Unveiling the Cosmic Genes: How does the sun play its part?

Amar RAJ
4 min readJan 18, 2024

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Embellished with its celestial wonders, the nighttime sky frequently treats us to an enthralling spectacle called the aurora borealis, or the Northern Lights. This ethereal dance of mild is a cosmic collaboration between the Sun and Earth, a symphony of solar winds, magnetic fields, and celestial wonders.

The Sun’s Cosmic Symphony

At the heart of our Milky Way galaxy, there is a celestial performer, which is the Sun, the big giant with which we are blessed to have a burst of continuous sunshine. The Sun isn’t just a hot ball; it’s a lively thing with spots, flares, and faculae. This big cosmic event with flares going on, as shown in Figure 1, is called solar activity and has far-reaching consequences, such as climate disruption on Earth. These storms will disrupt communications or make electrical systems go haywire. We’ve seen worse before, like in 1989 when a big storm knocked out power in Quebec for nine hours. Plus, these magnetic storms are the reason we get to see the aurora borealis.

Figure 1: Solar storm instigating Northern Lights on Earthlings.

The Sun does not need any introduction; however, I will still give a short scientific one. It’s made up of 92.1% hydrogen and 7.8% helium by the number of atoms, with an additional 0.1% metals. The surface temperature is a toasty 5800°C, but at the center, it soars to a staggering 15 million °C, accompanied by a mind-boggling pressure of 3 billion atmospheres. Imagine the Sun as a colossal cosmic engine, emitting a continuous stream of plasma into the amoeba of space which is known as solar wind. The zone of influence of this wind is called the heliosphere, and it extends to the confines of the solar system.

Now that we’ve explored the mesmerizing illusion of the sun, let’s delve into convection. The Sun’s heat stirs up its outer layers, a phenomenon called convection, involving movements in its liquid and gaseous layers due to temperature and density variations. Unlike Earth, the Sun’s rotation is uneven, with the equator spinning faster than the poles. This, combined with convection, gives rise to sunspots — areas with strong magnetic fields. Often appearing in pairs with opposite magnetic poles, these spots represent cooler regions amid the surrounding gases. Sunspots host powerful magnetic events on the Sun’s surface, although they don’t always trigger the aurora borealis. For the Northern Lights to grace us, a sunspot needs both an eruption and a subsequent coronal mass ejection.

But the real drama unfolds with the coronal mass ejections (CMEs). Born from solar flares and sunspots, these CMEs create a breathtaking display of magnetic arcs. When these arcs can no longer contain their energy, they burst forth, releasing a torrent of plasma into space. It is this coronal mass ejection that, when directed towards Earth, may set the stage for the enchanting aurora borealis.

Since scientists started observing and researching the Sun, a significant finding emerged in 1850: The Sun, with its ever-changing moods and rhythms, operates on a solar cycle that peaks every 11 years. This discovery has empowered astrophysicists to forecast the Sun’s activity intensity. Surprisingly, even during the least active phase of this cycle, we can witness the spectacular beauty of the aurora borealis on Earth. These awe-inspiring lights find their origin in the regularly appearing coronal holes which could be a source for these mystical and enchanting displays.

Let’s talk more about these holes, so in a nutshell, coronal holes, dark areas on the Sun’s surface, act as cosmic gateways. These are the areas where density is minimal, the solar plasma coming from these holes is not retained, and a continuous stream is ejected towards space in the form of high-speed solar wind. Basically, it is a door toward the interior of the sun.

Figure 2: Coronal mass ejections in process.

Solar Storms define majestic sympony, aurora

Solar flares, or storms, are pivotal events in the sun’s activity. They can disrupt radio transmissions on Earth and set the stage for the appearance of polar auroras. Picture them as dynamic events, marked by coronal mass ejections and open coronal holes. These solar storms add a touch of drama to our cosmic narrative, affecting the delicate balance between the sun and Earth. The Dance Continues!!! As we delve deeper into the secrets of our cosmic neighbors, the aurora borealis stands as a testament to the dynamic interplay between the sun and Earth. In the vast theater of the cosmos, these lights transform scientific phenomena into a celestial spectacle for all to enjoy — a cosmic dance that continues to captivate and inspire. So, the next time you find yourself under the night sky, look up, and witness the celestial ballet of the northern lights, a dance choreographed by the forces of the sun and Earth.

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Let’s keep exploring and delve deeper into the world of the Aurora. Join us on the next part of this fascinating journey.

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