Due to the magnetic effects, the occurrence rate of the instability is not symmetric in longitudes even at the magnetic equator.

由于地磁位型的不同，发生率的分布并不具有经度对称性，即使在磁赤道附近也如此。

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When the magnetic field is at its strongest, and sunspots at their most plentiful, they cluster close to the equator.

当磁场最强，太阳黑子最丰富的时候，它们会聚集在赤道附近。

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While aurora are generally only visible close to the poles, severe magnetic storms impacting the Earth’s magnetic field can shift them towards the equator.

虽然极光一般仅在两极附近可见，不过在强烈的磁暴对地球磁场的影响下，极光也会在赤道附近出现。

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