The solar wind is commonly said to mean that the sun blows wind into the cosmic space, how is it for

Updated on science 2024-04-19
21 answers
  1. Anonymous users2024-02-08

    We divide the solar atmosphere into six layers, which are named in order from the inside to the outside: the solar core, the radiation zone, and the convection. This is where the solar wind is formed and emitted.

  2. Anonymous users2024-02-07

    The solar wind is controlled by the solar kinetic electric field in its radiation to form the solar ecliptic around the sun itself, which is the fundamental reason for the constraining and generation of the children of the solar system and its star belts!

  3. Anonymous users2024-02-06

    The troposphere inside the atmosphere forms the solar wind.

  4. Anonymous users2024-02-05

    Convection occurs in the Sun's atmosphere, forming winds.

  5. Anonymous users2024-02-04

    Formed in the atmosphere of the Sun, a normal phenomenon.

  6. Anonymous users2024-02-03

    There are so many places to study and learn.

  7. Anonymous users2024-02-02

    That's not quite reasonable.

  8. Anonymous users2024-02-01

    The sun and the wind are the first time I've heard of it.

  9. Anonymous users2024-01-31

    So how did the sun form, turning the air and bringing it up.

  10. Anonymous users2024-01-30

    I really don't know how it came to be.

  11. Anonymous users2024-01-29

    What is the solar wind? LetAstronomical phenomenaTell you about it! The solar wind is a stream of charged particles from supersonic plasma ejected from the Sun's upper atmosphere.

    In the absence of the Sun, this stream of charged particles is also often referred to as the "stellar wind", which is a continuous stream of high-velocity charged particles that comes from the Sun and moves at a speed of 200-800 km/s.

    Chinese name: solar wind.

    Foreign name: solar wind

    Attributes: Eruption of a stream of energetic particles in the solar coronal layer.

    Features: High-speed flow of charged particles, producing auroras.

    Subjects: Physics, Astronomy, Sun.

    The solar wind is a stream of charged particles from supersonic plasma ejected from the Sun's upper atmosphere. In the absence of the Sun, this stream of charged particles is also often referred to as a "stellar wind." The solar wind is a continuous stream of charged particles from the sun and moving at a speed of 200-800 kms.

    Although this substance is different from the air on the earth in that it is not composed of gas molecules, but is composed of simpler elementary particles that are one level smaller than atoms, such as protons and electrons, the effect of their flow is very similar to that of air flow, so it is called the solar wind. In March 2012, the strongest solar storm in five years erupted on the morning of the 7th, affecting wireless communications.

    The density of the solar wind is very thin and insignificant compared to the density of the wind on Earth. In general, in interplanetary space near the Earth, there are a few to dozens of particles per cubic centimeter, while the density of the wind on Earth is 268.7 billion molecules per cubic centimeter. However, although the solar wind is very thin, it blows far more violently than the wind on earth.

    On Earth, the wind speed of a Category 12 typhoon is more than one meter per second, while the wind speed of the solar wind is often maintained at 350,450 kilometers per second near the earth, which is tens of thousands of times the wind speed of the earth, and can reach more than 800 kilometers per second at the most violent time.

    Brief introduction. The solar wind is a near-strong spillover of charged particles. They are released into interplanetary space from the Sun's corona.

    These particles, mainly protons and electrons, move near the Earth's orbit at a speed of 200-900 kilometers per second. Although it has a low density (about 8 cm3), it can also interact with the Earth's magnetosphere.

  12. Anonymous users2024-01-28

    The solar wind is a clear bond particle from the surface of the sun, specifically from ().

    a.Sunspot.

    b.Solar prominence. c.Taimu is in the sun nuclear fusion.

    d.Corona. Correct answer: d

  13. Anonymous users2024-01-27

    Effects of the solar wind on humans:

    1.When the solar wind passes over the Earth, it will cause changes in the electromagnetic field, causing geomagnetic storms, ionospheric storms, and affecting communications, especially shortwave communications.

    2.It sends a strong original charge to the power grid, pipelines and other large structures on the ground, affecting the safety of the power transmission, oil transmission and gas pipeline systems.

    3.There will also be an impact on the satellites that are operating.

    4.The amount of radiation from a single solar wind can easily reach the amount of multiple x-rays for a person. It can also cause a decrease in the body's immunity, which can easily cause lesions, and will also make people prone to mood swings and even an increase in car accidents.

    5.It will increase the temperature.

    6.Auroras are formed at the north and south poles.

