#convection — Public Fediverse posts

Convection Inside the Mantle

Most of what we know about Earth’s interior comes from observing how seismic waves–mostly from earthquakes–bounce around. As our observations have gotten better–more seisometers, better imaging techniques–scientists have identified two large anomalies sitting near the bottom of the mantle. Known as large low-velocity provinces, or LLVPs, these zones take up continent-sized areas beneath parts of Africa and the Pacific.

The LLVPs are hot, which would normally make them buoyant, but their stationary nature suggests they are made up of extremely dense material. Narrow plumes of hot material make their way up from the LLVPs to form volcanic hotspots like those that made the Hawaiian and Galapagos Islands. Balancing that upward convection is the downward convection of former tectonic material carried into the mantle at subduction zones.

What the LLVPs are made of remains an active research question. One suggestion is that they contain remnants of Theia, the planet thought to have impacted the proto-Earth to form our Moon. (Image credits: E. Garnero and C. Richardson; see also Physics Today)

Convection Inside the Mantle

Most of what we know about Earth’s interior comes from observing how seismic waves–mostly from earthquakes–bounce around. As our observations have gotten better–more seisometers, better imaging techniques–scientists have identified two large anomalies sitting near the bottom of the mantle. Known as large low-velocity provinces, or LLVPs, these zones take up continent-sized areas beneath parts of Africa and the Pacific.

The LLVPs are hot, which would normally make them buoyant, but their stationary nature suggests they are made up of extremely dense material. Narrow plumes of hot material make their way up from the LLVPs to form volcanic hotspots like those that made the Hawaiian and Galapagos Islands. Balancing that upward convection is the downward convection of former tectonic material carried into the mantle at subduction zones.

What the LLVPs are made of remains an active research question. One suggestion is that they contain remnants of Theia, the planet thought to have impacted the proto-Earth to form our Moon. (Image credits: E. Garnero and C. Richardson; see also Physics Today)

Convection Inside the Mantle

Most of what we know about Earth’s interior comes from observing how seismic waves–mostly from earthquakes–bounce around. As our observations have gotten better–more seisometers, better imaging techniques–scientists have identified two large anomalies sitting near the bottom of the mantle. Known as large low-velocity provinces, or LLVPs, these zones take up continent-sized areas beneath parts of Africa and the Pacific.

The LLVPs are hot, which would normally make them buoyant, but their stationary nature suggests they are made up of extremely dense material. Narrow plumes of hot material make their way up from the LLVPs to form volcanic hotspots like those that made the Hawaiian and Galapagos Islands. Balancing that upward convection is the downward convection of former tectonic material carried into the mantle at subduction zones.

What the LLVPs are made of remains an active research question. One suggestion is that they contain remnants of Theia, the planet thought to have impacted the proto-Earth to form our Moon. (Image credits: E. Garnero and C. Richardson; see also Physics Today)

Convection Inside the Mantle

Most of what we know about Earth’s interior comes from observing how seismic waves–mostly from earthquakes–bounce around. As our observations have gotten better–more seisometers, better imaging techniques–scientists have identified two large anomalies sitting near the bottom of the mantle. Known as large low-velocity provinces, or LLVPs, these zones take up continent-sized areas beneath parts of Africa and the Pacific.

The LLVPs are hot, which would normally make them buoyant, but their stationary nature suggests they are made up of extremely dense material. Narrow plumes of hot material make their way up from the LLVPs to form volcanic hotspots like those that made the Hawaiian and Galapagos Islands. Balancing that upward convection is the downward convection of former tectonic material carried into the mantle at subduction zones.

What the LLVPs are made of remains an active research question. One suggestion is that they contain remnants of Theia, the planet thought to have impacted the proto-Earth to form our Moon. (Image credits: E. Garnero and C. Richardson; see also Physics Today)

Convection Inside the Mantle

Most of what we know about Earth’s interior comes from observing how seismic waves–mostly from earthquakes–bounce around. As our observations have gotten better–more seisometers, better imaging techniques–scientists have identified two large anomalies sitting near the bottom of the mantle. Known as large low-velocity provinces, or LLVPs, these zones take up continent-sized areas beneath parts of Africa and the Pacific.

