Coronal ejections or solar flares or prominences
The huge fiery arms or loops extending from the sun's surface are called solar prominences. These are large, bright features that extend outward from the sun's surface, often in a loop shape, due to the sun's magnetic field. Solar prominences are composed of hot plasma and can last for several days or even weeks. They are often associated with solar activity, such as sunspots and solar flares.
gasses
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.
They are solar flares.
the SUN
The hot gases moving away from the sun's corona are known as the solar wind. These gases consist of charged particles, mainly electrons and protons, that are ejected from the sun's atmosphere at high speeds. The solar wind interacts with the Earth's magnetic field and can cause phenomena like auroras.
Yes, loops of gas on the Sun, known as coronal loops, are structures that connect different sunspot regions. These loops are formed by the Sun's magnetic fields, which can trap hot plasma and create beautiful, arching formations in the solar atmosphere. They are often observed in ultraviolet and X-ray wavelengths and play a significant role in solar activity, including solar flares and coronal mass ejections.
Those loop-like shapes of hot gas on the sun are called solar prominences or solar loops. They are formed by the Sun's magnetic field trapping and shaping the plasma.
The hot gases that extend from the Sun's corona are primarily composed of plasma, consisting of ionized hydrogen and helium, along with trace amounts of heavier elements. These gases are expelled into space during solar events, such as coronal mass ejections and solar flares, forming the solar wind. The solar wind travels through the solar system, influencing planetary atmospheres and magnetic fields. The temperature of the corona can reach millions of degrees Celsius, causing these gases to flow outward at high speeds.
These loops are called penumbral fibrils. They are structures of hot gas in the sun's photosphere that connect different parts of sunspots, contributing to the magnetic activity and energy transfer within those regions.
rominences A) Streams of glowing gas that shoot out from the sun in an arch Solar flares B) Brief eruptions of intense high-energy radiation from the sun's surface Sunspots C) Dark spots appearing from time to time on the sun's surface Convection D) The rise of hotter, less dense fluid and the sinking of cooler, denser fluid can you match them up? i need help
Its super huge, super hot, and it is considered to be in the center of the planets orbits.