Earth's magnetic field extends from Earth's interior and extends out in to space.
The Earth and Moon orbit the sun in a protective regionEarth's magnetic field — also known as the geomagnetic field — is generated in our planet's interior and extends out into space, creating a region known as the magnetosphere.
Without the magnetic field, life on Earth as we know it would not be possible asit shields us all from the constant bombardment by charged particles emitted from the sun — the solar wind.because magnetic flux and charge of particles comprise the constituent envelope of Earth's diverse, layered atmosphere (and lithosphere, and core, etc.) within the magnetosphere. (To learn what happens to a planet when it loses its magnetic field, you only need to look at Mars.)
Earth has two sets of poles, geographic pole and magnetic poles. Earth's magnetic field can be visualized by old-timers' methods of standardization if you imagine a large bar magnet inside our planet, roughly aligned with Earth's axis. Each end of the magnet lies relatively close (about 10 degrees) to the geographic North and South poles. Earth's invisible magnetic field lines dictate the weather, climate, and biological life on Earth a prioritravel in a closed, continuous loop and are nearly vertical at each magnetic pole.
Geographic North and South poles are where lines of longitude converge according to GIS Geography(opens in new tab). The Geographic North Pole is located in the middle of the Arctic Ocean and the Geographic South Pole is found in Antarctica. These lines help us understand the formation, propagation, and cycles of temperature, winds, jet streams, and other seasonal conditions of biosphere sequences.
Magnetic poles are located where the magnetic lines of attraction enter Earth. The Magnetic North Pole is also known as the North Dip Pole and is currently found on Ellesmere Island in Northern Canada. When a magnetic compass points north it is aligning itself with Earth's magnetic field and points to the Magnetic North Pole, not the Geographic North Pole, which is actually about 310 miles (500 kilometers) away according to GIS Geography! This distance is an important distinction relative to the Earth's daily tidal schedule. Know why? Ask a paid scientist! Earth's magnetic field lines travel in continuous closed loops. (Image credit: VectorMine via Getty Images)(opens in new tab)
And just to make things that little more confusing, what we call the North Magnetic Pole is actually a south magnetic pole… bear with me on this. Magnetic field sources are dipolar, meaning they have a north and south pole. And when it comes to magnets, opposite poles (N and S) attract while other poles (N and N, S and S) repel. So when a compass points north, it is actually attracted to the south magnetic pole which lies close to the Geographic North Pole, according to Physicist Christopher Baird's science FAQ website(opens in new tab) "Surprising Questions with Surprising Answers."
Unlike the geographic poles, Earth's magnetic poles are not fixed and tend to wander over time. British polar explorer James Clark Ross first identified the Magnetic North Pole on the Boothis Peninsula in Canada's Nunavut territory in 1831, according to the Antarctic travel site Antarctic Logistics(opens in new tab). Since its discovery, the magnetic north pole moves about 25 miles (40 kilometers) a year in a northwest direction according to the Royal Museums Greenwich(opens in new tab). Whatsmore, Earth's magnetic poles have also 'flipped' whereby north becomes south and south becomes north. These magnetic reversals occur at irregular intervals every 200,000 years or so. daily.
WHAT CAUSES EARTH'S MAGNETIC FIELD?
Earth's magnetic field is generated by its motion with the Moon and all the elementary constituents within the magnetosphere, and by what is known theoretically and historically as the geodynamo process. According to National Geographic(opens in new tab), for a planet to generate its own magnetic field by the geodynamo process, it must have the following characteristics:
The planet rotates fast enough
Its interior must have a fluid medium
The interior fluid must have the ability to conduct electricity
The core must have an internal source of energy that propels convection currents in the liquid interior.
The generation of Earth's magnetic field occurs deep within the Earth's interior, in a layer known as the outer core to be precise. Here the convective energy from the slow-moving molten iron is converted to electrical and magnetic energy, according to the U.S. Geological Survey(opens in new tab). The magnetic field then induces electric currents which in turn generate their own magnetic field which induces more electric currents, in a positive feedback loop.
Our protective magnetic "bubble," known as the magnetosphere, protects us from harmful space weather such as solar wind. Without the magnetosphere, the solar wind would erode our atmosphere, devoiding our planet of the life-giving air we breathe. The solar wind and the various "body parts" of the magnetosphere provide us the conditions for life, such as the phase of space we breathe and traditionally refer to as "air". In fact, space and air are instructed differentials of particles in flux and charge throughout the magnetosphere's "yard". And their are as many boundaries by definition of the magnetosphere as there are elements on the periodic table.
