Solar wind turbulence refers to the complex, chaotic fluid motions and magnetic field fluctuations observed in the solar wind plasma as it flows outward...
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Sun (redirect from Solar diameter)
where the solar wind dominates over the interstellar medium. Turbulence and dynamic forces in the heliosphere cannot affect the shape of the solar corona...
174 KB (19,374 words) - 10:52, 28 May 2025
The solar wind is a stream of charged particles released from the Sun's outermost atmospheric layer, the corona. This plasma mostly consists of electrons...
57 KB (6,717 words) - 12:33, 29 May 2025
accuracy. OTUR focused on detecting and analyzing turbulence in Venus's upper atmosphere and the solar wind. By examining fluctuations in radio signal properties...
44 KB (4,379 words) - 17:00, 20 May 2025
satellites"), that will measure solar wind turbulence - fluctuations in the magnetic field and motions of the solar wind. The mission PI is Harlan Spence...
3 KB (129 words) - 03:41, 6 January 2025
Heliosphere (section Solar wind)
its solar wind moves "away" from the Sun supersonically. When the interstellar wind hits the heliosphere it slows and creates a region of turbulence. A...
63 KB (6,577 words) - 12:30, 3 March 2025
the center to about 0.2 of the solar radius (139,000 km; 86,000 mi). It is the hottest part of the Sun and of the Solar System. It has a density of 150...
14 KB (1,893 words) - 21:12, 15 April 2025
magnetosheath turbulence April 9 - The Solar-cycle Variations of the Anisotropy of Taylor Scale and Correlation Scale in the Solar Wind Turbulence February...
144 KB (12,933 words) - 15:54, 22 May 2025
In solar physics, a prominence, sometimes referred to as a filament, is a large plasma and magnetic field structure extending outward from the Sun's surface...
17 KB (1,885 words) - 11:39, 21 March 2025
experiment to study the upper atmosphere a radio science atmospheric and solar wind turbulence experiment a gamma ray burst detector to record gamma-ray burst...
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modelling, experiments, and observations (e.g., solar wind). Magnetohydrodynamics Turbulence Alfvén wave Solar dynamo Reynolds number Navier–Stokes equations...
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sequence stars below about 0.3 solar masses are entirely convective, meaning they do not have a radiative zone. From 0.3 to 1.2 solar masses, the region around...
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of which is visible in the Sun as solar granulation. Low-mass main-sequence stars, such as red dwarfs below 0.35 solar masses, as well as pre-main sequence...
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the solar wind passes Earth. The flow of plasma into the magnetosphere increases with additional turbulence, density, and speed in the solar wind. This...
116 KB (12,892 words) - 21:18, 24 May 2025
Copper in renewable energy (redirect from Copper in solar panels)
Renewable energy sources such as solar, wind, tidal, hydro, biomass, and geothermal have become significant sectors of the energy market. The rapid growth...
59 KB (7,263 words) - 22:24, 13 November 2024
hours, to global winds resulting from the difference in absorption of solar energy between the climate zones on Earth. The study of wind is called anemology...
106 KB (11,246 words) - 16:17, 18 May 2025
is a type of dry, relatively warm downslope wind in the lee of a mountain range. It is a rain shadow wind that results from the subsequent adiabatic warming...
20 KB (2,388 words) - 01:23, 26 May 2025
The Parker Solar Probe (PSP; previously Solar Probe, Solar Probe Plus or Solar Probe+) is a NASA space probe launched in 2018 to make observations of...
95 KB (8,589 words) - 18:27, 19 May 2025
building height it is near the optimum for maximum wind energy and minimum wind turbulence. While wind speeds within the built environment are generally...
85 KB (9,111 words) - 16:39, 26 May 2025
around the telescope is heated, which causes turbulence and degrades the resolution. To alleviate this, solar telescopes are usually built on towers and...
17 KB (1,884 words) - 02:50, 30 May 2025
Solar phenomena are natural phenomena which occur within the atmosphere of the Sun. They take many forms, including solar wind, radio wave flux, solar...
48 KB (5,256 words) - 11:03, 24 May 2025
polar cyclone. In areas where winds tend to be light, the sea breeze-land breeze cycle (powered by differential solar heating and night cooling of sea...
23 KB (2,604 words) - 23:36, 17 April 2025
a phenomenon known as clear air turbulence (CAT), caused by vertical and horizontal wind shear connected to the wind gradient at the edge of the jet streams...
29 KB (3,346 words) - 15:56, 3 November 2024
zone of energetic charged particles, most of which originate from the solar wind, that are captured by and held around a planet by that planet's magnetosphere...
41 KB (4,779 words) - 00:30, 21 May 2025
display rapid fluctuations (turbulence) and vertical mixing is strong. Above the PBL is the "free atmosphere", where the wind is approximately geostrophic...
21 KB (2,077 words) - 14:06, 16 May 2025
wind or plasma fountain is a permanent outflow of plasma from the polar regions of Earth's magnetosphere.: 29 Conceptually similar to the solar wind...
13 KB (1,344 words) - 17:03, 24 May 2025
intermittent such as wind and solar, but at the expense of utilities and consumers. Subsidizing this with production tax credits makes wind power cheaper for...
134 KB (10,515 words) - 00:29, 24 May 2025
Interplanetary scintillation (section Solar wind)
I\rangle }}.} This can be related to the phase deviation caused by turbulence in the solar wind by considering the incident electromagnetic plane wave, and yields...
10 KB (1,261 words) - 04:08, 5 April 2025
Small wind turbines, also known as micro wind turbines or urban wind turbines, are wind turbines that generate electricity for small-scale use. These...
27 KB (2,910 words) - 14:01, 24 May 2025
Decay: Turbulence generated by buoyancy which drives the mixing decays after sunset and CBL collapses as well. In the atmospheric boundary layer, wind shear...
17 KB (2,573 words) - 11:22, 3 March 2024