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#turbulence — Public Fediverse posts

Live and recent posts from across the Fediverse tagged #turbulence, aggregated by home.social.

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  1. Strong magnetic fields inhibit the formation of Rayleigh Taylor instabilities at the interface between #coffee and milk in the café bombon in #Santander #turbulence

  2. Strong magnetic fields inhibit the formation of Rayleigh Taylor instabilities at the interface between #coffee and milk in the café bombon in #Santander #turbulence

  3. Strong magnetic fields inhibit the formation of Rayleigh Taylor instabilities at the interface between #coffee and milk in the café bombon in #Santander #turbulence

  4. Strong magnetic fields inhibit the formation of Rayleigh Taylor instabilities at the interface between #coffee and milk in the café bombon in #Santander #turbulence

  5. Strong magnetic fields inhibit the formation of Rayleigh Taylor instabilities at the interface between #coffee and milk in the café bombon in #Santander #turbulence

  6. 💁🏻‍♀️ TIL: 🧠🐝 A University of #Colorado #Boulder team studied how #turbulence transforms odor signals as they travel.

    Using #wind tunnels, #lasers, and real-world plume measurements, they identified three ways airflow filters, spreads, and generates odor frequencies. They argue these systematic changes encode distance and direction information #animals use for olfactory #navigation.

    👉 phys.org/news/2026-08-decoding

    #science #smell #olfaction #bees #neuroscience #physics #cuboulder #research #biology

  7. 💁🏻‍♀️ TIL: 🧠🐝 A University of #Colorado #Boulder team studied how #turbulence transforms odor signals as they travel.

    Using #wind tunnels, #lasers, and real-world plume measurements, they identified three ways airflow filters, spreads, and generates odor frequencies. They argue these systematic changes encode distance and direction information #animals use for olfactory #navigation.

    👉 phys.org/news/2026-08-decoding

    #science #smell #olfaction #bees #neuroscience #physics #cuboulder #research #biology

  8. 💁🏻‍♀️ TIL: 🧠🐝 A University of #Colorado #Boulder team studied how #turbulence transforms odor signals as they travel.

    Using #wind tunnels, #lasers, and real-world plume measurements, they identified three ways airflow filters, spreads, and generates odor frequencies. They argue these systematic changes encode distance and direction information #animals use for olfactory #navigation.

    👉 phys.org/news/2026-08-decoding

    #science #smell #olfaction #bees #neuroscience #physics #cuboulder #research #biology

  9. 💁🏻‍♀️ TIL: 🧠🐝 A University of #Colorado #Boulder team studied how #turbulence transforms odor signals as they travel.

    Using #wind tunnels, #lasers, and real-world plume measurements, they identified three ways airflow filters, spreads, and generates odor frequencies. They argue these systematic changes encode distance and direction information #animals use for olfactory #navigation.

    👉 phys.org/news/2026-08-decoding

    #science #smell #olfaction #bees #neuroscience #physics #cuboulder #research #biology

  10. 💁🏻‍♀️ TIL: 🧠🐝 A University of #Colorado #Boulder team studied how #turbulence transforms odor signals as they travel.

    Using #wind tunnels, #lasers, and real-world plume measurements, they identified three ways airflow filters, spreads, and generates odor frequencies. They argue these systematic changes encode distance and direction information #animals use for olfactory #navigation.

    👉 phys.org/news/2026-08-decoding

    #science #smell #olfaction #bees #neuroscience #physics #cuboulder #research #biology

  11. @Umbertogaetani Their simulations suggest that #water rising through narrow dykes would freeze too quickly to supply the volumes needed for features such as chaos terrain, pits, domes or ridges. #Turbulence makes this worse by enhancing heat loss, supercooling the water, producing frazil ice, and clogging the dyke.

    If correct, shallow liquid reservoirs on #Europa may form more by local in situ melting than by direct #ocean-to-surface exchange.

    #PlanetaryScience #SpacePhysics #IcyMoons

  12. @Umbertogaetani Their simulations suggest that #water rising through narrow dykes would freeze too quickly to supply the volumes needed for features such as chaos terrain, pits, domes or ridges. #Turbulence makes this worse by enhancing heat loss, supercooling the water, producing frazil ice, and clogging the dyke.

