Compressed magnetic fields tend to push themselves apart. Yet sunspots can be stable for as long as 2 months. How do we explain this?
A) Sunspots are stabilized by the circulation of charged gases around the field below the surface of the photosphere.
B) Sunspots tend to occur in pairs of opposite polarity. The repulsive forces tend to keep each group compressed.
C) The energy that is needed to push the field lines apart is instead expended in sending spicules into the chromosphere.
D) The sunspot pairs (preceding and following members) cancel out, relaxing the magnetic fields and their tendency to repel.
Correct Answer:
Verified
Q56: Sunspots have been observed:
A)since at least 2000
Q57: If sunspots are cooler than the photosphere
Q58: If the temperature near the center of
Q59: Due to differential rotation, sunspot groups near
Q60: What is the character of the sunspot
Q62: If the magnetic polarity of the north
Q63: At the maximum of the sunspot cycle
Q64: Most solar variations associated with the so-called
Q65: The 11-year sunspot cycle on the Sun
Q66: What is a plage?
A)a bright area on
Unlock this Answer For Free Now!
View this answer and more for free by performing one of the following actions
Scan the QR code to install the App and get 2 free unlocks
Unlock quizzes for free by uploading documents