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#convection

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Salt Fingers

Any time a fluid under gravity has areas of differing density, it convects. We’re used to thinking of this in terms of temperature — “hot air rises” — but temperature isn’t the only source of convection. Differences in concentration — like salinity in water — cause convection, too. This video shows a special, more complex case: what happens when there are two sources of density gradient, each of which diffuses at a different rate.

The classic example of this occurs in the ocean, where colder fresher water meets warmer, saltier water (and vice versa). Cold water tends to sink. So does saltier water. But since temperature and salinity move at different speeds, their competing convection takes on a shape that resembles dancing, finger-like plumes as seen here. (Video and image credit: M. Mohaghar et al.)

Arctic Melt

Temperatures in the Arctic are rising faster than elsewhere, triggering more and more melting. Photographer Scott Portelli captured a melting ice shelf protruding into the ocean in this aerial image. Across the top of the frozen landscape, streams and rivers cut through the ice, leading to waterfalls that flood the nearby ocean with freshwater. This meltwater will do more than raise ocean levels; it changes temperature and salinity in these regions, disrupting the convection that keeps our planet healthy. (Image credit: S. Portelli/OPOTY; via Colossal)

Why Icy Giants Have Strange Magnetic Fields

When Voyager 2 visited Uranus and Neptune, scientists were puzzled by the icy giants’ disorderly magnetic fields. Contrary to expectations, neither planet had a well-defined north and south magnetic pole, indicating that the planets’ thick, icy interiors must not convect the way Earth’s mantle does. Years later, other researchers suggested that the icy giants’ magnetic fields could come from a single thin, convecting layer in the planet, but how that would look remained unclear. Now a scientist thinks he has an answer.

When simulating a mixture of water, methane, and ammonia under icy giant temperature and pressure conditions, he saw the chemicals split themselves into two layers — a water-hydrogen mix capable of convection and a hydrocarbon-rich, stagnant lower layer. Such phase separation, he argues, matches both the icy giants’ gravitational fields and their odd magnetic fields. To test whether the model holds up, we’ll need another spacecraft — one equipped with a Doppler imager — to visit Uranus and/or Neptune to measure the predicted layers firsthand. (Image credit: NASA; research credit: B. Militzer; via Physics World)

How Cooling Towers Work

Power plants (and other industrial settings) often need to cool water to control plant temperatures. This usually requires cooling towers like the iconic curved towers seen at nuclear power plants. Towers like these use little to no moving parts — instead relying cleverly on heat transfer, buoyancy, and thermodynamics — to move and cool massive amounts of water. Grady breaks them down in terms of operation, structural engineering, and fluid/thermal dynamics in this Practical Engineering video. Grady’s videos are always great, but I especially love how this one tackles a highly visible piece of infrastructure from multiple engineering perspectives. (Video and image credit: Practical Engineering)

Time lapse of convective activity along a convergence line on 14 July. Infrared view, which makes the blue sky very dark and the conifers very bright.

If you're a glider pilot, this video shows that you want to be at the extreme upwind edge of the cloud formation, just under cloud base. That's the area of best lift.

Exposure interval was two seconds. This video represents about 35 minutes of elapsed time.

youtube.com/watch?v=jqKW30c1sT

[@IRAP #seminar] this Thursday at 11am. Andrea Chiavassa from the Lagrange Laboratory of the Observatoire de la Côte d'Azur will present his recent research work concerning 3D #modeling of stellar atmospheres - in particular the taking into account of the #convection phenomenon, which directly influences stellar parameters, radial velocity, chemical abundances, photometric colors and the characterization of #exoplanets.

Details+ : irap.omp.eu/event/a-viewpoint-

[#Séminaire @IRAP ] ce jeudi à 11h. Andrea Chiavassa du Laboratoire Lagrange de l'Observatoire de la Côte d'Azur présentera ses récents travaux de recherche concernant la #modélisation 3D des atmosphères stellaires - notamment la prise en compte du phénomène de #convection, qui influence directement les paramètres stellaires, la vitesse radiale, les abondances chimiques, les couleurs photométriques et la caractérisation des #exoplanètes.

Infos+ : irap.omp.eu/event/a-viewpoint-