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HomeLatest NewsThe Sun’s magnetic field flip: What to expect and when

The Sun’s magnetic field flip: What to expect and when



NEW DELHI: The Sun is approaching a critical phase known as a magnetic field polarity reversal, an event that occurs roughly every 11 years. This flip is a key component of the solar cycle, influencing space weather and the Earth’s magnetic environment.

The mechanism behind the flip

The Sun’s magnetic field reversal is driven by the movement of magnetic fields from active regions towards the poles, leading to a switch in polarity.“The magnetic field from active regions makes its way toward the poles and eventually causes the reversal,” solar physicist Todd Hoeksema, director of the Wilcox Solar Observatory at Stanford University, told Space.com.

The enigma of polarity reversal

Despite understanding the general process, the exact mechanisms underlying the flip remain elusive. “That gets into the whole [solar] cycle, and wondering what that is,” noted Phil Scherrer, also a solar physicist at Stanford University. “We still don’t have a really self-consistent mathematical description of what’s happening. And until you can model it, you don’t really understand it — it’s hard to really understand it.”
The complexity of the solar magnetic field and the varying contributions from sunspots add to the challenge of predicting and understanding the reversal. “Are there going to be many sunspots? And are the sunspots going to contribute to the magnetic field of the pole, or are they going to kind of cancel locally?” Hoeksema added. “That question we don’t yet know how to answer.”

What this means for Earth

As the Sun’s magnetic field flips, it affects the solar activity and space weather experienced on Earth. The increased activity can lead to more frequent and intense solar flares and coronal mass ejections (CMEs), which can cause geomagnetic storms, disrupt satellite communications, and enhance auroral displays.
Furthermore, the shifting magnetic field provides better protection against cosmic rays, shielding Earth from these high-energy particles more effectively. The “current sheet,” a large surface extending from the Sun’s equator, becomes wavier during this period, enhancing its ability to block cosmic rays.
Scientists continue to monitor the Sun closely to gather more data and improve their understanding of these magnetic flips. While the polarity reversal is a normal part of the Sun’s cycle, it offers a unique opportunity for researchers to study solar dynamics and improve space weather predictions.





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