The Sun's structure is uniform throughout its interior, with no evidence of different layers.
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Q1: Granulation is the most obvious proof of
Q9: The photosphere is the coolest layer close
Q10: The Sun's radius is one astronomical unit
Q11: The prolonged period of few sunspots between
Q12: Observations of sunspots at different solar latitudes
Q13: The Sun's average density is about the
Q16: The chromosphere is faint because of its
Q18: The solar corona is much cooler than
Q18: A typical solar flare lasts only a
Q19: The proton storms in the solar wind
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