Sun news: These 2 astronomers changed how we see the sun

Sun news November 15: These 2 astronomers changed how we see the sun

Today’s top story: November 15 marks two breakthroughs that changed how we see the sun. The first revealed how planets orbit the sun. The second showed there’s a hidden world in sunlight — beyond what our eyes can see.

Johannes Kepler died on today’s date in 1630, but not before he’d discovered the laws of planetary motion. For example, he showed that planets travel around the sun in ellipses, or stretched circles, rather than perfect circles. And here’s a fun coincidence: NASA’s Kepler space telescope, named in his honor, received its final “goodnight” commands on November 15, 2018, exactly 388 years after his death.

About a century after Kepler’s death, William Herschel was born on this date in 1738. He began as a musician and composer, then became famous for discovering the planet Uranus in 1781. But his greatest sun discovery came in 1800. Herschel passed sunlight through a prism to split it into a rainbow. He then measured each color’s temperature with a thermometer. Surprisingly, the temperature kept rising just beyond the red end of the rainbow, where no color showed at all. In other words, Herschel had discovered that sunlight carries invisible light. Today we know the invisible “light” whose temperature he measured as infrared, or heat energy.

That discovery opened the door to studying the sun in light our eyes can’t see. In fact, many of the solar images in our daily reports, from extreme ultraviolet to X-rays, follow in Herschel’s footsteps.

Past 24 hours on the sun

(11 UTC November 14 – 11 UTC November 15)

Flare activity: Low. The sun fired six flares during the period: four C-class (common) and two B-class (weak). It produced no M-class or X-class flares.

• Strongest flare: C2.8 from AR4579, the big newcomer that rotated into view on the northeast limb, peaking at 21:27 UTC on November 14. It came with Type II and Type IV radio bursts, which often signal a shock wave racing out from the sun. The Type II burst suggested a shock speed of about 1,972 km/s. As a C-class flare, it caused no radio blackouts.
• Other notable flares: AR4576 fired a C2.2 at 18:45 UTC on November 14. AR4578 added a C1.1 at 21:08 UTC on November 14 and a C1.0 at 01:23 UTC on November 15. AR4576 also fired a B9.4 at 16:55 UTC and a B9.8 at 22:50 UTC on November 14.
• Lead flare producer: AR4576 produced three flares, one C-class and two B-class. Close behind, AR4578 fired two C-class flares.

Sunspot regions: Eight numbered sunspot regions dot the sun’s Earth-facing side. AR4566 has rotated out of view on the west limb. Meanwhile, yesterday’s unnumbered newcomer on the northeast limb is now AR4579.

• AR4568 (alpha): This simple region now sits on the sun’s southwest limb, about to rotate out of view. It’s stable or decaying.
• AR4572 (alpha): This region stayed on the disk and produced no flares.
• AR4574 (beta): This region sits at N16E20 in the northeast. It grew during the period.
• AR4575 (alpha): This region stayed on the disk and produced no flares.
• AR4576 (beta-gamma): This region sits at S17W39 in the southwest. It grew during the period and fired the C2.2 and both B flares. It’s now the most magnetically complex region on the sun’s Earth-facing side.
• AR4577 (beta): This region sits at S06E04, just south of the center of the solar disk. It grew during the period.
• AR4578 (beta): This region fired the C1.1 and C1.0 flares.
• AR4579 (alpha): This region sits at N15E72 near the northeast limb. It’s large and mature, and it grew during the period. It fired the C2.8 flare, plus the C5.5 we reported yesterday.

Blasts from the sun? Forecasters saw no Earth-directed coronal mass ejections (CMEs)in available coronagraph imagery. Still, analysts cataloged three CMEs in the period.

Past 24 hours in space weather

Solar wind: Solar wind speeds ran between about 350 and 400 km/s early in the period. Then, around 11 UTC on November 14, a weak boost pushed speeds to about 430 km/s. Afterward, speeds slowly eased back toward background levels.

Bt, Bz and magnetic coupling: The total interplanetary magnetic field (Bt) ranged from 4 to 6 nT. Meanwhile, Bz wavered between +4 and -4 nT. The phi angle stayed mostly negative. In other words, the solar wind coupled only weakly with Earth’s magnetic field.

Earth’s magnetic field: Earth’s magnetic field stayed quiet, with Kp values of 0 to 2. No geomagnetic storms occurred. As a result, auroras stayed mostly at high latitudes.

What’s ahead? Sun–Earth forecast

Flare activity forecast: Forecasters expect low activity, with a chance for M-class flares and R1 to R2 (minor to moderate) radio blackouts on November 15-17. Likewise, SIDC forecasters call C-class flares very likely, with a chance for M-class flares. The chance of M flares holds at 25%, and X flares stay at 5%, both unchanged from yesterday. The regions to watch are AR4576 (beta-gamma and growing) and AR4579 (large and growing). AR4578 also deserves a look after its two C flares.

