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See Also
See Again
© Getty Images
0 / 30 Fotos
What is a flare?
- A solar flare is an intense burst of radiation. It involves a large release of magnetic energy, that is associated with sunspots.
© Shutterstock
1 / 30 Fotos
What is a flare?
- Solar flares are the largest explosive events in our entire solar system. They can be viewed as bright areas appearing on the Sun.
© Shutterstock
2 / 30 Fotos
What is a flare?
- A flare can last anywhere from a few minutes to several hours in length. Solar flares release photons (light particles) at almost every wavelength in the spectrum.
© Shutterstock
3 / 30 Fotos
Measurement
- The primary ways a solar flare is measured is via x-rays and optical light. Sites where particles (electrons, protons, and heavier particles) are accelerated are also considered a solar flare.
© Shutterstock
4 / 30 Fotos
Solar flares in 2024
- In February 2024, the Sun emitted two strong solar flares. The first one peaked at 6:07 pm EST on February 21, 2024, and the second peaked at 1:32 am EST on February 22, 2024.
© Shutterstock
5 / 30 Fotos
Solar Dynamics Observatory
- NASA's Solar Dynamics Observatory watches the Sun constantly. It captured images of the solar flare as they occurred, in February 2024.
© Shutterstock
6 / 30 Fotos
Interruptions
- Flares and solar eruptions can impact radio communications, electric power grids, and navigation signals.
© Shutterstock
7 / 30 Fotos
Interruptions
- As a result, depending on the strength of the explosion, they can pose potential risks to both spacecraft and astronauts.
© Shutterstock
8 / 30 Fotos
Classification
- The intensity of the explosion determines what classification the flare belongs to. The most powerful are X-class flares, followed by M-, C- and B-class; A-class flares are the smallest.
© Shutterstock
9 / 30 Fotos
Classification
- The first of the flares was classified as an X1.8 flare. The second flare was classified as an X1.7 flare. X-class denotes the most intense flares, while the number provides more information about its strength.
© Shutterstock
10 / 30 Fotos
Energy output
- Similar to the Richter scale that measures the strength of earthquakes, each class letter represents a 10-fold increase in energy output.
© Shutterstock
11 / 30 Fotos
Energy output
- M-class flares are 10 times smaller than X-class flares, followed by C-class, B-class, and finally A-class; A-class flares are too weak to significantly affect Earth.
© Shutterstock
12 / 30 Fotos
2003 solar flare
- A 2003 solar flare was so powerful that it overloaded the sensors measuring it. Before cutting out, the sensors reported an X28 flare.
© Shutterstock
13 / 30 Fotos
Geomagnetic storms
- Strong M-class and X-class flares can lead to a large release of plasma and magnetic field from the Sun. This can result in geomagnetic storms.
© Shutterstock
14 / 30 Fotos
Geomagnetic storms
- Geomagnetic storms can lead to auroras closer to the equator than is possible during calm conditions. In 1989, an aurora borealis could be seen as far south as Florida and Cuba following a solar flare.
© Shutterstock
15 / 30 Fotos
Radio frequency
- During an eruption, M-class and X-class flares can also cause minor to extensive radio blackouts on the side of Earth facing the Sun.
© Shutterstock
16 / 30 Fotos
Solar cycle
- These outbursts are intrinsically linked to the solar cycle. This is an approximately 11-year cycle of solar activity, driven by the Sun's magnetic field.
© Shutterstock
17 / 30 Fotos
Magnetically mixed-up
- The Sun's surface is a magnetically mixed-up place. Electrically charged gases generate electrical currents. These currents then act as a magnetic dynamo, creating magnetic fields.
© Shutterstock
18 / 30 Fotos
Magnetically mixed-up
- Due to the turbulent nature of the gases that create them, these magnetic fields continually twist, tangle, and reorganize themselves.
© Shutterstock
19 / 30 Fotos
Electromagnetic radiation
- This unsettled magnetic field behavior is what leads to the trigger of solar flare eruptions, when vast amounts of electromagnetic radiation are released from the surface of the Sun.
© Shutterstock
20 / 30 Fotos
Electromagnetic radiation
- Electromagnetic radiation is a form of energy that includes radio waves, microwaves, X-rays, gamma rays, and visible light.
© Shutterstock
21 / 30 Fotos
Sunspots
- Sunspots are darker, cooler portions of the solar surface where magnetic fields are particularly strong. Solar flares tend to originate from these.
