Using the observations of the Solar and Heliospheric Observatory (SOHO)and SolarDynamics Observatory (SDO), it may be possible to predict mass ejections from the Sun days inadvance.
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Q11: Scientists suspect changes in the flow of
Q12: Solar activity cannot disrupt communications on Earth.
Q13: The Sun's mass and volume are over
Q14: At very large distances from the Sun,
Q15: The Sun's magnetic field has been traced
Q17: The solar corona produces a lot more
Q18: The solar corona is much cooler than
Q19: As with Uranus, the solar equator rotates
Q20: Prominences hanging off the limb of the
Q21: The density of the Sun is most
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