How do the magnetic field lines sustain themselves as the coronal mass ejection flies away from the Sun?
The Earth's magnetic field is constant however the lines of magnetism are swept back by CMEs(Coronal Mass Ejection).
The figure above illustrates the Earth's magnetic field during a CME.
The figure above shows the magnetic field normally.
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The magnetic field lines are anchored in the surface of the Sun and are carried along by the plasma ejected from the Sun as the coronal mass ejection (CME) moves away from the Sun, maintaining the structure of the magnetic field lines as they propagate through space.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
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