    If correct, shallow liquid reservoirs on #Europa may form more by local in situ melting than by direct #ocean-to-surface exchange.

    #PlanetaryScience #SpacePhysics #IcyMoons

  13. @Umbertogaetani Their simulations suggest that #water rising through narrow dykes would freeze too quickly to supply the volumes needed for features such as chaos terrain, pits, domes or ridges. #Turbulence makes this worse by enhancing heat loss, supercooling the water, producing frazil ice, and clogging the dyke.

    If correct, shallow liquid reservoirs on #Europa may form more by local in situ melting than by direct #ocean-to-surface exchange.

    #PlanetaryScience #SpacePhysics #IcyMoons

  14. @Umbertogaetani Their simulations suggest that #water rising through narrow dykes would freeze too quickly to supply the volumes needed for features such as chaos terrain, pits, domes or ridges. #Turbulence makes this worse by enhancing heat loss, supercooling the water, producing frazil ice, and clogging the dyke.

    If correct, shallow liquid reservoirs on #Europa may form more by local in situ melting than by direct #ocean-to-surface exchange.

    #PlanetaryScience #SpacePhysics #IcyMoons

  15. @Umbertogaetani Their simulations suggest that #water rising through narrow dykes would freeze too quickly to supply the volumes needed for features such as chaos terrain, pits, domes or ridges. #Turbulence makes this worse by enhancing heat loss, supercooling the water, producing frazil ice, and clogging the dyke.

    If correct, shallow liquid reservoirs on #Europa may form more by local in situ melting than by direct #ocean-to-surface exchange.

    #PlanetaryScience #SpacePhysics #IcyMoons

  16. Thanks to the world's most powerful solar telescope, scientists have captured the solar surface in unprecedented detail and captured photos and videos of solar plasma vortices. These images were obtained using the Inouye Telescope, the world's largest solar telescope, located atop a mountain in Hawaii. Ubiquitous magnetized Kelvin-Helmholtz instabilities at the edges of magnetic flux concentrations, long predicted theoretically, have been discovered.

    nature.com/articles/s41586-026

    #astronomy #sun #turbulence #physics #solar_dynamics #solar_activity

  17. Thanks to the world's most powerful solar telescope, scientists have captured the solar surface in unprecedented detail and captured photos and videos of solar plasma vortices. These images were obtained using the Inouye Telescope, the world's largest solar telescope, located atop a mountain in Hawaii. Ubiquitous magnetized Kelvin-Helmholtz instabilities at the edges of magnetic flux concentrations, long predicted theoretically, have been discovered.

    nature.com/articles/s41586-026

    #astronomy #sun #turbulence #physics #solar_dynamics #solar_activity

  18. Thanks to the world's most powerful solar telescope, scientists have captured the solar surface in unprecedented detail and captured photos and videos of solar plasma vortices. These images were obtained using the Inouye Telescope, the world's largest solar telescope, located atop a mountain in Hawaii. Ubiquitous magnetized Kelvin-Helmholtz instabilities at the edges of magnetic flux concentrations, long predicted theoretically, have been discovered.

    nature.com/articles/s41586-026

    #astronomy #sun #turbulence #physics #solar_dynamics #solar_activity

  19. Thanks to the world's most powerful solar telescope, scientists have captured the solar surface in unprecedented detail and captured photos and videos of solar plasma vortices. These images were obtained using the Inouye Telescope, the world's largest solar telescope, located atop a mountain in Hawaii. Ubiquitous magnetized Kelvin-Helmholtz instabilities at the edges of magnetic flux concentrations, long predicted theoretically, have been discovered.

    nature.com/articles/s41586-026

    #astronomy #sun #turbulence #physics #solar_dynamics #solar_activity

  20. Thanks to the world's most powerful solar telescope, scientists have captured the solar surface in unprecedented detail and captured photos and videos of solar plasma vortices. These images were obtained using the Inouye Telescope, the world's largest solar telescope, located atop a mountain in Hawaii. Ubiquitous magnetized Kelvin-Helmholtz instabilities at the edges of magnetic flux concentrations, long predicted theoretically, have been discovered.

    nature.com/articles/s41586-026

    #astronomy #sun #turbulence #physics #solar_dynamics #solar_activity

  21. Weekly Update from the Open Journal of Astrophysics 08/08/2026

    Although it’s holiday season for some, it’s time once more for another Saturday update of activity at the Open Journal of Astrophysics. Since the last update we have published a further four papers, bringing the number in Volume 9 (2026) to 167 and the total so far published by OJAp up to 615.