  14. Anonymous users2024-01-26

    Solar wind refers to a stream of charged particles from supersonic plasma ejected from the upper atmosphere of the Sun. In the case of not the sun, this kind of bichivalry.

    Streams of charged particle particles are also often referred to as "sidereal winds". The solar wind is a continuous existence, coming from the sun and ending at 200-

    A stream of high-speed charged particles moving at a speed of 800 km s.

    This substance, although different from the air on Earth, is not composed of molecules of gas, but is made up of simpler molecules, and one size smaller than an atom.

    The basic particles of the skin leak - protons and electrons, but the effect they produce when they flow is very similar to that of air flow, so.

    It is called the solar wind.

    In the solar system, the composition of the solar wind and the composition of the sun's corona are exactly the same. Of these, hydrogen occupies 73 and helium occupies 73.

    25, and there are also a small amount of impurities. Usually the bursts of energy of the solar wind come from solar flares or other known as the "solar wind."

    storm" of the climatic phenomenon. This solar activity can be detected by space detectors and satellites, and the main sign detected is radiation.

    In the interstellar medium, the solar wind from the hand source can be seen as if blowing a large "bubble".

  15. Anonymous users2024-01-25

    It's a storm of particles blown by the sun. It will not blow the Earth away, and the violent solar wind will only affect the Earth's magnetic field.

  16. Anonymous users2024-01-24

    The solar wind is the stream of electric particles from the sun's atmosphere that ejects a supersonic plasma belt. The violent solar wind can't blow the earth away, otherwise it would have been blown away a long time ago, how can we wait until now?

  17. Anonymous users2024-01-23

    The solar wind often occurs in the "coronal layer" of the sun, the coronal layer is the outermost layer of the sun, the temperature is higher, and the "solar wind" formed by it is a supersonic charged particle stream emitted by the sun, the density of the solar wind is not large, it is generally very thin, but its intensity is amazing, although the solar wind can not blow the earth away, but it will affect the earth's wireless communication, and form auroras at the north and south poles.

  18. Anonymous users2024-01-22

    The coronal hole is an open area of the sun's magnetic field, where the magnetic field lines spread out into space, and a large amount of plasma runs out along the magnetic field lines, forming a stream of particles moving at high speed. The particle stream travels at about 16 km per second at the bottom of the coronal hole and can reach speeds of more than 300 400 km per second when it reaches the vicinity of the Earth's orbit. This high-speed flow of ions is the solar wind.

  19. Anonymous users2024-01-21

    The Sun's outer atmosphere, the solar corona, is constantly expanding outwards to form a stream of plasma radially outward from the Sun, commonly referred to as it.

    solar wind". The solar wind causes comets to form long tails that run in the direction of the opposite Sun. When one admires the beautiful comet tail can imagine too.

    The presence of the yang wind. The colorful aurora phenomenon seen in the high latitudes of the Earth is also the acceleration of solar wind particles entering the Earth's magnetic field in the Earth's atmosphere.

    Produced by sedimentation. Direct observations from spacecraft indicate that the solar wind is composed mainly of protons and electrons, but with a small amount of helium nuclei and trace heavy ions.

    It is assumed that beyond about 100 astronomical units (astronomical units = average distance between the sun and the earth = kilometers), the solar wind will be similar to the Milky Way.

    The interstellar gas junction of the system, the extent of space occupied by the solar wind is called the "heliosphere". The study of the physical processes of the solar wind and its laws has become empty.

    A new branch of physics - heliospheric physics.

  20. Anonymous users2024-01-20

    The sun is a stream of ionized gas continuously released towards the solar system at very high speed and with erratic intensity. When this gas stream passes near the Earth, it will interact with the Earth's magnetic field and produce various effects in the upper atmosphere.

    The solar wind is a stream of charged particles from supersonic plasma ejected from the upper atmosphere of a star.

  21. Anonymous users2024-01-19

    The solar wind is a large-scale stream of charged particles released by the corona in the Sun's atmosphere. When it reaches the earth, it is adsorbed by the earth's magnetic field, and the charged particles adsorbed at the north and south magnetic poles rub against the atmosphere at the north and south poles to produce auroras. In other areas, the atmospheric ionosphere can be further excited, and the atmospheric ionosphere at high altitude can be thickened, adsorbing or changing the original radio shortwave, resulting in the interruption of radio shortwave communication.

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Generally speaking, it will take a long time to meet again, because if you meet it at this time, it means that your luck is very good, so you can wait until a while to meet the next solar wind, so this is also very simple, everyone wait patiently.

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5-10 years. I can't help it, I'm looking into this.