convection
We can't see material below the photosphere because it is opaque to visible light. The high density and temperature of the material, combined with the scattering and absorption of light within it, prevent light from passing through it easily. This makes it impossible for us to directly observe what lies beneath the photosphere with visible light.
The photosphere is the visible surface of the Sun and is located above the convection zone and below the chromosphere. It sits at an approximate temperature of 5,500 degrees Celsius (about 9,932 degrees Fahrenheit) and is the layer from which sunlight is emitted. Above the photosphere, the chromosphere and then the corona extend outward into space.
The Cromoshpere Is Found Just Above The Photosphere. For A Few Moments You Can See The Chromoshpere During A Solar Eclipse Or When Using a Special Instrument.
No, sunspots are "holes" in the sun's photosphere that allow you to see the layer just below. They are produced by concentrations of solar magnetic flux lines.
The photosphere is the layer in the sun's atmosphere that is dense enough to emit plenty of light but not so dense that the light can't escape. Below the photosphere, the gas is denser and hotter therefore radiates plenty of light, but that light cannot escape from the sun because it is blocked by the outer layers of gas. so you cannot detect light from these deeper layers.Sources: Book The Solar System by Seeds/Backman (7th Edition) P.143
The energy transport just below the sun's photosphere is mainly by convection. Convection is the process where hot material rises, cools down, and then sinks back down to be reheated, creating a cycle of energy transfer. This convection zone helps move heat from the sun's core to its surface.
The photosphere is the outer part of the star that is visible, inside which the star becomes opaque to visible light. The photosphere is the layer below the star's atmosphere (the chromosphere, and so forth).
We can't see material below the photosphere because it is opaque to visible light. The high density and temperature of the material, combined with the scattering and absorption of light within it, prevent light from passing through it easily. This makes it impossible for us to directly observe what lies beneath the photosphere with visible light.
The radiative zone extends from about 25% to 70% of the distance from the Sun's core to its surface, which corresponds to roughly 70-200 thousand kilometers below the photosphere.
The photosphere is the visible surface of the Sun and is located above the convection zone and below the chromosphere. It sits at an approximate temperature of 5,500 degrees Celsius (about 9,932 degrees Fahrenheit) and is the layer from which sunlight is emitted. Above the photosphere, the chromosphere and then the corona extend outward into space.
Ask at the Atomic Energy of Canada Limited for details; see the link below.
Energy carriers are molecules that can temporarily store or transport energy within cells. They typically have high-energy bonds that can release energy when broken. Additionally, energy carriers have the ability to transfer energy to other molecules in metabolic processes.
The Cromoshpere Is Found Just Above The Photosphere. For A Few Moments You Can See The Chromoshpere During A Solar Eclipse Or When Using a Special Instrument.
I'm unable to see the illustration you mentioned, but if you describe it, I can help explain the process occurring in it.
No, sunspots are "holes" in the sun's photosphere that allow you to see the layer just below. They are produced by concentrations of solar magnetic flux lines.
The photosphere is the layer in the sun's atmosphere that is dense enough to emit plenty of light but not so dense that the light can't escape. Below the photosphere, the gas is denser and hotter therefore radiates plenty of light, but that light cannot escape from the sun because it is blocked by the outer layers of gas. so you cannot detect light from these deeper layers.Sources: Book The Solar System by Seeds/Backman (7th Edition) P.143
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.