    I continue to include the posts made on our Mastodon account (on Fediscience); these announcements also show the DOI for each paper.

    The first paper to report this week was published on Tuesday 4th August in the folder Astrophysics of Galaxies with the title “Small-scale turbulence alongside large-scale turbulence in a z=1.87 star-forming galaxy with an outflowing wind, revealed by multi-point structure functions” by Itzhak Goldman (Afeka College, Israel). A previous study by the author found evidence of large and small scale turbulence in the star-forming galaxy CSWA13, suggesting that star clusters and large clumps within the galaxy could be driving this turbulence.

    The overlay for this paper is here

    You can find the officially accepted version on arXiv here and the announcement on Fediverse here:

    https://fediscience.org/@OJ_Astro/117036181269903989

    The second paper for this week, published on Thursday 6th August in the folder Astrophysics of Galaxies, is “From Clumps to Sheets: Geometry Controls the Temperature PDF of Multi-Phase Gas” by Zirui Chen and S. Peng Oh (UC Santa Barbara, USA). This study uses 3D hydrodynamic simulations to show that the temperature probability distribution functions (PDFs) of multi-phase turbulent gas differ significantly under interstellar medium (ISM) and circumgalactic medium (CGM) conditions.

    The overlay looks like this:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/117047322340826393

    The third paper of the week, published on Thursday 6th August in folder Instrumentation and Methods for Astrophysics is “First Detection of Extensive Air Showers Using a Small-Aperture Fluorescence Telescope” by M. Zotov (M.V. Lomonosov Moscow State University, Russia) and 7 others based in Russia and Armenia. The study reports the first-ever detection of extensive air showers from ultra-high-energy cosmic rays using a compact fluorescence telescope, employing both conventional and deep learning analysis methods.

    The overlay is here:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/117047408583672745

    The fourth and final paper of the week was published on Friday 7th August in the folder Cosmology and Nongalactic Astrophysics: “TDCOSMO XXVI: Uniform Lens Modeling of Eight Doubly Imaged Quasars“, by Ryan Brady (Stony Brook University, USA) and 9 others based all around the world, presents a new method for analyzing doubly imaged quasars using the Hubble Space Telescope, revealing that arc surface brightness is key to precision in mass model measurements.

    The overlay is here:

    The officially-accepted version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/117053056092162466

    That’s all for this week. We have about a dozen more papers accepted and waiting for the authors to put the final version on arXiv, which they will presumably do when they’re back from holiday. I’ll do an update next weekend and we’ll see!

    #airShowers #arXiv260114887v3 #arXiv260413154v2 #arXiv260424908v2 #arXiv260505004v2 #AstrophysicsOfGalaxies #CircumgalacticMedium #CosmologyAndNonGalacticAstrophysics #DiamondOpenAccess #DiamondOpenAccessPublishing #GalacticOutflows #GravitationalLensing #highEnergyCosmicRays #HubbleSpaceTelescope #hydrodynamicSimulations #InstrumentationAndMethodsForAstrophysics #OpenAccess #OpenAccessPublishing #peculiarVelocities #quasars #starFormingGalaxy #structureFunctions #Turbulence #ultraHighEnergyCosmicRays
  22. Weekly Update from the Open Journal of Astrophysics 08/08/2026

    Although it’s holiday season for some, it’s time once more for another Saturday update of activity at the Open Journal of Astrophysics. Since the last update we have published a further four papers, bringing the number in Volume 9 (2026) to 167 and the total so far published by OJAp up to 615.

    I continue to include the posts made on our Mastodon account (on Fediscience); these announcements also show the DOI for each paper.

