Customize Consent Preferences

We use cookies to help you navigate efficiently and perform certain functions. You will find detailed information about all cookies under each consent category below.

The cookies that are categorized as "Necessary" are stored on your browser as they are essential for enabling the basic functionalities of the site. ... 

Always Active

Necessary cookies are required to enable the basic features of this site, such as providing secure log-in or adjusting your consent preferences. These cookies do not store any personally identifiable data.

No cookies to display.

Functional cookies help perform certain functionalities like sharing the content of the website on social media platforms, collecting feedback, and other third-party features.

No cookies to display.

Analytical cookies are used to understand how visitors interact with the website. These cookies help provide information on metrics such as the number of visitors, bounce rate, traffic source, etc.

No cookies to display.

Performance cookies are used to understand and analyze the key performance indexes of the website which helps in delivering a better user experience for the visitors.

No cookies to display.

Advertisement cookies are used to provide visitors with customized advertisements based on the pages you visited previously and to analyze the effectiveness of the ad campaigns.

No cookies to display.

Tech/Science

Understanding the Sun’s 11-Year Magnetic Pole Flip Cycle

Every 11 years, the Sun undergoes a magnetic pole flip, leading to increased solar activity such as sunspots, solar flares, and mesmerizing northern and southern lights. The current solar cycle, known as ‘solar cycle 25,’ began in 2019 and is expected to peak around 2024 or 2025 before returning to lower activity levels in the early 2030s.

The 11-year solar cycle was first definitively identified in 1843 by German amateur astronomer Heinrich Schwabe through the observation of sunspots on the Sun’s surface. This cycle has been relatively consistent for millions of years, with evidence suggesting that other stars also exhibit similar but varying cycle durations.

When the Sun’s magnetic field flips, it triggers various phenomena like sunspots. The Sun’s magnetic field is a complex process driven by the charged particles in the Sun’s ionized hydrogen gas, creating a magnetic field with changing polarity. While the exact mechanisms are not fully understood, this magnetic field plays a crucial role in solar activity.

LEAVE A RESPONSE

Your email address will not be published. Required fields are marked *