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@toxi@mastodon.thi.ng
2026-10-09 12:23:32

Valle dei Sogni (2026)
(Complete solitude in the valley of dreams — that's how it felt and how I will remember/cherish it...)
#FootpathFriday #LandscapePhotography #NaturePhotography

An large open cirque in an alpine valley with still partially glaciated peaks and ridges in the background and open grassy plain in the foreground. Rock & rubble deposits surrounding the creek bed, overgrown with small bushes in their rich autumn colors and some larch trees (still green). In the distance sparse forest of swiss pines on the lower mountain slopes below the talus fields and terraced rocks. Bright hazy dazy with mostly clear azure sky.
@primonatura@mstdn.social
2026-08-04 13:00:58

"Record low water levels across Europe reveal mammoth skeletons and forgotten shipwrecks – video"
#Europe #Climate #ClimateChange

@Techmeme@techhub.social
2026-09-02 01:55:49

Source: OpenAI's Astra model uses "recurrent depth", a technique that improves cost and performance but obscures the AI's reasoning, making it harder to monitor (The Information)
theinformation.com/articles/se

@der_raddler@dresden.network
2026-10-05 04:16:26

Hätte man auch schon beim ersten Mal wissen können. 🤷
🗺️ Blueprint #37 2/6
🟩🟨⬛⬛⬛⬆️
🟩🟩🟩🟩🟩🎉
#Blueprint

@cowboys@darktundra.xyz
2026-07-29 16:16:22

Cowboys Reveal ‘Tampering’ Concern on Blockbuster NFL Trade for $106 Million Superstar heavy.com/sports/nfl/dallas-co

@cosmos4u@scicomm.xyz
2026-07-15 23:29:07

An ancient sandstorm recorded by supercritical climbing wind ripple strata in Gale crater, Mars: #Curiosity Finds Evidence of an Ancient Sandstorm: science.nasa.gov/photojournal/

@v_i_o_l_a@openbiblio.social
2026-07-30 10:45:49

"What 311 academic librarians from 31 countries told us about AI"
blog.degruyter.com/what-311-ac
"The use of artificial intelligence in higher education is s…

@arXiv_astrophCO_bot@mastoxiv.page
2026-08-06 07:52:32

Non-Thermal Pressure due to Gas Motions in the Intracluster Medium: Confronting XRISM/Resolve with TNG-Cluster Simulations
Erwin T. Lau, Naomi Ota, Daisuke Nagai
arxiv.org/abs/2608.04757 arxiv.org/pdf/2608.04757 arxiv.org/html/2608.04757
arXiv:2608.04757v1 Announce Type: new
Abstract: Intracluster medium (ICM) gas motions probe cluster assembly, feedback, and non-thermal pressure support, but recent XRISM observations reveal velocity dispersions and non-thermal pressure fractions systematically lower than simulations predict, with extreme systems such as Abell 2029 falling below nearly all simulated clusters. Using the TNG-Cluster simulations, we show that the non-thermal pressure fraction depends sensitively on cool-core state and formation history, and provide a two-scale fitting function capturing both the inner cool-core suppression and outer rise of the radial profile. By forward-modeling mock XRISM observations and comparing them with both projected and intrinsic three-dimensional quantities, we find that azimuthal variations and projection effects contribute to the deficit in the observed velocity dispersion and non-thermal pressure fraction. This bias increases with radius and partially offsets the intrinsic outward rise in the true three-dimensional non-thermal pressure fraction. However, these effects cannot explain the extremely low values of the non-thermal pressure fraction observed in Abell 2029, which fall below approximately the 0th - 6th percentiles of the simulated cool-core cluster distribution at every measured radius under both the turbulence-only and turbulence-plus-bulk definitions. The remaining tension points to rare dynamical conditions or missing physics affecting the amplitude of gas motions in current ICM models.
toXiv_bot_toot

@der_raddler@dresden.network
2026-09-03 05:04:25

Dafür, dass ich oft einfach ins Blaue rate, läuft es eigentlich ganz gut.
🗺️ Blueprint #5 1/6
🟩🟩🟩🟩🟩🎉
#Blueprint

@der_raddler@dresden.network
2026-09-02 04:17:50

Heute war wieder einfach.
🗺️ Blueprint #4 1/6
🟩🟩🟩🟩🟩🎉
#Blueprint #polarcade