    The first paper to report this week was published on Tuesday 4th August in the folder Astrophysics of Galaxies with the title “Small-scale turbulence alongside large-scale turbulence in a z=1.87 star-forming galaxy with an outflowing wind, revealed by multi-point structure functions” by Itzhak Goldman (Afeka College, Israel). A previous study by the author found evidence of large and small scale turbulence in the star-forming galaxy CSWA13, suggesting that star clusters and large clumps within the galaxy could be driving this turbulence.

    The overlay for this paper is here

    You can find the officially accepted version on arXiv here and the announcement on Fediverse here:

    https://fediscience.org/@OJ_Astro/117036181269903989

    The second paper for this week, published on Thursday 6th August in the folder Astrophysics of Galaxies, is “From Clumps to Sheets: Geometry Controls the Temperature PDF of Multi-Phase Gas” by Zirui Chen and S. Peng Oh (UC Santa Barbara, USA). This study uses 3D hydrodynamic simulations to show that the temperature probability distribution functions (PDFs) of multi-phase turbulent gas differ significantly under interstellar medium (ISM) and circumgalactic medium (CGM) conditions.

    The overlay looks like this:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/117047322340826393

    The third paper of the week, published on Thursday 6th August in folder Instrumentation and Methods for Astrophysics is “First Detection of Extensive Air Showers Using a Small-Aperture Fluorescence Telescope” by M. Zotov (M.V. Lomonosov Moscow State University, Russia) and 7 others based in Russia and Armenia. The study reports the first-ever detection of extensive air showers from ultra-high-energy cosmic rays using a compact fluorescence telescope, employing both conventional and deep learning analysis methods.

    The overlay is here:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/117047408583672745

    The fourth and final paper of the week was published on Friday 7th August in the folder Cosmology and Nongalactic Astrophysics: “TDCOSMO XXVI: Uniform Lens Modeling of Eight Doubly Imaged Quasars“, by Ryan Brady (Stony Brook University, USA) and 9 others based all around the world, presents a new method for analyzing doubly imaged quasars using the Hubble Space Telescope, revealing that arc surface brightness is key to precision in mass model measurements.

    The overlay is here:

    The officially-accepted version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/117053056092162466

    That’s all for this week. We have about a dozen more papers accepted and waiting for the authors to put the final version on arXiv, which they will presumably do when they’re back from holiday. I’ll do an update next weekend and we’ll see!

    #airShowers #arXiv260114887v3 #arXiv260413154v2 #arXiv260424908v2 #arXiv260505004v2 #AstrophysicsOfGalaxies #CircumgalacticMedium #CosmologyAndNonGalacticAstrophysics #DiamondOpenAccess #DiamondOpenAccessPublishing #GalacticOutflows #GravitationalLensing #highEnergyCosmicRays #HubbleSpaceTelescope #hydrodynamicSimulations #InstrumentationAndMethodsForAstrophysics #OpenAccess #OpenAccessPublishing #peculiarVelocities #quasars #starFormingGalaxy #structureFunctions #Turbulence #ultraHighEnergyCosmicRays
  23. Weekly Update from the Open Journal of Astrophysics 08/08/2026

    Although it’s holiday season for some, it’s time once more for another Saturday update of activity at the Open Journal of Astrophysics. Since the last update we have published a further four papers, bringing the number in Volume 9 (2026) to 167 and the total so far published by OJAp up to 615.

    I continue to include the posts made on our Mastodon account (on Fediscience); these announcements also show the DOI for each paper.

    The first paper to report this week was published on Tuesday 4th August in the folder Astrophysics of Galaxies with the title “Small-scale turbulence alongside large-scale turbulence in a z=1.87 star-forming galaxy with an outflowing wind, revealed by multi-point structure functions” by Itzhak Goldman (Afeka College, Israel). A previous study by the author found evidence of large and small scale turbulence in the star-forming galaxy CSWA13, suggesting that star clusters and large clumps within the galaxy could be driving this turbulence.

