimney requires ice or that every local change follows a single climate index. The Greenland Sea salt-flux model explicitly includes ice production and advection.

For the brine rejection mechanism, let ${\dot{h}}_i>0$ be ice growth and let $s_w,s_i$ be water and ice salt mass fractions. Newly formed ice removes mass ${\rho }_i{\dot{h}}_i$ per area per time. Compared with removing water at concentration $s_w$, it leaves an excess salt flux in the liquid ofThe units are $\mathrm{kg}{\mathrm{m}}^{-2}{\mathrm{s}}^{-1}$. With the exam's approximation $s=10^{-3}S$ for salinity $S$ in psu, the corresponding mixed-layer salinity tendency is, to first order,If ${\beta }_S=(1/{\rho }_w)(\partial \rho /\partial S)>0$, the surface buoyancy input is negative, with scale $-g{\beta }_S({\rho }_i/{\rho }_w){\dot{h}}_i(S_w-S_i)$. The enhanced density produces downward saline plumes that deepen mixing if this buoyancy loss overcomes the available density stratification. This explains why exporting new ice while retaining its rejected salt can strengthen overturning, whereas later local melt reverses the freshwater effect.

For the numerical comparison, the cover gives the specific heat capacity of ice, not of seawater. A seawater value must therefore be supplied explicitly. Take $c_{p,w}=4000\mathrm{J}\mathrm{k}{\mathrm{g}}^{-1}{\mathrm{K}}^{-1}$ and use the stipulated ${\rho }_w=1025\mathrm{kg}{\mathrm{m}}^{-3}$. A $100\mathrm{m}$ column has initial water mass per areaCooling it by $1.8\mathrm{K}$ removesThe specified thermal density relation givesThis assumes the whole column mixes and neglects entrainment and advected heat. Using the supplied ice heat capacity $2100$ for liquid seawater would change $Q$ incorrectly.

At the freezing point the same heat extraction produces a pure-ice mass per areaHere $f_i$ is the fraction of the original water mass removed into ice. With the explicit ice-density approximation ${\rho }_i=900\mathrm{kg}{\mathrm{m}}^{-3}$, the resulting ice thickness isThe water-equivalent thickness uses a reference water density: with fresh water at $1000\mathrm{kg}{\mathrm{m}}^{-3}$, it is $m_i/1000=\boxed{2.196\mathrm{m}\simeq 2.2\mathrm{m}}$. The depth of the original seawater removed is instead $m_i/1025=\boxed{2.143\mathrm{m}}$. These three quantities are different; $2.2\mathrm{m}$ is not the physical ice thickness for the stated density approximation.

Let the initial salinity be $S_0$. Complete exclusion of salt from the ice leaves all the initial salt in a liquid mass $M_1=M_0-m_i$. Conservation of salt during freezing givesThe initial salinity is not printed, so a unique numerical salinity increase requires another explicit assumption. For $S_0=35\mathrm{psu}$,The total density increase after cooling followed by freezing is then about $0.9464\mathrm{kg}{\mathrm{m}}^{-3}$. The factor $1/(1-f_i)$ is required because salt concentration refers to the remaining liquid mass. Using ice thickness divided by the original water depth as the removed mass fraction would violate this accounting.

For this assumed salinity, the freezing-to-cooling density efficiency shows that equal heat extraction at freezing produces about $0.7664/0.18=\boxed{4.26}$ times the density increase of the initial cooling. At low temperature the thermal expansion response is weak, whereas brine rejection changes salinity efficiently. This supports strong freezing-driven convection where water is already near its freezing point. It does not mean freezing always creates deep chimneys: the initial density stratification, freshwater supply, mixing depth and later melting remain decisive. The freezing point itself decreases as salinity rises; keeping it at $-1.8^{\circ }\mathrm{C}$ is the exam's approximation. Allowing that small additional cooling and a temperature-dependent equation of state would require a refined heat budget.

Important other sites of freezing-enhanced downward transfer include the Ross and Weddell Antarctic shelves and their coastal polynyas, Adélie Land and Cape Darnley, Arctic shelves such as the Barents and Kara Seas, and the Sea of Okhotsk. On shelves the saline dense water can cascade down a continental slope and feed deeper waters; the same salt-removal balance operates without requiring an isolated open-ocean chimney. A later direct observational example is bottom-water formation associated with Cape Darnley sea-ice production.

