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Pat Kalla & Le Super Mojo:
🎵 Caramel
#PatKalla #LeSuperMojo
https://open.spotify.com/track/3jOG7tiQP8uvvXurZEEI2x
https://patkallalesupermojo.bandcamp.com/track/caramel

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Carme López:
🎵 CACHELOS. A César de Farbšn
#CarmeLópez
https://open.spotify.com/track/7dwXsUfbmbZPx0k7EfJk1E
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Coronal energy release by MHD avalanches II. EUV line emission from a multi-threaded coronal loop
G. Cozzo, J. Reid, P. Pagano, F. Reale, P. Testa, A. W. Hood, C. Argiroffi, A. Petralia, E. Alaimo, F. D'Anca, L. Sciortino, M. Todaro, U. Lo Cicero, M. Barbera, B. De Pontieu, J. Martinez-Sykora
https://arxiv.org/abs/2406.11701…

Coronal energy release by MHD avalanches II. EUV line emission from a multi-threaded coronal loop
MHD kink instability can trigger the fragmentation of a twisted magnetic flux tube into small-scale current sheets that dissipate as aperiodic impulsive heating events. This instability propagates as an avalanche to nearby flux tubes and leads to a nanoflare storm. Our previous work was devoted to related 3D MHD numerical modeling with a stratified and realistic atmosphere. This work addresses predictions for the EUV imaging spectroscopy of such structure and evolution of a loop, with an averag…

Anders als ursprünglich geplant, wird es einen vierten Band geben, der direkt an Band 3 anschließt und aus Fenias Sicht erzählt.
#DieRosenVonElsett funktioniert nicht chronologisch zu schreiben. Ich muss das in Szenen schreiben, wie sie mir kommen, ehe ich verbinden kann.

Jazzaria – Pond-rous
@…
https://www.clongclongmoo.org/2024/06/16/jazzaria-pond-rous/

Parameter effects on the total intensity of H I Ly{\alpha} line for a modelled coronal mass ejection and its driven shock
Beili Ying, Guanglu Shi, Li Feng, Lei Lu, Jianchao Xue, Shuting Li, Weiqun Gan, Hui Li
https://arxiv.org/abs/2406.11297

Parameter effects on the total intensity of H I Lyα line for a modelled coronal mass ejection and its driven shock
The combination of the H I Lyα (121.6 nm) line formation mechanism with ultraviolet (UV) Lyα and white-light (WL) observations provides an effective method for determining the electron temperature of coronal mass ejections (CMEs). A key to ensuring the accuracy of this diagnostic technique is the precise calculation of theoretical Lyα intensities. This study performs a modelled CME and its driven shock via the 3D MHD simulation. We generate synthetic UV and WL images of the CME and shock to …

Kelvin-Helmholtz instability and heating in oscillating loops perturbed by power-law transverse wave drivers
Konstantinos Karampelas, Tom Van Doorsselaere, Mingzhe Guo, Timothy Duckenfield, Gabriel Pelouze
https://arxiv.org/abs/2406.11700

Kelvin-Helmholtz instability and heating in oscillating loops perturbed by power-law transverse wave drivers
Instabilities in oscillating loops are believed to be essential for dissipating the wave energy and heating the solar coronal plasma. Our aim is to study the development of the Kelvin-Helmholtz (KH) instability in an oscillating loop that is driven by random footpoint motions. Using the PLUTO code, we performed 3D simulations of a straight gravitationally stratified flux tube. The loop footpoints are embedded in chromospheric plasma, in the presence of thermal conduction and an artificially bro…

Precise timing of solar flare footpoint sources from mid-infrared observations
Paulo J. A. Sim\~oes, Lyndsay Fletcher, Hugh S. Hudson, Graham S. Kerr, Matt Penn, Karla F. Lopez
https://arxiv.org/abs/2406.11361

Precise timing of solar flare footpoint sources from mid-infrared observations
Solar flares are powerful particle accelerators, and in the accepted standard flare model most of the flare energy is transported from a coronal energy-release region by accelerated electrons which stop collisionally in the chromosphere, heating and ionising the plasma, producing a broadband enhancement to the solar radiative output. We present a time-delay analysis of the infrared emission from two chromospheric sources in the flare SOL2014-09-24T17:50 taken at the McMath-Pierce telescope. By …