Pressure distribution in the sun

AI Thread Summary
The discussion centers on the pressure distribution within the sun, specifically from the core to the convection zone. The core pressure is noted to be approximately 25 PPa, but there is a request for comparable pressure values in the radiative and convection zones. Several resources are provided to help understand the internal structure of the sun. Additionally, it is suggested that approximations can be made using the ideal gas law, P = nkT, based on temperature and particle density. The conversation emphasizes the importance of these calculations for studying solar dynamics.
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Hi,

I am currently studying the internal structure of the sun and I was wondering if there exists scientific information regarding the pressure distribution along a hypothetical line from the core to the, let´s say, convection zone. You can find frequently in the internet that the pressure in the core is about 25 PPa. Are there comparable values for the radiative zone and the convection zone?

Greetings,

Andreas
 
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Thanks a lot, that gave me a good insight. I will study your links step by step.
 
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