© Shutterstock
22 / 30 Fotos
Sunspots
- During periods of low solar activity, when there are no sunspots present, it is unlikely for a solar flare to occur.
© Shutterstock
23 / 30 Fotos
Solar cycle 25
- We are currently in solar cycle 25, with the solar maximum predicted to occur in 2025. The peak of sunspot activity coincides with the solar maximum.
© Shutterstock
24 / 30 Fotos
Solar flare speed
- We don't have long to respond to solar flares when they occur. The radiation emitted travels at the speed of light and can reach the Earth in just eight minutes.
© Shutterstock
25 / 30 Fotos
Solar flare speed
- Our ability to predict space weather has improved in the past few years, but it's still a tricky business. Several organizations keep a close eye on solar weather fluctuations.
© Shutterstock
26 / 30 Fotos
Flare reporting
- Organizations such as NASA, NOAA, and the U.S. Air Force Weather Agency (AFWA) monitor the Sun for such flares.
© Shutterstock
27 / 30 Fotos
Flare reporting
- These organizations can send out warnings to technology sectors vulnerable to solar flare activity so that appropriate precautions can be taken.
© Shutterstock
28 / 30 Fotos
Disruption
- While solar flares can cause considerable technological disruption, their energy cannot do any lasting damage to the Earth itself. So you don't need to worry! Sources: (Space) (NASA) (NCEI) (Deseret News) (Scientific American)
© Shutterstock
29 / 30 Fotos
© Getty Images
0 / 30 Fotos
What is a flare?
- A solar flare is an intense burst of radiation. It involves a large release of magnetic energy, that is associated with sunspots.
© Shutterstock
1 / 30 Fotos
What is a flare?
- Solar flares are the largest explosive events in our entire solar system. They can be viewed as bright areas appearing on the Sun.
© Shutterstock
2 / 30 Fotos
What is a flare?
- A flare can last anywhere from a few minutes to several hours in length. Solar flares release photons (light particles) at almost every wavelength in the spectrum.
© Shutterstock
3 / 30 Fotos
Measurement
- The primary ways a solar flare is measured is via x-rays and optical light. Sites where particles (electrons, protons, and heavier particles) are accelerated are also considered a solar flare.
© Shutterstock
4 / 30 Fotos
Solar flares in 2024
- In February 2024, the Sun emitted two strong solar flares. The first one peaked at 6:07 pm EST on February 21, 2024, and the second peaked at 1:32 am EST on February 22, 2024.
© Shutterstock
5 / 30 Fotos
Solar Dynamics Observatory
- NASA's Solar Dynamics Observatory watches the Sun constantly. It captured images of the solar flare as they occurred, in February 2024.
© Shutterstock
6 / 30 Fotos
Interruptions
- Flares and solar eruptions can impact radio communications, electric power grids, and navigation signals.
© Shutterstock
7 / 30 Fotos
Interruptions
- As a result, depending on the strength of the explosion, they can pose potential risks to both spacecraft and astronauts.
© Shutterstock
8 / 30 Fotos
Classification
- The intensity of the explosion determines what classification the flare belongs to. The most powerful are X-class flares, followed by M-, C- and B-class; A-class flares are the smallest.
© Shutterstock
9 / 30 Fotos
Classification
- The first of the flares was classified as an X1.8 flare. The second flare was classified as an X1.7 flare. X-class denotes the most intense flares, while the number provides more information about its strength.
© Shutterstock
10 / 30 Fotos
Energy output
- Similar to the Richter scale that measures the strength of earthquakes, each class letter represents a 10-fold increase in energy output.
© Shutterstock
11 / 30 Fotos
Energy output
- M-class flares are 10 times smaller than X-class flares, followed by C-class, B-class, and finally A-class; A-class flares are too weak to significantly affect Earth.
© Shutterstock
12 / 30 Fotos
2003 solar flare
- A 2003 solar flare was so powerful that it overloaded the sensors measuring it. Before cutting out, the sensors reported an X28 flare.
© Shutterstock
13 / 30 Fotos
Geomagnetic storms
- Strong M-class and X-class flares can lead to a large release of plasma and magnetic field from the Sun. This can result in geomagnetic storms.
© Shutterstock
14 / 30 Fotos
Geomagnetic storms
- Geomagnetic storms can lead to auroras closer to the equator than is possible during calm conditions. In 1989, an aurora borealis could be seen as far south as Florida and Cuba following a solar flare.
