The Solar Wind
The solar wind varies in density, temperature and speed over time and over solar latitude and longitude. Its particles can escape the Sun's gravity because of ...
Solar wind: What is it and how does it affect Earth? - Space.com
When the solar wind reaches Earth it sends a flurry of charged particles into the magnetosphere and along Earth's magnetic field lines, towards ...
Solar Wind | NOAA / NWS Space Weather Prediction Center
Different regions on the Sun produce solar wind of different speeds and densities. Coronal holes produce solar wind of high speed, ranging from 500 to 800 ...
Solar Wind - Space Technology 5 - NASA
As the Sun rotates (once every 27 days), it winds up its magnetic field lines above its polar regions into a large rotating spiral, creating a constant stream ...
The solar wind, explained - UChicago News
The corona is so hot that the sun's gravity can't hold it, so particles are flung off into space and travel throughout the solar system in every direction. As ...
Solar Wind - UCAR Center for Science Education
The solar wind is continuously flowing from the Sun. It is made up of ionized plasma and particles that escape from the Sun's corona. In this outer atmosphere, ...
ESA - The solar wind - European Space Agency
The space between the planets of the Solar System is not actually empty, but filled with a driving rain of particles constantly streaming outwards from the ...
Solar Wind on the Moon - NASA Science
The Moon is not a magnet, so it has no global magnetic field, although some areas on the Moon have localized magnetic fields. With no magnetosphere, and almost ...
Solar Wind - an overview | ScienceDirect Topics
Solar Rotation and the Magnetic Field in the Solar Wind. Solar wind is an ionized gas made up primarily of protons and electrons with minor ions in amounts ...
Solar Wind, Geomagnetic Storms, and Coronal Mass Ejections
Coronal Mass Ejections (CMEs) are large clouds of plasma and magnetic fields hurled into space from the Sun. The ejected material can travel a million or more ...
Solar wind | Interplanetary Medium, Heliosphere, Plasma | Britannica
Solar wind, flux of particles, chiefly protons and electrons together with nuclei of heavier elements in smaller numbers, ...
What is Solar Wind? | Definition & Causes - Study.com
The solar wind refers to the steady stream of highly charged particles that continually blow off the Sun in all directions. It is caused by the solar corona ...
NASA ScienceCasts: Effects of the Solar Wind - YouTube
The continuously expanding solar wind begins in our Sun and doesn't stop until after it reaches the edge of the heliosphere.
The origin of the solar wind is the thermal expansion of the solar corona against the gravitational attraction of the Sun, but at the present time it is not ...
The solar wind from a stellar perspective - How do low-resolution ...
In this paper, we explore the effects of the input Alfvén wave energy flux and the surface magnetogram on the wind properties predicted by the Alfvén Wave ...
2 solar probes are helping researchers understand what ...
For years, researchers have wondered what energy source allows the solar wind − a projection of charged particles from the Sun − to rush by ...
The Origin of the Solar Wind | American Scientist
The solar wind is merely the extension of the Sun's atmosphere, the solar corona, which is visible to us during a total solar eclipse.
The asymptotic velocity u∞ of the wind is comparable to the escape velocity vesc. Winds from solar-type stars are thought to be driven by gas pressure gradients ...
The solar wind is a stream of energized, charged particles, primarily electrons and protons, flowing outward from the Sun, through the solar system at speeds as ...
The solar wind | Help | SpaceWeatherLive.com
The solar wind is a stream of charged particles (a plasma) released from the Sun. This stream constantly varies in speed, density and temperature.