Tootfinder

Instagrams Teen-Konten bekommen ein filmreifes Update
Social Media für Jugendliche: Teenager bekommen bei Instagram künftig nur noch das zu sehen, was in etwa FSK 12 bei Filmen entspricht.
https://www.

🇺🇦 #NowPlaying on KEXP's #VarietyMix
Flamin’ Groovies:
🎵 Don't You Lie to Me
#FlaminGroovies
https://open.spotify.com/track/6WHI0VLB7Dr0J0505wvt6n

from my link log —
An angry rant about locales and filenames in libarchive.
https://github.com/mpv-player/mpv/commit/1e70e82baa9193f6f027338b0fab0f5078971fbe
saved 2025-10-13

stream_libarchive: workaround various types of locale braindeath · mpv-player/mpv@1e70e82
Fix that libarchive fails to return filenames for UTF-8/UTF-16 entries. The reason is that it uses locales and all that garbage, and mpv does not set a locale. Both C locales and wchar_t are shitf...

A Catalog of Filaments in the Central Molecular Zone
Richard G. Arendt, F. Yusef-Zadeh, I. Heywood
https://arxiv.org/abs/2510.12491 https://arxiv.org/pdf/2…

A Catalog of Filaments in the Central Molecular Zone
We present a catalog of 1.28 GHz radio filaments observed by MeerKAT over the innermost 200 pc of the Galaxy (roughly $\pm 1.5°$), which includes the central molecular zone (CMZ). The catalog is generated by repurposing software developed for the automated detection of filaments in solar coronal loops. There are two parts to the catalog. The first part, the main catalog, provides a point-by-point listing of locations and basic observational properties along each detected filament. The second p…

Supra-arcade downflows in an extensive fan associated with a giant quiescent solar filament eruption
Xiaoyan Xie, Katharine Reeves, Chengcai Shen, Nishu Karna, Yan Xu, Christopher Moore, Crisel Suarez, Ritesh Patel, Daniel Seaton
https://arxiv.org/abs/2509.09944

Supra-arcade downflows in an extensive fan associated with a giant quiescent solar filament eruption
We investigate the aftermath of a giant quiescent solar filament eruption on December 24, 2023. One feature of the eruption is an extensive fan above the filament channel that is about three times as wide as similar structures that appear above active regions (ARs) during solar flares. The fan contains numerous supra-arcade downflows (SADs), and we investigate the largest SADs with continuous Hinode X-ray Telescope (XRT) observations. The measured maximum width of the SADs in this event is at l…

Formation of axially modulated plasma strings by filamentation of interfering femtosecond Bessel beams
Fatemeh Mansourimanesh, Amirreza Sadeghpour, Daryoush Abdollahpour
https://arxiv.org/abs/2508.10163

Formation of axially modulated plasma strings by filamentation of interfering femtosecond Bessel beams
We numerically investigate the formation of axially modulated plasma strings through the filamentation of two interfering femtosecond Bessel beams. The constituent Bessel beams have different central spot sizes and propagate collinearly. Our results show that filamentation of these beams in air leads to the formation of intense axially modulated light filaments, and corrugated plasma strings with high modulation depths and tunable modulation periods. We find that the modulation periods of the i…

Der deutsche Filmemacher Wim Wenders wird 80!
#wimwenders #Regisseur

Wim Wenders wird 80: Der Blick des Meisters des Kinos kann eine Stadt verzaubern
Mit Filmen wie „Paris, Texas“ und „Der Himmel über Berlin“ hat Wim Wenders dem deutschen Kino auf der ganzen Welt Geltung verschafft. Jetzt wird der Meisterregisseur achtzig. Eine Hommage.

Modal analysis and optimization of swimming active filaments
John Severn, Eric Lauga
https://arxiv.org/abs/2510.09627 https://arxiv.org/pdf/2510.09627

Modal analysis and optimization of swimming active filaments
Active flexible filaments form the classical continuum framework for modelling the locomotion of spermatozoa and algae driven by the periodic oscillation of flagella. This framework also applies to the locomotion of various artificial swimmers. Classical studies have quantified the relationship between internal forcing (localised or distributed internal moments or forces) and external output (filament shape and swimming speed). In this paper, we pose locomotion as a mathematical optimisation pr…

Association of cold gas, massive galaxies, and AGNs in a filamentary protocluster traced by triple narrow-band imaging
Kazuki Daikuhara, Tadayuki Kodama, Haruka Kusakabe, Charles C. Steidel, Ichi Tanaka, Satoshi Kikuta, Hideki Umehata, Rhythm Shimakawa, Yusei Koyama, Kentaro Motohara, Masahiro Konishi, Jose Manuel Perez Martinez, Mariko Kubo, Dawn Erb, Kosuke Takahashi, Keita Fukushima

Association of cold gas, massive galaxies, and AGNs in a filamentary protocluster traced by triple narrow-band imaging
We investigate galaxy populations in the HS1700+64 protocluster at $z=2.30$, characterized by two prominent linear filaments traced by spatially extended Ly$α$ blobs. We conducted a wide area mapping of emission line galaxies across the protocluster using the unique combination of three matched narrow-band filters, corresponding to Ly$α$, H$α$, and [OIII] emission lines at $z=2.30$. We find that H$α$ emitters are strongly clustered at the intersection of the filaments, suggesting a protoclu…

Polar Filaments Capture High Latitude Solar Poloidal Field Interactions and can Foretell the Future Sunspot Cycle Amplitude before Polar Field Precursors
Srinjana Routh, Shaonwita Pal, Dibyendu Nandy, Subhamoy Chatterjee, Dipankar Banerjee, Mohd. Saleem Khan
https://arxiv.org/abs/2510.12142

Polar Filaments Capture High Latitude Solar Poloidal Field Interactions and can Foretell the Future Sunspot Cycle Amplitude before Polar Field Precursors
Polar fields at the minimum of a sunspot cycle -- which are a manifestation of the radial component of the Sun's poloidal field -- are deemed to be the best indicator of the strength of the toroidal component, and hence the amplitude of the future sunspot cycle. However, the Sun's polar magnetic fields are difficult to constrain with ground-based or space-based observations from near the plane-of-ecliptic. In this context, polar filaments -- dark, elongated structures that overlie polarity inve…