The LLVPs are hot, which would normally make them buoyant, but their stationary nature suggests they are made up of extremely dense material. Narrow plumes of hot material make their way up from the LLVPs to form volcanic hotspots like those that made the Hawaiian and Galapagos Islands. Balancing that upward convection is the downward convection of former tectonic material carried into the mantle at subduction zones.

What the LLVPs are made of remains an active research question. One suggestion is that they contain remnants of Theia, the planet thought to have impacted the proto-Earth to form our Moon. (Image credits: E. Garnero and C. Richardson; see also Physics Today)

“Inferno”

Nothing showcases the incredible power of our atmosphere like storms, and no one does stormchase photography like Mike Olbinski. In this vignette, he shows a stunning line of supercells caught near sunset on July 17, 2022. The high shear–combined with the setting sun–put on an incredible show. Dust blown up in a haboob, microbursts and downpours in the distance, and lots of churning, roiling turbulence. (Video and image credit: M. Olbinski)

“Inferno”

Nothing showcases the incredible power of our atmosphere like storms, and no one does stormchase photography like Mike Olbinski. In this vignette, he shows a stunning line of supercells caught near sunset on July 17, 2022. The high shear–combined with the setting sun–put on an incredible show. Dust blown up in a haboob, microbursts and downpours in the distance, and lots of churning, roiling turbulence. (Video and image credit: M. Olbinski)

“Inferno”

Nothing showcases the incredible power of our atmosphere like storms, and no one does stormchase photography like Mike Olbinski. In this vignette, he shows a stunning line of supercells caught near sunset on July 17, 2022. The high shear–combined with the setting sun–put on an incredible show. Dust blown up in a haboob, microbursts and downpours in the distance, and lots of churning, roiling turbulence. (Video and image credit: M. Olbinski)

“Inferno”

Nothing showcases the incredible power of our atmosphere like storms, and no one does stormchase photography like Mike Olbinski. In this vignette, he shows a stunning line of supercells caught near sunset on July 17, 2022. The high shear–combined with the setting sun–put on an incredible show. Dust blown up in a haboob, microbursts and downpours in the distance, and lots of churning, roiling turbulence. (Video and image credit: M. Olbinski)

“Inferno”

Nothing showcases the incredible power of our atmosphere like storms, and no one does stormchase photography like Mike Olbinski. In this vignette, he shows a stunning line of supercells caught near sunset on July 17, 2022. The high shear–combined with the setting sun–put on an incredible show. Dust blown up in a haboob, microbursts and downpours in the distance, and lots of churning, roiling turbulence. (Video and image credit: M. Olbinski)

Some powerful #convection for your viewing pleasure. This from one of the many #thunderstorms that swept across #Belgium yesterday.

Some powerful #convection for your viewing pleasure. This from one of the many #thunderstorms that swept across #Belgium yesterday.

Some powerful #convection for your viewing pleasure. This from one of the many #thunderstorms that swept across #Belgium yesterday.

Some powerful #convection for your viewing pleasure. This from one of the many #thunderstorms that swept across #Belgium yesterday.

Some powerful #convection for your viewing pleasure. This from one of the many #thunderstorms that swept across #Belgium yesterday.

For a day that's been mostly sunny, we're getting a lot of very dramatic cloud action in Edinburgh! #convection #slomo #cloudspotting #cumulus

'torrefaction'

#Convection #Accretion #AbstractArt #Surreal #Spiral #ClimateChange #ClimateEmergency #GlobalWarming #HeatStress #MastoArt #Watercolour #Krita

'torrefaction'

#Convection #Accretion #AbstractArt #Surreal #Spiral #ClimateChange #ClimateEmergency #GlobalWarming #HeatStress #MastoArt #Watercolour #Krita

'torrefaction'

#Convection #Accretion #AbstractArt #Surreal #Spiral #ClimateChange #ClimateEmergency #GlobalWarming #HeatStress #MastoArt #Watercolour #Krita

'torrefaction'