Atmospheric warming of the Greenland Sea can reduce surface cooling and ice formation, while increased freshwater input can inhibit convection. If these changes weaken the Atlantic meridional overturning circulation and its northward heat transport, their ocean-mediated tendency is relative cooling, or reduced warming, of northwestern Europe compared with otherwise identical atmospheric warming. This is not a prediction of net European cooling under all emissions scenarios, nor does one chimney determine the whole overturning circulation: other convection regions, winds, freshwater pathways and coupled ocean adjustment also matter. The physical conclusion is the sign of the heat-transport response, not a specified century-scale temperature decrement.

It is important to distinguish loss of forward-going surface-gravity-wave energy from conversion of mechanical energy into heat. Scattering attenuation by ice floes redirects energy; it can attenuate a coherent transmitted wave without dissipating the total energy.

For fixed floe geometry, increasing frequency usually increases attenuation over the relevant swell range: shorter wavelengths respond more strongly to the contrast between water and the elastic plate, and to repeated floe edges. Long surface gravity waves have weak curvature and often penetrate much farther. This is a trend over a specified frequency range, not a theorem excluding resonances.

The diameter dependence is governed by $d/\lambda$. An ice floe much smaller than the wavelength moves nearly with the water and scatters weakly. Scattering becomes appreciable when floe size is comparable with the wavelength, and interference between its two edges can give maxima and minima. At fixed ice concentration, larger ice floes also mean fewer edges per unit propagation distance, roughly proportional to $p/d$. Consequently the attenuation coefficient need not increase monotonically with diameter: the single-floe reflection and the number of encounters must both be considered. Thickness increases areal inertia as ${\rho }_{i}h$ and bending stiffness as $h^3$, generally increasing wave mismatch and reflection, although detailed frequency-dependent resonances again prevent a universal monotonic law.

When $d\ll \lambda$, particularly for frazil ice and pancake ice, weak individual scattering leaves other processes dominant. Relative crystal and water motion causes viscous dissipation; an aggregate layer can behave as a viscous or viscoelastic material, and pancake ice collisions, rubbing and overwash remove energy. Their importance depends on concentration and wave amplitude.

For a uniform continuous sheet with horizontal dimensions much greater than the wavelength, there are no repeated floe edges in its interior. A perfectly elastic sheet over inviscid water supports undamped flexural-gravity waves, so internal scattering is not an explanation of decay there. Real attenuation can instead arise from internal ice anelasticity or viscoelasticity, a dissipative sub-ice viscous boundary layer, turbulence, cracks and brine-related processes. Small-floe mixtures and continuous sheets require dissipation models beyond the isolated-floe scattering picture.

The simplest Pease polynya model balances offshore ice export at speed $U$ against production of new ice at thickness rate $F$ within an open strip of width $L$. Newly formed ice is collected into an edge of prescribed thickness $H$, with negligible residence time. Per unit coastline length, conservation gives $H(U-\dot{L})=FL$. For constant positive parameters,Thus the equilibrium width is $HU/F$ and the relaxation time is $H/F$. If warming reduces $F$ while $U,H$ stay fixed, both increase. With $F\le 0$ the positive-freezing equilibrium ceases to apply. Finite frazil ice residence, variable atmospheric forcing and alongshore transport require extensions of the model.

The sea-ice crystal fabric describes grain shapes and crystallographic orientations. Calm-water congelation ice tends to develop vertical columns with predominantly horizontal crystal c-axes, whereas accumulated frazil ice produces a granular texture with much less systematic orientation.

// Target: geophysics.bigb

Represent disconnected frazil ice and pancake ice as an upper layer with effective density, thickness and viscosity, rather than a continuous elastic plate. Linear Navier-Stokes equations in that layer are coupled to underlying water through velocity and stress conditions. A complex wavenumber describes both dispersion and wave attenuation in sea ice. A simpler conservative limit keeps ice mass loading but removes the elastic bending term; it does not predict viscous attenuation. The suspension model's effective viscosity is a fitted property, and a compact pancake cover need not behave like dilute frazil.