    The overlay for this paper is here

    You can find the officially accepted version on arXiv here and the announcement on Fediverse here:

    https://fediscience.org/@OJ_Astro/117036181269903989

    The second paper for this week, published on Thursday 6th August in the folder Astrophysics of Galaxies, is “From Clumps to Sheets: Geometry Controls the Temperature PDF of Multi-Phase Gas” by Zirui Chen and S. Peng Oh (UC Santa Barbara, USA). This study uses 3D hydrodynamic simulations to show that the temperature probability distribution functions (PDFs) of multi-phase turbulent gas differ significantly under interstellar medium (ISM) and circumgalactic medium (CGM) conditions.

    The overlay looks like this:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/117047322340826393

    The third paper of the week, published on Thursday 6th August in folder Instrumentation and Methods for Astrophysics is “First Detection of Extensive Air Showers Using a Small-Aperture Fluorescence Telescope” by M. Zotov (M.V. Lomonosov Moscow State University, Russia) and 7 others based in Russia and Armenia. The study reports the first-ever detection of extensive air showers from ultra-high-energy cosmic rays using a compact fluorescence telescope, employing both conventional and deep learning analysis methods.

    The overlay is here:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/117047408583672745

    The fourth and final paper of the week was published on Friday 7th August in the folder Cosmology and Nongalactic Astrophysics: “TDCOSMO XXVI: Uniform Lens Modeling of Eight Doubly Imaged Quasars“, by Ryan Brady (Stony Brook University, USA) and 9 others based all around the world, presents a new method for analyzing doubly imaged quasars using the Hubble Space Telescope, revealing that arc surface brightness is key to precision in mass model measurements.

    The overlay is here:

    The officially-accepted version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/117053056092162466

    That’s all for this week. We have about a dozen more papers accepted and waiting for the authors to put the final version on arXiv, which they will presumably do when they’re back from holiday. I’ll do an update next weekend and we’ll see!

    #airShowers #arXiv260114887v3 #arXiv260413154v2 #arXiv260424908v2 #arXiv260505004v2 #AstrophysicsOfGalaxies #CircumgalacticMedium #CosmologyAndNonGalacticAstrophysics #DiamondOpenAccess #DiamondOpenAccessPublishing #GalacticOutflows #GravitationalLensing #highEnergyCosmicRays #HubbleSpaceTelescope #hydrodynamicSimulations #InstrumentationAndMethodsForAstrophysics #OpenAccess #OpenAccessPublishing #peculiarVelocities #quasars #starFormingGalaxy #structureFunctions #Turbulence #ultraHighEnergyCosmicRays
  24. Weekly Update from the Open Journal of Astrophysics 08/08/2026

    Although it’s holiday season for some, it’s time once more for another Saturday update of activity at the Open Journal of Astrophysics. Since the last update we have published a further four papers, bringing the number in Volume 9 (2026) to 167 and the total so far published by OJAp up to 615.

    I continue to include the posts made on our Mastodon account (on Fediscience); these announcements also show the DOI for each paper.

    The first paper to report this week was published on Tuesday 4th August in the folder Astrophysics of Galaxies with the title “Small-scale turbulence alongside large-scale turbulence in a z=1.87 star-forming galaxy with an outflowing wind, revealed by multi-point structure functions” by Itzhak Goldman (Afeka College, Israel). A previous study by the author found evidence of large and small scale turbulence in the star-forming galaxy CSWA13, suggesting that star clusters and large clumps within the galaxy could be driving this turbulence.

    The overlay for this paper is here

    You can find the officially accepted version on arXiv here and the announcement on Fediverse here:

    https://fediscience.org/@OJ_Astro/117036181269903989

    The second paper for this week, published on Thursday 6th August in the folder Astrophysics of Galaxies, is “From Clumps to Sheets: Geometry Controls the Temperature PDF of Multi-Phase Gas” by Zirui Chen and S. Peng Oh (UC Santa Barbara, USA). This study uses 3D hydrodynamic simulations to show that the temperature probability distribution functions (PDFs) of multi-phase turbulent gas differ significantly under interstellar medium (ISM) and circumgalactic medium (CGM) conditions.