#Convection #Accretion #AbstractArt #Surreal #Spiral #ClimateChange #ClimateEmergency #GlobalWarming #HeatStress #MastoArt #Watercolour #Krita

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Melting Can Propel Icebergs

Icebergs have long served as a metaphor for not knowing what’s going on beneath the surface. Studies like today’s are a reminder of why that is. Researchers found that asymmetric icebergs–shaped, in this case, like a right triangular prism–can self-propel as they melt. Their shape forces cold, dense meltwater to slide down the surface, generating a sinking plume that propels the ice as a whole. The team demonstrated this effect in both fresh- and saltwater. For icebergs wandering into warm waters, the effect is particularly strong and may reach levels about 10% of the magnitude of dominant propulsive forces like wind. (Image and research credit: M. Berhanu et al.; via APS)

Melting Can Propel Icebergs

Icebergs have long served as a metaphor for not knowing what’s going on beneath the surface. Studies like today’s are a reminder of why that is. Researchers found that asymmetric icebergs–shaped, in this case, like a right triangular prism–can self-propel as they melt. Their shape forces cold, dense meltwater to slide down the surface, generating a sinking plume that propels the ice as a whole. The team demonstrated this effect in both fresh- and saltwater. For icebergs wandering into warm waters, the effect is particularly strong and may reach levels about 10% of the magnitude of dominant propulsive forces like wind. (Image and research credit: M. Berhanu et al.; via APS)

Melting Can Propel Icebergs

Icebergs have long served as a metaphor for not knowing what’s going on beneath the surface. Studies like today’s are a reminder of why that is. Researchers found that asymmetric icebergs–shaped, in this case, like a right triangular prism–can self-propel as they melt. Their shape forces cold, dense meltwater to slide down the surface, generating a sinking plume that propels the ice as a whole. The team demonstrated this effect in both fresh- and saltwater. For icebergs wandering into warm waters, the effect is particularly strong and may reach levels about 10% of the magnitude of dominant propulsive forces like wind. (Image and research credit: M. Berhanu et al.; via APS)

Melting Can Propel Icebergs

Icebergs have long served as a metaphor for not knowing what’s going on beneath the surface. Studies like today’s are a reminder of why that is. Researchers found that asymmetric icebergs–shaped, in this case, like a right triangular prism–can self-propel as they melt. Their shape forces cold, dense meltwater to slide down the surface, generating a sinking plume that propels the ice as a whole. The team demonstrated this effect in both fresh- and saltwater. For icebergs wandering into warm waters, the effect is particularly strong and may reach levels about 10% of the magnitude of dominant propulsive forces like wind. (Image and research credit: M. Berhanu et al.; via APS)

Melting Can Propel Icebergs

Icebergs have long served as a metaphor for not knowing what’s going on beneath the surface. Studies like today’s are a reminder of why that is. Researchers found that asymmetric icebergs–shaped, in this case, like a right triangular prism–can self-propel as they melt. Their shape forces cold, dense meltwater to slide down the surface, generating a sinking plume that propels the ice as a whole. The team demonstrated this effect in both fresh- and saltwater. For icebergs wandering into warm waters, the effect is particularly strong and may reach levels about 10% of the magnitude of dominant propulsive forces like wind. (Image and research credit: M. Berhanu et al.; via APS)

Bioconvection

Convection isn’t always driven by temperature. Here, researchers explore the convective patterns formed by Thiovulum bacteria. These bacteria are negatively buoyant, meaning they will sink if they aren’t swimming. They also have an asymmetric moment of inertia, so any flow moving past them tends to affect their swimming direction.

When let loose in a Hele-Shaw cell with a oxygen levels that decrease with depth, the bacteria create complex convection-like patterns. They swim slowly upward in wide, slow plumes and sink in denser, narrow plumes. In other areas, they form large-scale rotating vortices. (Video and image credit: O. Kodio et al.)

Bioconvection

Convection isn’t always driven by temperature. Here, researchers explore the convective patterns formed by Thiovulum bacteria. These bacteria are negatively buoyant, meaning they will sink if they aren’t swimming. They also have an asymmetric moment of inertia, so any flow moving past them tends to affect their swimming direction.

