Prominences hanging off the limb of the Sun are the same as filaments seen in front of thedisk.
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Q15: The Sun's magnetic field has been traced
Q16: Using the observations of the Solar and
Q17: The solar corona produces a lot more
Q18: The solar corona is much cooler than
Q19: As with Uranus, the solar equator rotates
Q21: The density of the Sun is most
Q22: The proton-proton chain requires a temperature of
Q23: Both the gravitational and electromagnetic forces obey
Q24: The light we see from the Sun
Q25: The solar constant measures the energy received
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