CMEs, or Coronal Mass Ejections
Bright explosions of hot gases from the chromosphere are known as solar flares. They release huge amounts of energy in the form of electromagnetic radiation, x-rays, and charged particles that can impact Earth's magnetic field and cause disruptions in communication systems and power grids.
The Sun's atmosphere is called the chromosphere and the corona. The photosphere which is below the chromosphere and is the visible surface of the Sun is usually considered to be part of the atmosphere also.
Cooler gases in the sun include elements like helium, oxygen, carbon, and iron. These gases typically exist in the outer layers of the sun's atmosphere, such as the chromosphere and the corona, where temperatures are lower compared to the sun's core.
Yes, explosions can occur in space, but they differ from explosions on Earth due to the absence of atmosphere. In space, explosions can happen in a vacuum and are often driven by chemical reactions, nuclear reactions, or the rapid expansion of gases. For instance, supernovae are massive stellar explosions that occur when a star exhausts its nuclear fuel. However, the lack of air means there is no sound to accompany these explosions, and the energy is released in different forms, like radiation.
Stars are not plants they are really hot gases.
Bright explosions of hot gases from the chromosphere are known as solar flares. They release huge amounts of energy in the form of electromagnetic radiation, x-rays, and charged particles that can impact Earth's magnetic field and cause disruptions in communication systems and power grids.
The answer is chromosphere
In the chromosphere, gases move due to convection, which involves the rising of hot gases and sinking of cooler gases. These movements are driven by the transfer of energy from the Sun's interior. Additionally, magnetic fields in the chromosphere can also influence the movement of gases, leading to phenomena such as solar flares and prominences.
The outer edge of the Sun's fiery gases is called the chromosphere. It lies above the photosphere and below the corona, and it is characterized by its reddish color, which becomes visible during solar eclipses. The chromosphere is where solar phenomena like spicules and solar flares occur.
the gases of the sun extend far beyond the photosphere, which may be considered the lowest level of the solar atmosphere. The region immediatly above the photosphere is called the chromosphere.
the chromosphere glows because of the release of hot, low density gases that are emitted from the sun. Normally, it can't be seen by the naked eye due to light from the photosphere blocking it. During a solar eclipse, the chromosphere is visible, appearing as a red ring around the Sun.
Mott Souders has written: 'Gaseous explosions' -- subject(s): Explosions, Gases, Tetraethyllead
the chromosphere glows because of the release of hot, low density gases that are emitted from the sun. Normally, it can't be seen by the naked eye due to light from the photosphere blocking it. During a solar eclipse, the chromosphere is visible, appearing as a red ring around the Sun.
L. J. E Hofer has written: 'The evaluation of gases from mine explosions by elemental balancing' -- subject(s): Mine gases, Mine explosions, Analysis
To avoid overheating and explosions.
Pyroclastic flows.
The Sun's atmosphere is called the chromosphere and the corona. The photosphere which is below the chromosphere and is the visible surface of the Sun is usually considered to be part of the atmosphere also.