solar wind
A stream of charged particles produced by the sun's corona is called the solar wind. This continuous flow of charged particles, mostly electrons and protons, emanates from the sun and extends throughout the solar system, affecting the planets and interstellar space.
A fast-moving stream of particles released into space is called a solar wind. It is composed of charged particles, such as protons and electrons, that are expelled from the Sun and can interact with planetary magnetospheres.
Solar wind is created by the Sun's outer atmosphere, called the corona, which is made up of highly energized particles. These particles are ejected into space at high speeds, carrying magnetic fields with them. This constant stream of charged particles flowing away from the Sun is what we call solar wind.
A stream of particles produced by the corona is known as the solar wind. It consists of charged particles, such as electrons and protons, that are continuously emitted from the Sun's outer atmosphere. These particles can interact with the Earth's magnetic field and cause phenomena like auroras.
Solar wind.
A stream of electrically charged particles sent out by the corona is called solar wind. These particles are continually emitted from the Sun and travel through the solar system at high speeds, influencing the space environment and potentially interacting with planetary atmospheres.
Solar wind.
solar wind
The general dissipation of charged particles from the sun is called the Solar Wind. Occasionally the sun also emits vast quantities of matter from bursts known as "Coronal Mass Ejections". (The Corona is the Sun's atmosphere.)
A stream of charged particles is called an electrical current.
It is called the corona of the sun.
The stream of charged particles that escape through holes in the sun's corona is called the solar wind. This continuous flow of particles, primarily electrons and protons, travels through the solar system at high speeds, affecting planetary atmospheres and magnetic fields.
A stream of charged particles produced by the sun's corona is called the solar wind. This continuous flow of charged particles, mostly electrons and protons, emanates from the sun and extends throughout the solar system, affecting the planets and interstellar space.
Coronal Mass Ejection. or sun flare.
SOLAR WIND
Thomson knew that the glow in the cathode ray tube (CRT) was from a stream of charged particles because the particles were deflected by electric and magnetic fields, indicating they were negatively charged. By measuring the deflection of the particles, he was able to calculate the charge-to-mass ratio of the particles, leading to the discovery of the electron.