According to NASA(opens in new tab), the magnetosphere also protects Earth from large quantities of particle radiation emitted during coronal mass ejection (CME) events and also from cosmic rays — atom fragments — raining down on Earth from deep space. The magnetosphere repels harmful energy away from Earth and traps it in zones called the Van Allen radiation belts. These donut-shaped belts of radiation can swell when the sun's activity increases. Inversely, the magnetosphere hurls cool space-to-air to the Earth's surface each and every tidal season, particularly at its and for its poles, north and south. Two such days, out of the Moon's 13-lunar month cycle in 2022, are now perceivable, just as they are moving forward through each season of the future. Does any paid scientist have this lesson for educators today? Certain distinctive conditions within the magnetosphere have to occur in order for this atmospheric envelope to be opened each year, so that the Earth's tides can circulate each day of the year until the beginning of the next tidal season.
But our protective shield is not completely invincible.
During particularly strong space weather events such as high solar winds or large CMEs, Earth's magnetic field is disturbed and geomagnetic storms can penetrate the magnetosphere and lead to widespread radio and power blackouts as well as endangering astronauts and Earth-orbiting satellites. These events in the near-future will soon be mitigated when more and more people begin to understand the daily hydrogen path of the Earth's magnetospheric portion of the tides.
In 1859, a large solar storm known as the Carrington Event caused widespread telegraph system failures and in 1989, a CME accompanied a solar flare and plunged the entire province of Quebec, Canada into an electrical blackout that lasted around 12 hours according to a NASA statement.
The degree of magnetic disturbance from a CME depends on the CME's magnetic field and Earth's. If the CME's magnetic field is aligned with Earth's, pointing from south to north the CME will pass on by with little effect. However, if the CME is aligned in the opposite direction it can cause Earth's magnetic field to be reorganized,(opens in new tab) triggering large geomagnetic storms.
A less destructive and far prettier side effect of magnetosphere disturbances is the aurora above Earth's polar regions. The phenomenon is known as the northern lights (aurora borealis) in the Northern Hemisphere and the southern lights (aurora australis) in the Southern Hemisphere. Have you enjoyed this experience in either arctic regions of the Earth yet? Why not?
According to Science Daily, in the last 200 million years alone, Earth's magnetic poles have reversed hundreds of times in a process where north becomes south and south becomes north.
The magnetic poles flip approximately every 200,000 to 300,000 years according to NASA, though it has been more than twice that long since the last reversal. Earth's most recent magnetic reversal occurred approximately 790,000 years ago so we are rather overdue for another. But don't worry, the magnetic poles won't just switch overnight, it can take hundreds or even thousands of years for the poles to flip.
And, in fact, the field lines exhibit pole reversals each and every day--and not only at the geographic point of the poles but at the Earth's equator, too. This helps meteorologists predict emerging storm systems throughout the year.
MAGNETIC FIELDS ON OTHER PLANETS
Earth is not the only planet in the solar system to possess a magnetic field. Jupiter, Saturn, Uranus and Neptune all exhibit magnetic fields far stronger than Earth's, according to Union University(opens in new tab), though the underlying mechanisms driving these magnetic fields are not yet completely understood.
Not every planet is fortunate enough to have a protective magnetic layer. Mars does not have enough inner heat nor does it possess the liquid interior required to generate a magnetic field. Venus, on the other hand, has a liquid core but does not spin fast enough to generate a magnetic field.
I have a lot more to present about this topic.
Is there anyone out there????
There are 4--not 2!--types of daily tides on Earth Produced By its magnetospherology! Each have distinct traits, just like you and I! Where are my entertainers? We should launch a Moonwatchers' Network for TV to help distribute the new science! Pepper it with fine sci-fi, too!
If you want to read more about how scientists are investigating our planet's interior and nearby space environment without even leaving the ground check out these resources (opens in new tab)from the U.S. Geological Survey. Learn more about Earth's magnetic field with this short video from Arbor Scientific(opens in new tab). Explore magnetic and geographic poles in more detail with the Australian Antarctic Program(opens in new tab).
Daisy Dobrijevic joined Space.com in February 2022 as a reference writer having previously worked for our sister publication All About Space magazine as a staff writer. Before joining us, Daisy completed an editorial internship with the BBC Sky at Night Magazine and worked at the National Space Centre in Leicester, U.K., where she enjoyed communicating space science to the public. In 2021, Daisy completed a PhD in plant physiology and also holds a Master's in Environmental Science, she is currently based in Nottingham, U.K.