Use that the pressure on the Sunspot (ideal gas) plus the magnetic pressure B?/(2µo) equals the photosphere pressure (also ideal gas but at different pressure) in order for the Sunspot not to sink. Use that p=3.5x10ª kg/m³ and µ=1 to find the magnetic field strength in the Sunspot.

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Use the concept that the pressure on the Sunspot (ideal gas) plus the magnetic pressure \( B^2/(2\mu_0) \) equals the photosphere pressure (also ideal gas but at a different pressure) to ensure the Sunspot does not sink. Given \( \rho = 3.5 \times 10^{-4} \, \text{kg/m}^3 \) and \( \mu = 1 \), calculate the magnetic field strength in the Sunspot.
Transcribed Image Text:Use the concept that the pressure on the Sunspot (ideal gas) plus the magnetic pressure \( B^2/(2\mu_0) \) equals the photosphere pressure (also ideal gas but at a different pressure) to ensure the Sunspot does not sink. Given \( \rho = 3.5 \times 10^{-4} \, \text{kg/m}^3 \) and \( \mu = 1 \), calculate the magnetic field strength in the Sunspot.
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