| Corrections are only applied to data poleward of the convection zone boundary. |
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| The convection zone is bounded by the HMB which extends to 61° MLAT on the nightside. |
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| As the wave front comes in contact with the tropical convection zone, it scatters and a secondary wave is generated. |
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| During this period the Swarm A satellite makes a complete pass through the northern hemisphere high-latitude convection zone. |
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| Helioseismology studies have built up a certain picture of the solar interior, including such details as the depth of the convection zone. |
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| It is believed that the movement of mass within the convection zone creates the magnetic activity that generates sunspots. |
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| The regions just below the photosphere are known as the convection zone and the radiation zone, which allow heat and energy to travel up from the core to the surface. |
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| Helioseismology provides unique information about the global dynamics of the Sun and local flows in active regions in the upper convection zone. |
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| The energy flow coming from the core passes gradually through the Sun's less dense layers before reaching a region called the convection zone, where the flow becomes turbulent. |
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| Above that is the convection zone where the gas material transports energy primarily through physical displacement of the gas known as convection. |
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