Results 341 to 350 of about 2,436,355 (386)
Electron characteristics in the high speed solar wind. [Review since 1976]
W. C. Feldman
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This study presents robust polyimide superhydrophobic surfaces with excellent mechanical durability, thermal stability, and chemical stability. A high‐yield and cost‐effective method to fabricate high‐aspect‐ratio polyimide surface microstructures is developed by controlling the template surface treatment, precursor molecular weight, and vacuum process
Jinpyeo Jeung+3 more
wiley +1 more source
Decoupling Degradation at the Electrode Interfaces in Prussian White Full Cells
Prussian White (PW) as a sodium‐ion battery (SIB) cathode material is advancing, having already been commercialized. Yet, capacity fade and cyanide‐related safety risks persist. By integrating Mössbauer‐ and online electrochemical mass spectrometry, this study analyzes degradation in PW cells, observing hydrogen and cyanide evolution.
Casimir Misiewicz+4 more
wiley +1 more source
The design, optimization and characterization of a new bilayer painting system is presented. The underlying layer is engineered to provide exceptional thermal insulation through the synergistic effect of hollow perlite microspheres and micrometer‐sized cellulose particles. The external painting layer is designed to induce the formation of a homogeneous
Antonino Caputo+8 more
wiley +1 more source
The siphonic energy transfer between hot solar wind and cold martian ionosphere through open magnetic flux rope. [PDF]
Xu X+14 more
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The relation of solar wind structure to hydromagnetic discontinuities
C. Alexander+3 more
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Solar Physics and Solar Wind, 2021
The solar corona produces a continuous outflow of plasma influencing the entire solar system and beyond to over a hundred of astronomical units. Due to the Sun's proximity the source regions of that wind can be observed remotely with great precision and ...
A. Rouillard+12 more
semanticscholar +1 more source
The solar corona produces a continuous outflow of plasma influencing the entire solar system and beyond to over a hundred of astronomical units. Due to the Sun's proximity the source regions of that wind can be observed remotely with great precision and ...
A. Rouillard+12 more
semanticscholar +1 more source
The current status of our understanding of the nature and origin of the solar wind is briefly reviewed, with emphasis being placed on the need for wave-particle interactions to account for the main energy source as well as details of the particle distribution functions.
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ACCELERATION OF THE SOLAR WIND
Space Science Reviews, 1982In this review, we discuss critically recent research on the acceleration of the solar wind, giving emphasis to high-speed solar wind streams emanating from solar coronal holes. We first explain why thermally driven wind models constrained by solar and interplanetary observations encounter substantial difficulties in explaining high speed streams. Then,
Tor Flå, Egil Leer, Thomas E. Holzer
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