    The overlay looks like this:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/117047322340826393

    The third paper of the week, published on Thursday 6th August in folder Instrumentation and Methods for Astrophysics is “First Detection of Extensive Air Showers Using a Small-Aperture Fluorescence Telescope” by M. Zotov (M.V. Lomonosov Moscow State University, Russia) and 7 others based in Russia and Armenia. The study reports the first-ever detection of extensive air showers from ultra-high-energy cosmic rays using a compact fluorescence telescope, employing both conventional and deep learning analysis methods.

    The overlay is here:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/117047408583672745

    The fourth and final paper of the week was published on Friday 7th August in the folder Cosmology and Nongalactic Astrophysics: “TDCOSMO XXVI: Uniform Lens Modeling of Eight Doubly Imaged Quasars“, by Ryan Brady (Stony Brook University, USA) and 9 others based all around the world, presents a new method for analyzing doubly imaged quasars using the Hubble Space Telescope, revealing that arc surface brightness is key to precision in mass model measurements.

    The overlay is here:

    The officially-accepted version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/117053056092162466

    That’s all for this week. We have about a dozen more papers accepted and waiting for the authors to put the final version on arXiv, which they will presumably do when they’re back from holiday. I’ll do an update next weekend and we’ll see!

    #airShowers #arXiv260114887v3 #arXiv260413154v2 #arXiv260424908v2 #arXiv260505004v2 #AstrophysicsOfGalaxies #CircumgalacticMedium #CosmologyAndNonGalacticAstrophysics #DiamondOpenAccess #DiamondOpenAccessPublishing #GalacticOutflows #GravitationalLensing #highEnergyCosmicRays #HubbleSpaceTelescope #hydrodynamicSimulations #InstrumentationAndMethodsForAstrophysics #OpenAccess #OpenAccessPublishing #peculiarVelocities #quasars #starFormingGalaxy #structureFunctions #Turbulence #ultraHighEnergyCosmicRays
  25. This is the exciting part: #KHI can mix magnetized and non-magnetized #plasma, drive #turbulence, transport mass/energy/momentum/ #MagneticFlux, and may contribute to small-scale #magnetic braiding, thus one route by which free #MagneticEnergy is built up in the solar #atmosphere.

    That makes them relevant to the long-standing puzzle of why the #corona is heated to millions of kelvin while the visible surface is only ~5,800 K. 😎🔥

    #SolarPhysics #PlasmaPhysics #SpacePhysics #KHI

  26. This is the exciting part: #KHI can mix magnetized and non-magnetized #plasma, drive #turbulence, transport mass/energy/momentum/ #MagneticFlux, and may contribute to small-scale #magnetic braiding, thus one route by which free #MagneticEnergy is built up in the solar #atmosphere.

    That makes them relevant to the long-standing puzzle of why the #corona is heated to millions of kelvin while the visible surface is only ~5,800 K. 😎🔥

    #SolarPhysics #PlasmaPhysics #SpacePhysics #KHI

  27. This is the exciting part: #KHI can mix magnetized and non-magnetized #plasma, drive #turbulence, transport mass/energy/momentum/ #MagneticFlux, and may contribute to small-scale #magnetic braiding, thus one route by which free #MagneticEnergy is built up in the solar #atmosphere.

    That makes them relevant to the long-standing puzzle of why the #corona is heated to millions of kelvin while the visible surface is only ~5,800 K. 😎🔥

    #SolarPhysics #PlasmaPhysics #SpacePhysics #KHI

  28. This is the exciting part: #KHI can mix magnetized and non-magnetized #plasma, drive #turbulence, transport mass/energy/momentum/ #MagneticFlux, and may contribute to small-scale #magnetic braiding, thus one route by which free #MagneticEnergy is built up in the solar #atmosphere.

    That makes them relevant to the long-standing puzzle of why the #corona is heated to millions of kelvin while the visible surface is only ~5,800 K. 😎🔥

    #SolarPhysics #PlasmaPhysics #SpacePhysics #KHI

  29. This is the exciting part: #KHI can mix magnetized and non-magnetized #plasma, drive #turbulence, transport mass/energy/momentum/ #MagneticFlux, and may contribute to small-scale #magnetic braiding, thus one route by which free #MagneticEnergy is built up in the solar #atmosphere.