When let loose in a Hele-Shaw cell with a oxygen levels that decrease with depth, the bacteria create complex convection-like patterns. They swim slowly upward in wide, slow plumes and sink in denser, narrow plumes. In other areas, they form large-scale rotating vortices. (Video and image credit: O. Kodio et al.)

Bioconvection

Convection isn’t always driven by temperature. Here, researchers explore the convective patterns formed by Thiovulum bacteria. These bacteria are negatively buoyant, meaning they will sink if they aren’t swimming. They also have an asymmetric moment of inertia, so any flow moving past them tends to affect their swimming direction.

When let loose in a Hele-Shaw cell with a oxygen levels that decrease with depth, the bacteria create complex convection-like patterns. They swim slowly upward in wide, slow plumes and sink in denser, narrow plumes. In other areas, they form large-scale rotating vortices. (Video and image credit: O. Kodio et al.)

Bioconvection

Convection isn’t always driven by temperature. Here, researchers explore the convective patterns formed by Thiovulum bacteria. These bacteria are negatively buoyant, meaning they will sink if they aren’t swimming. They also have an asymmetric moment of inertia, so any flow moving past them tends to affect their swimming direction.

When let loose in a Hele-Shaw cell with a oxygen levels that decrease with depth, the bacteria create complex convection-like patterns. They swim slowly upward in wide, slow plumes and sink in denser, narrow plumes. In other areas, they form large-scale rotating vortices. (Video and image credit: O. Kodio et al.)

Bioconvection

Convection isn’t always driven by temperature. Here, researchers explore the convective patterns formed by Thiovulum bacteria. These bacteria are negatively buoyant, meaning they will sink if they aren’t swimming. They also have an asymmetric moment of inertia, so any flow moving past them tends to affect their swimming direction.

When let loose in a Hele-Shaw cell with a oxygen levels that decrease with depth, the bacteria create complex convection-like patterns. They swim slowly upward in wide, slow plumes and sink in denser, narrow plumes. In other areas, they form large-scale rotating vortices. (Video and image credit: O. Kodio et al.)

Aging Salty Ice

When ice forms in salty water, it starts out mushy and porous. Salt does not freeze neatly into ice’s crystalline structure, so the forming ice has pores and gaps where salty brine gathers. As the ice ages, more brine is pushed out and gradually convects downward, due to its greater density. Over time, this makes the ice layer thinner but more solid, with fewer pores. You can see a timelapse of the process in a laboratory experiment below. (Image credit: sea ice – C. Matias, experiment – F. Wang et al.; research credit: F. Wang et al.)

Aging Salty Ice

When ice forms in salty water, it starts out mushy and porous. Salt does not freeze neatly into ice’s crystalline structure, so the forming ice has pores and gaps where salty brine gathers. As the ice ages, more brine is pushed out and gradually convects downward, due to its greater density. Over time, this makes the ice layer thinner but more solid, with fewer pores. You can see a timelapse of the process in a laboratory experiment below. (Image credit: sea ice – C. Matias, experiment – F. Wang et al.; research credit: F. Wang et al.)

Aging Salty Ice

When ice forms in salty water, it starts out mushy and porous. Salt does not freeze neatly into ice’s crystalline structure, so the forming ice has pores and gaps where salty brine gathers. As the ice ages, more brine is pushed out and gradually convects downward, due to its greater density. Over time, this makes the ice layer thinner but more solid, with fewer pores. You can see a timelapse of the process in a laboratory experiment below. (Image credit: sea ice – C. Matias, experiment – F. Wang et al.; research credit: F. Wang et al.)

Aging Salty Ice

When ice forms in salty water, it starts out mushy and porous. Salt does not freeze neatly into ice’s crystalline structure, so the forming ice has pores and gaps where salty brine gathers. As the ice ages, more brine is pushed out and gradually convects downward, due to its greater density. Over time, this makes the ice layer thinner but more solid, with fewer pores. You can see a timelapse of the process in a laboratory experiment below. (Image credit: sea ice – C. Matias, experiment – F. Wang et al.; research credit: F. Wang et al.)

