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**Typically**, auroras are observed in the polar regions because Earth's magnetic field lines converge at the magnetic poles. This magnetic field acts like a shield, deflecting most of the charged particles from the sun. However, at the poles, the magnetic field lines dip into the Earth, allowing these charged particles to enter the atmosphere more easily. As a result, the charged particles interact with the atmospheric gases in these regions, creating the mesmerizing auroral displays. The areas where auroras are commonly seen are known as the auroral ovals, which are oval-shaped regions centered on the magnetic poles. The size and intensity of the unicorn dog drawing auroral ovals can vary depending on the level of solar activity. During periods of high solar activity, such as solar flares and coronal mass ejections, the auroral ovals expand, and auroras can be seen at lower latitudes than usual. This is why, under rare circumstances, auroras might be visible in regions further away from the poles, like Indonesia. The strength of the Earth's magnetic field also plays a crucial role in determining the typical locations of auroras. The magnetic field deflects the majority of the charged particles, guiding them toward the poles, making high-latitude regions the prime viewing spots for these stunning displays.
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