    That makes them relevant to the long-standing puzzle of why the #corona is heated to millions of kelvin while the visible surface is only ~5,800 K. 😎🔥

    #SolarPhysics #PlasmaPhysics #SpacePhysics #KHI

  30. The anti-tourism guides revealing Lisbon’s true, radical heart

    Manu joined We Hate Tourism a decade later, arriving through Lisbon’s skateboarding and street-art scene. He possesses the unnerving…
    #Portugal #PT #Europe #Europa #EU #backdrop #capital #crisis #fuelled #housing #millions #noticias #people #political #portugal #Portuguese #sees #short #Tours #turbulence #visit #year
    europesays.com/3177997/

  31. Speaking of #turbulence (mastodon.social/@franco_vazza/) here is instead the simulated version of it, for the plasma conditions of the hot x-ray halo of the Milky Way (about one million degrees Kelvin)

    This shows the possibile outcome of stationary driven turbulence in a small portion of it, using supersonic forcing in the ENZO code #astrophysics #physics #science

  32. Speaking of #turbulence (mastodon.social/@franco_vazza/) here is instead the simulated version of it, for the plasma conditions of the hot x-ray halo of the Milky Way (about one million degrees Kelvin)

    This shows the possibile outcome of stationary driven turbulence in a small portion of it, using supersonic forcing in the ENZO code #astrophysics #physics #science

  33. Speaking of #turbulence (mastodon.social/@franco_vazza/) here is instead the simulated version of it, for the plasma conditions of the hot x-ray halo of the Milky Way (about one million degrees Kelvin)

    This shows the possibile outcome of stationary driven turbulence in a small portion of it, using supersonic forcing in the ENZO code #astrophysics #physics #science

  34. Speaking of #turbulence (mastodon.social/@franco_vazza/) here is instead the simulated version of it, for the plasma conditions of the hot x-ray halo of the Milky Way (about one million degrees Kelvin)

    This shows the possibile outcome of stationary driven turbulence in a small portion of it, using supersonic forcing in the ENZO code #astrophysics #physics #science

  35. Speaking of #turbulence (mastodon.social/@franco_vazza/) here is instead the simulated version of it, for the plasma conditions of the hot x-ray halo of the Milky Way (about one million degrees Kelvin)

    This shows the possibile outcome of stationary driven turbulence in a small portion of it, using supersonic forcing in the ENZO code #astrophysics #physics #science

  36. #Turbulence is probably the complex emergent phenomenon we can observe in a more iniquitous way, at all scales, epochs and in all environments. It is also continuously around us on Earth, although we don't often pay attention to it - and sometimes it is just a nuisance.

    Here a short parade of turbulence I randomly recorded (or generated) around me in these latest years

    1. Droplets of coffee in milk

    #physics #science #fluids

  37. #Turbulence is probably the complex emergent phenomenon we can observe in a more iniquitous way, at all scales, epochs and in all environments. It is also continuously around us on Earth, although we don't often pay attention to it - and sometimes it is just a nuisance.

    Here a short parade of turbulence I randomly recorded (or generated) around me in these latest years

    1. Droplets of coffee in milk

    #physics #science #fluids

  38. #Turbulence is probably the complex emergent phenomenon we can observe in a more iniquitous way, at all scales, epochs and in all environments. It is also continuously around us on Earth, although we don't often pay attention to it - and sometimes it is just a nuisance.

    Here a short parade of turbulence I randomly recorded (or generated) around me in these latest years

    1. Droplets of coffee in milk

    #physics #science #fluids

  39. #Turbulence is probably the complex emergent phenomenon we can observe in a more iniquitous way, at all scales, epochs and in all environments. It is also continuously around us on Earth, although we don't often pay attention to it - and sometimes it is just a nuisance.

    Here a short parade of turbulence I randomly recorded (or generated) around me in these latest years

    1. Droplets of coffee in milk

    #physics #science #fluids

  40. #Turbulence is probably the complex emergent phenomenon we can observe in a more iniquitous way, at all scales, epochs and in all environments. It is also continuously around us on Earth, although we don't often pay attention to it - and sometimes it is just a nuisance.

    Here a short parade of turbulence I randomly recorded (or generated) around me in these latest years

    1. Droplets of coffee in milk

    #physics #science #fluids