Aging Salty Ice

When ice forms in salty water, it starts out mushy and porous. Salt does not freeze neatly into ice’s crystalline structure, so the forming ice has pores and gaps where salty brine gathers. As the ice ages, more brine is pushed out and gradually convects downward, due to its greater density. Over time, this makes the ice layer thinner but more solid, with fewer pores. You can see a timelapse of the process in a laboratory experiment below. (Image credit: sea ice – C. Matias, experiment – F. Wang et al.; research credit: F. Wang et al.)

Inside Cepheid Variable Stars

Cepheid variable stars pulsate in brightness over regular periods. That’s one reason astronomers use them as a standard candle to judge distances–even for stars well outside our galaxy. In this image, researchers display a simulation of convection inside a Cepheid eight times more massive than our sun. The colors represent vorticity, with zero vorticity in white.(Image credit: M. Stuck and J. Pratt)

Inside Cepheid Variable Stars

Cepheid variable stars pulsate in brightness over regular periods. That’s one reason astronomers use them as a standard candle to judge distances–even for stars well outside our galaxy. In this image, researchers display a simulation of convection inside a Cepheid eight times more massive than our sun. The colors represent vorticity, with zero vorticity in white.(Image credit: M. Stuck and J. Pratt)

Inside Cepheid Variable Stars

Cepheid variable stars pulsate in brightness over regular periods. That’s one reason astronomers use them as a standard candle to judge distances–even for stars well outside our galaxy. In this image, researchers display a simulation of convection inside a Cepheid eight times more massive than our sun. The colors represent vorticity, with zero vorticity in white.(Image credit: M. Stuck and J. Pratt)

Inside Cepheid Variable Stars

Cepheid variable stars pulsate in brightness over regular periods. That’s one reason astronomers use them as a standard candle to judge distances–even for stars well outside our galaxy. In this image, researchers display a simulation of convection inside a Cepheid eight times more massive than our sun. The colors represent vorticity, with zero vorticity in white.(Image credit: M. Stuck and J. Pratt)

Inside Cepheid Variable Stars

Cepheid variable stars pulsate in brightness over regular periods. That’s one reason astronomers use them as a standard candle to judge distances–even for stars well outside our galaxy. In this image, researchers display a simulation of convection inside a Cepheid eight times more massive than our sun. The colors represent vorticity, with zero vorticity in white.(Image credit: M. Stuck and J. Pratt)

Jupiter in a Lab

The vivid bands of a gas giant like Jupiter come from the planet’s combination of rotation and convection. It’s possible to create the same effect in a lab by rapidly spinning a tank of water around a central ice core. That’s the physical set-up behind this research poster–note the illustration in the lower right corner. The central snapshots show how temperature gradients on the water surface change the faster the tank rotates. At higher rotational speeds, the parabolic water surface gets ever steeper and Jupiter-like temperature bands form. (Image credit: C. David et al.)

Jupiter in a Lab

The vivid bands of a gas giant like Jupiter come from the planet’s combination of rotation and convection. It’s possible to create the same effect in a lab by rapidly spinning a tank of water around a central ice core. That’s the physical set-up behind this research poster–note the illustration in the lower right corner. The central snapshots show how temperature gradients on the water surface change the faster the tank rotates. At higher rotational speeds, the parabolic water surface gets ever steeper and Jupiter-like temperature bands form. (Image credit: C. David et al.)

Jupiter in a Lab

The vivid bands of a gas giant like Jupiter come from the planet’s combination of rotation and convection. It’s possible to create the same effect in a lab by rapidly spinning a tank of water around a central ice core. That’s the physical set-up behind this research poster–note the illustration in the lower right corner. The central snapshots show how temperature gradients on the water surface change the faster the tank rotates. At higher rotational speeds, the parabolic water surface gets ever steeper and Jupiter-like temperature bands form. (Image credit: C. David et al.)

