Results 71 to 80 of about 960,034 (278)
Effect of motions in prominences on the helium resonance lines in the extreme ultraviolet [PDF]
<b>Context</b>: Extreme ultraviolet resonance lines of neutral and ionised helium observed in prominences are difficult to interpret as the prominence plasma is optically thick at these wavelengths. If mass motions are taking place, as is the
N. Labrosse +5 more
core +1 more source
Our work introduces a new framework that fundamentally changes how orientation in bismuth oxyhalide systems is approached. Comprehensive experiments, backed by theoretical models, reveal the pivotal role of halide anions to modify the van der Waals stacking energies required to direct orientation. Our method enables the fabrication of near perfect (001)
Gabriel Aygur +10 more
wiley +1 more source
Non-linear force-free magnetic dip models of quiescent prominence fine structures [PDF]
S.G. and P.H. acknowledge the support from grant 209/12/0906 of the Grant Agency of the Czech Republic. P.H. acknowledges the support from grant P209/10/1680 of the Grant Agency of the Czech Republic. S.G. and P.H.
Mackay, D. +11 more
core +1 more source
Alkoxy chain length drives a continuous transition from eclipsed AA to a serrated, slipped AA* configuration over Co‐porphyrin COFs. A moderate slip both contracts the pore channel to enrich CO2 and suppress hydrogen evolution, and enhances collective high‐spin of Co sites, which delivers a record CO production rate with high selectivity.
Jie He +8 more
wiley +1 more source
Water harvesting, radiative cooling, and interfacial solar evaporation are fundamentally governed by coupled heat, mass, and light transport processes. These processes are mediated by pore architecture, including pore size, connectivity, and hierarchical organization.
Dejan J. Trajkovski +5 more
wiley +1 more source
Statistical Study of Solar Prominence Plumes Based on NVST Hα Observations
Plumes are one of the most representative dynamic features observed in prominences and play a key role in mass and magnetic transport within them. However, their physical nature and triggering processes remain actively debated.
Yangrui Chen +11 more
doaj +1 more source
Laboratory simulations of solar prominences [PDF]
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in .pdf document. A solar prominence is a large, arch-shaped structure of magnetized hydrogen plasma protruding from the surface of the sun.
Hansen, John Freddy
core +1 more source
Environmental Synthesis Radar (ESR) evaluates the environmental impact of (early‐stage) multi‐step chemical syntheses, providing a holistic view by using 18 midpoint impact categories. Unlike conventional life‐cycle assessment (LCA) approaches, ESR reveals three complementary metrics: overall impact Vtotal, environmental hotspots VEF, and critical ...
Laura Plein +8 more
wiley +1 more source
Coronal Prominence Cavities: A Survey across the Solar Cycle
Coronal prominences are involved in many coronal mass ejections (CMEs), but the prominence traces only a portion of the 3D magnetic field of the core of the CME.
Urszula Ba̧k-Stȩślicka +2 more
doaj +1 more source
A Dynamical Model of Solar Prominences with Current Sheet [PDF]
Recent observations of solar prominences show that slow upward motions ( ≌ 1 kms^ ) occur through quiescent prominences and a fast input of material with horizontal motions ( ≌ 5 kms^ ) occurs at both edges of prominences.
鷲見, 治一, 坂井, 純一
core +1 more source

