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Ice streams are bands of fast-flowing ice in ice sheets. We investigate their formation as an example of spontaneous pattern formation, based on positive feedbacks between dissipation and basal sliding. Our focus is on temperature-dependent…

Fluid Dynamics · Physics 2020-11-06 Christian Schoof , Elisa Mantelli

Frozen water might appear opaque since gas bubbles can get trapped in the ice during the freezing process. They nucleate and then grow near the advancing solidification front, due to the formation of a gas supersaturation region in its…

We report a 2D modeling of the thermal diffusion-controlled growth of a vapor bubble attached to a heating surface during saturated boiling. The heat conduction problem is solved in a liquid that surrounds a bubble with a free boundary and…

Fluid Dynamics · Physics 2016-01-27 Vadim Nikolayev , Daniel Beysens , G. -L. Lagier , J. Hegseth

Aims. We track the time evolution of planet traps and snowlines in a viscously evolving protoplanetary disk using an opacity table that accounts for the composition of the dust material. Methods. We coupled a dynamical and thermodynamical…

Earth and Planetary Astrophysics · Physics 2015-05-06 Kévin Baillié , Sébastien Charnoz , Éric Pantin

Around the snow line, icy pebbles and silicate dust may locally pile-up and form icy and rocky planetesimals via streaming instability and/or gravitational instability. We perform 1D diffusion-advection simulations that include the…

Earth and Planetary Astrophysics · Physics 2021-02-03 Ryuki Hyodo , Tristan Guillot , Shigeru Ida , Satoshi Okuzumi , Andrew N. Youdin

Protoplanetary disks naturally emerge during protostellar core-collapse. In their early evolutionary stages, infalling material dominates their dynamical evolution. In the context of planet formation, this means that the conditions in young…

Earth and Planetary Astrophysics · Physics 2025-04-23 L. -A. Hühn , C. P. Dullemond , U. Lebreuilly , R. S. Klessen , A. Maury , G. P. Rosotti , P. Hennebelle , E. Pacetti , L. Testi , S. Molinari

Solar prominences are cool and dense plasma structures floating in the hot solar corona. They are ubiquitous features in the solar atmosphere, but their formation mechanism is still unclear. Here we perform comprehensive fully…

Solar and Stellar Astrophysics · Physics 2026-05-04 Lisa-Marie Zessner , Robert H. Cameron , Sami K. Solanki , Damien Przybylski

Snow crystals growing from water vapor occasionally exhibit morphologies with three-fold (trigonal) symmetry, even though the ice crystal lattice has a molecular structure with six-fold symmetry. In extreme cases, thin platelike snow…

Materials Science · Physics 2021-06-21 Kenneth G. Libbrecht

There are three fundamental physical processes that gives rise to the morphology of a surface: deposition, surface diffusion and desorption. The characteristics of the interfaces generated by the combination of deposition and surface…

Statistical Mechanics · Physics 2007-05-23 Juan R. Sanchez

We describe observations of a novel hysteresis behavior in the growth of ice crystals under near-vacuum conditions. Above a threshold supersaturation, we find that the ice growth rate often exhibits a sudden increase that we attribute to an…

Materials Science · Physics 2008-09-30 Kenneth G. Libbrecht

We propose a new type of morphological instability in the diffusion-limited growth of faceted crystals from the vapor phase that can explain the formation of thin ice plates at temperatures near -15 C. The instability appears when the…

Materials Science · Physics 2007-05-23 Kenneth G. Libbrecht

The effect of turbulence on snow precipitation is not incorporated into present weather forecasting models. Here we show evidence that turbulence is in fact a key influence on both fall speed and spatial distribution of settling snow. We…

Sea ice is a key component of the Earth's climate system, making its aging process an essential focus of current research. The age of sea ice is closely linked to its thermal and mechanical properties, which govern its interactions with the…

Fluid Dynamics · Physics 2025-09-09 Yihong Du , Feng Wang , Enrico Calzavarini , Chao Sun

The temperature of newly forming dust is controlled by the radiation field. As dust forms around stars, stellar transients, quasars or supernovae, the grains must grow through a regime where they are stochastically heated by individual…

Solar and Stellar Astrophysics · Physics 2014-07-31 C. S. Kochanek

A glacier table consists of a rock supported by a slender column of ice and form naturally on glaciers. We investigate the onset of their formation at a smaller scale in a controlled environment. Depending on the size and thermal…

Fluid Dynamics · Physics 2021-09-10 Marceau Hénot , Nicolas Plihon , Nicolas Taberlet

We revisit the computation of a "snow line" in a passive protoplanetary disk during the stage of planetesimal formation. We examine how shadowing and illumination in the vicinity of a planet affects where in the disk ice can form, making…

Astrophysics · Physics 2009-11-10 Hannah Jang-Condell , Dimitar D. Sasselov

In this work we show that modifying the thermal history of the Universe by including an early period of matter domination can lead to the formation of astronomical objects. However, the survival of these objects can only be possible if the…

High Energy Physics - Phenomenology · Physics 2015-06-17 Gabriela Barenboim , Javier Rasero

It is proposed that primary nucleation of amorphous microspherulites of hydrated silica in natural proto-precious-opal can be followed by a long range superlattice ordering process by means of electrostatic self-assembly. Necessary…

Materials Science · Physics 2010-01-05 A. M. Stewart , Lewis T. Chadderton , Brian R. Senior

Spinning ice discs in nature have been reported for more than a century, yet laboratory experiments have yielded diverse observations and contradictory explanations, leaving the mechanism behind the disc motion elusive. Here we combine…

Fluid Dynamics · Physics 2025-11-18 Min Li , Lailai Zhu

Powder snow avalanches are highly dynamic, multiphase gravity-driven flows typically composed of a dense basal layer overlain by airborne layers in which snow particles are suspended within a turbulent air phase. Despite extensive work on…

Geophysics · Physics 2026-03-31 Ivan Calic , Filippo Coletti , Betty Sovilla