Jupiter in a Lab

The vivid bands of a gas giant like Jupiter come from the planet’s combination of rotation and convection. It’s possible to create the same effect in a lab by rapidly spinning a tank of water around a central ice core. That’s the physical set-up behind this research poster–note the illustration in the lower right corner. The central snapshots show how temperature gradients on the water surface change the faster the tank rotates. At higher rotational speeds, the parabolic water surface gets ever steeper and Jupiter-like temperature bands form. (Image credit: C. David et al.)

Jupiter in a Lab

The vivid bands of a gas giant like Jupiter come from the planet’s combination of rotation and convection. It’s possible to create the same effect in a lab by rapidly spinning a tank of water around a central ice core. That’s the physical set-up behind this research poster–note the illustration in the lower right corner. The central snapshots show how temperature gradients on the water surface change the faster the tank rotates. At higher rotational speeds, the parabolic water surface gets ever steeper and Jupiter-like temperature bands form. (Image credit: C. David et al.)

Analyzing Impact Of Heat From Western Wildfires On Air Pollution In The Eastern US
--
https://www.linkedin.com/pulse/analyzing-impact-heat-from-western-wildfires-air-us-eisenstadt-fzk1e/ <-- shared LinkedIn technical article
--
https://doi.org/10.1126/science.ads1957 <-- shared paper
--
https://doi.org/10.1126/science.aea7430 <-- shared technical article / perspective
--
https://scitechdaily.com/see-how-californias-intense-wildfires-are-making-their-own-weather/ <-- shared technical article
--
#fire #wildfire #climatemodels #heat #fireheat #release #atmosphere #convection #weather #weatherpatterns #airquality #publicsafety #risk #hazard #publichealth #USA #USWest #spatialanalysis #smoke #model #modeling #factors #pollution #emissions #updraught #particulates #downwind #regional #firemanagement #mitigation #extremeweather #cost #economics #damage #planning #policy #rainfall #pluvial

Analyzing Impact Of Heat From Western Wildfires On Air Pollution In The Eastern US
--
https://www.linkedin.com/pulse/analyzing-impact-heat-from-western-wildfires-air-us-eisenstadt-fzk1e/ <-- shared LinkedIn technical article
--
https://doi.org/10.1126/science.ads1957 <-- shared paper
--
https://doi.org/10.1126/science.aea7430 <-- shared technical article / perspective
--
https://scitechdaily.com/see-how-californias-intense-wildfires-are-making-their-own-weather/ <-- shared technical article
--
#fire #wildfire #climatemodels #heat #fireheat #release #atmosphere #convection #weather #weatherpatterns #airquality #publicsafety #risk #hazard #publichealth #USA #USWest #spatialanalysis #smoke #model #modeling #factors #pollution #emissions #updraught #particulates #downwind #regional #firemanagement #mitigation #extremeweather #cost #economics #damage #planning #policy #rainfall #pluvial

Analyzing Impact Of Heat From Western Wildfires On Air Pollution In The Eastern US
--
https://www.linkedin.com/pulse/analyzing-impact-heat-from-western-wildfires-air-us-eisenstadt-fzk1e/ <-- shared LinkedIn technical article
--
https://doi.org/10.1126/science.ads1957 <-- shared paper
--
https://doi.org/10.1126/science.aea7430 <-- shared technical article / perspective
--
https://scitechdaily.com/see-how-californias-intense-wildfires-are-making-their-own-weather/ <-- shared technical article
--
#fire #wildfire #climatemodels #heat #fireheat #release #atmosphere #convection #weather #weatherpatterns #airquality #publicsafety #risk #hazard #publichealth #USA #USWest #spatialanalysis #smoke #model #modeling #factors #pollution #emissions #updraught #particulates #downwind #regional #firemanagement #mitigation #extremeweather #cost #economics #damage #planning #policy #rainfall #pluvial