© Shutterstock
15 / 30 Fotos
Radio frequency
- During an eruption, M-class and X-class flares can also cause minor to extensive radio blackouts on the side of Earth facing the Sun.
© Shutterstock
16 / 30 Fotos
Solar cycle
- These outbursts are intrinsically linked to the solar cycle. This is an approximately 11-year cycle of solar activity, driven by the Sun's magnetic field.
© Shutterstock
17 / 30 Fotos
Magnetically mixed-up
- The Sun's surface is a magnetically mixed-up place. Electrically charged gases generate electrical currents. These currents then act as a magnetic dynamo, creating magnetic fields.
© Shutterstock
18 / 30 Fotos
Magnetically mixed-up
- Due to the turbulent nature of the gases that create them, these magnetic fields continually twist, tangle, and reorganize themselves.
© Shutterstock
19 / 30 Fotos
Electromagnetic radiation
- This unsettled magnetic field behavior is what leads to the trigger of solar flare eruptions, when vast amounts of electromagnetic radiation are released from the surface of the Sun.
© Shutterstock
20 / 30 Fotos
Electromagnetic radiation
- Electromagnetic radiation is a form of energy that includes radio waves, microwaves, X-rays, gamma rays, and visible light.
© Shutterstock
21 / 30 Fotos
Sunspots
- Sunspots are darker, cooler portions of the solar surface where magnetic fields are particularly strong. Solar flares tend to originate from these.
© Shutterstock
22 / 30 Fotos
Sunspots
- During periods of low solar activity, when there are no sunspots present, it is unlikely for a solar flare to occur.
© Shutterstock
23 / 30 Fotos
Solar cycle 25
- We are currently in solar cycle 25, with the solar maximum predicted to occur in 2025. The peak of sunspot activity coincides with the solar maximum.
© Shutterstock
24 / 30 Fotos
Solar flare speed
- We don't have long to respond to solar flares when they occur. The radiation emitted travels at the speed of light and can reach the Earth in just eight minutes.
© Shutterstock
25 / 30 Fotos
Solar flare speed
- Our ability to predict space weather has improved in the past few years, but it's still a tricky business. Several organizations keep a close eye on solar weather fluctuations.
© Shutterstock
26 / 30 Fotos
Flare reporting
- Organizations such as NASA, NOAA, and the U.S. Air Force Weather Agency (AFWA) monitor the Sun for such flares.
© Shutterstock
27 / 30 Fotos
Flare reporting
- These organizations can send out warnings to technology sectors vulnerable to solar flare activity so that appropriate precautions can be taken.
© Shutterstock
28 / 30 Fotos
Disruption
- While solar flares can cause considerable technological disruption, their energy cannot do any lasting damage to the Earth itself. So you don't need to worry! Sources: (Space) (NASA) (NCEI) (Deseret News) (Scientific American)
© Shutterstock
29 / 30 Fotos
Is today's severe solar storm something to fear?
An intense geomagnetic storm may affect large parts of the US starting on Friday
© Getty Images
Earth is heating up, but climate change isn't the only threat. The Sun also experiences 'weather' changes, and one thing you might have heard about is solar flares. But what are they, really? Well, we can think of them as storms that take place on the surface of the Sun. Energy that's built up is released, creating a magnetic storm. Fluctuations to the magnetic field can sometimes be felt as far away as here on Earth! So, should we be worried? Well, that all depends on the size of the storm.
The space weather department of the National Oceanic and Atmospheric Administration (NOAA) has predicted that large parts of the US will experience disruptions due to a “severe” G4 geomagnetic storm on Friday, May 10. The major geomagnetic storm, i.e. disruption to the Earth's magnetic field, was caused by an intense solar storm expelling powerful magnetic fields in our direction from the sun. A G4 geomagnetic storm is the second-strongest of its kind, and is capable of causing "widespread voltage problems,” issues with the electric power grid, radio and navigation systems, and other communications systems.
The effects of the storm are expected to hit on Friday and may continue through Sunday. One upside to this jarring news is that such cosmic weather events can trigger incredible displays of the Northern Lights in places they never normally appear. NOAA is predicting that they may be visible as far south as Alabama and Northern California. NASA has emphasized that harmful radiation from solar flares like this “cannot pass through Earth’s atmosphere to physically affect humans on the ground.” However, they can be dangerous to astronauts and damage satellites and other technology in space. The last time the NOAA issued a geomagnetic storm warning of this magnitude was in 2005.
If you're interested to learn more about solar storms and how they can impact the Earth, click through the gallery.
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