Analyzing Impact Of Heat From Western Wildfires On Air Pollution In The Eastern US
--
https://www.linkedin.com/pulse/analyzing-impact-heat-from-western-wildfires-air-us-eisenstadt-fzk1e/ <-- shared LinkedIn technical article
--
https://doi.org/10.1126/science.ads1957 <-- shared paper
--
https://doi.org/10.1126/science.aea7430 <-- shared technical article / perspective
--
https://scitechdaily.com/see-how-californias-intense-wildfires-are-making-their-own-weather/ <-- shared technical article
--
#fire #wildfire #climatemodels #heat #fireheat #release #atmosphere #convection #weather #weatherpatterns #airquality #publicsafety #risk #hazard #publichealth #USA #USWest #spatialanalysis #smoke #model #modeling #factors #pollution #emissions #updraught #particulates #downwind #regional #firemanagement #mitigation #extremeweather #cost #economics #damage #planning #policy #rainfall #pluvial

Analyzing Impact Of Heat From Western Wildfires On Air Pollution In The Eastern US
--
https://www.linkedin.com/pulse/analyzing-impact-heat-from-western-wildfires-air-us-eisenstadt-fzk1e/ <-- shared LinkedIn technical article
--
https://doi.org/10.1126/science.ads1957 <-- shared paper
--
https://doi.org/10.1126/science.aea7430 <-- shared technical article / perspective
--
https://scitechdaily.com/see-how-californias-intense-wildfires-are-making-their-own-weather/ <-- shared technical article
--
#fire #wildfire #climatemodels #heat #fireheat #release #atmosphere #convection #weather #weatherpatterns #airquality #publicsafety #risk #hazard #publichealth #USA #USWest #spatialanalysis #smoke #model #modeling #factors #pollution #emissions #updraught #particulates #downwind #regional #firemanagement #mitigation #extremeweather #cost #economics #damage #planning #policy #rainfall #pluvial

Mesoscale Discussion 2145 (not yet posted), but that includes #SanLuisObispoCounty #SantaBarbaraCounty #VenturaCounty

Will be here, soon:
https://www.spc.noaa.gov/products/md/2025/md2145.html

#CAwx #rain #convection

Mesoscale Discussion 2145 (not yet posted), but that includes #SanLuisObispoCounty #SantaBarbaraCounty #VenturaCounty

Will be here, soon:
https://www.spc.noaa.gov/products/md/2025/md2145.html

#CAwx #rain #convection

Mesoscale Discussion 2145 (not yet posted), but that includes #SanLuisObispoCounty #SantaBarbaraCounty #VenturaCounty

Will be here, soon:
https://www.spc.noaa.gov/products/md/2025/md2145.html

#CAwx #rain #convection

Mesoscale Discussion 2145 (not yet posted), but that includes #SanLuisObispoCounty #SantaBarbaraCounty #VenturaCounty

Will be here, soon:
https://www.spc.noaa.gov/products/md/2025/md2145.html

#CAwx #rain #convection

Mesoscale Discussion 2145 (not yet posted), but that includes #SanLuisObispoCounty #SantaBarbaraCounty #VenturaCounty

Will be here, soon:
https://www.spc.noaa.gov/products/md/2025/md2145.html

#CAwx #rain #convection

We will be hosting the 10th International #Conference on Rayleigh-Bénard #Turbulence in #Lyon (1-5 June 2026) !
Abstract submissions are now opened.

The aim of the conference is to bring together researchers from different fields to explore the latest advancements in high Rayleigh number #convection. A full day will review critical connections between #turbulent #thermal #convection and #geophysical processes.

More information on https://rbc2026.sciencesconf.org

#science

We will be hosting the 10th International #Conference on Rayleigh-Bénard #Turbulence in #Lyon (1-5 June 2026) !
Abstract submissions are now opened.

The aim of the conference is to bring together researchers from different fields to explore the latest advancements in high Rayleigh number #convection. A full day will review critical connections between #turbulent #thermal #convection and #geophysical processes.

More information on https://rbc2026.sciencesconf.org

#science

We will be hosting the 10th International #Conference on Rayleigh-Bénard #Turbulence in #Lyon (1-5 June 2026) !
Abstract submissions are now opened.

The aim of the conference is to bring together researchers from different fields to explore the latest advancements in high Rayleigh number #convection. A full day will review critical connections between #turbulent #thermal #convection and #geophysical processes.

More information on https://rbc2026.sciencesconf.org

#science