Geomagnetic activity forecast:

• November 15: Mostly quiet conditions expected (Kp 0 to 2), with normal solar wind. Auroras should stay at high latitudes.
• November 16: Forecasters expect unsettled conditions with isolated active periods (Kp 3 to 4). A solar sector boundary crossing should arrive ahead of a positive-polarity coronal hole stream. However, Met Office forecasters expect quiet conditions unless the fast wind arrives late in the day. Auroras should mostly stay at high latitudes.
• November 17: Experts expect active conditions with isolated G1 (minor) storm levels (Kp 4 to 5) as the coronal hole stream arrives. SIDC forecasters also flag possible active conditions. In addition, one CME model run shows a glancing arrival at 15:58 UTC. Auroras could briefly reach northern Scotland and similar latitudes, as well as far southern New Zealand.
• November 18: Met Office forecasters expect unsettled conditions with isolated active intervals (Kp 3 to 4) to continue, plus a slight chance of G1 (Kp 5) storm levels.

Sun news November 14: Hello, big newcomer sunspot!

The sun now shows eight numbered sunspot regions on its Earth-facing side. But the most exciting one doesn’t have a number yet. A large new region is just peeking over the sun’s northeast limb, or edge. Even with only its “nose” showing, it already looks big in contrast to the smaller regions scattered across the rest of the sun’s visible face.

What’s more, it wasted no time. This newcomer fired the period’s strongest flare, a C5.5 that peaked at 18:21 UTC on November 13. Meanwhile, AR4566, the star of the past two weeks, is slipping over the sun’s southwest limb. So it’s time for a changing of the guard. Farewell, AR4566, and welcome, newcomer! Stay tuned.

Past 24 hours on the sun

(11 UTC November 13 – 11 UTC November 14)

Flare activity: Low. The sun produced 11 flares this period: 10 C-class (common) and one B-class (weak) flare.

• Strongest flare: C5.5 from an as-yet-unnumbered region rotating in on the northeast limb, peaking at 18:21 UTC on November 13.
• Other notable flares: AR4568 fired a C4.4, and AR4576 added a C1.3.
• Lead flare producer: AR4578 took the top spot, producing five of the period’s 11 flares.

Sunspot regions: The sun shows eight numbered regions on its Earth-facing side. The two regions we mentioned yesterday got their numbers this period. The one in the southeast is now AR4577, and the one in the southwest is AR4578.

• AR4566 (beta): This region now sits at the very edge of the sun’s southwest limb and will rotate out of view any minute. It produced no flares. It now shows a beta configuration, though its position makes a full analysis difficult.
• AR4568 (alpha): This region simplified from beta yesterday to alpha today. Even so, it fired a C4.4 flare.
• AR4572 (alpha): This region stayed stable and produced no flares.
• AR4574 (beta): This region produced no flares during the period.
• AR4575 (alpha): This region stayed stable and produced no flares.
• AR4576 (beta): This region fired one C1.3 flare.
• AR4577 (beta): This newcomer in the southeast got its number this period. It produced no flares.
• AR4578 (beta): This newcomer in the southwest grew quickly into a beta configuration and became the period’s lead flare producer.

Blasts from the sun? Analysts found no Earth-directed coronal mass ejections (CMEs) in available coronagraph imagery from SOHO or other sources.

Past 24 hours in space weather

Solar wind: Solar wind speeds stayed low on average during the period. However, forecasters expect a high-speed stream from the new Earth-facing coronal hole to start arriving in the coming days.

Bt, Bz and magnetic coupling: The total interplanetary magnetic field (Bt) stayed weak on average, though it rose slightly at the time of this writing. The north-south component (Bz) flipped between north and south. However, its strongest and most frequent swings pointed north. As a result, little solar wind energy reached Earth’s magnetosphere for most of the period.

Earth’s magnetic field: Like yesterday, geomagnetic conditions stayed very quiet, with Kp index values of 0 to 1. At the time of this writing, Kp sits at 1.

Sun news November 13: How the sun stripped Mars of its air

One year ago today, on November 13, 2025, NASA launched a Mars mission that will also be monitoring our sun. The twin ESCAPADE spacecraft lifted off on a Blue Origin New Glenn rocket from Cape Canaveral, Florida. Fittingly, the the powerful X5.1 flare we looked back on this week delayed the launch slightly.

So what’s the sun connection? The two spacecraft are headed to Mars to study how the solar wind interacts with the planet’s magnetic environment. Over time, that steady stream of particles from the sun stripped away much of the atmosphere from the young planet Mars. As a result, the planet cooled and lost its surface water, becoming the dry desert we see today.

ESCAPADE will also measure how solar storms affect Mars in real time. In other words, it will help forecast Martian space weather for future astronauts. The two ESCAPADE spacecraft are set to reach Mars in September 2027, after several flybys of Earth.

Past 24 hours on the sun

(11 UTC November 12 – 11 UTC November 13)

Flare activity: Low. The sun produced eight flares this period: seven C-class (common) and one B-class (weak) flare.

• Strongest flare: C4.9 from AR4566, peaking at 11:41 UTC on November 12.
• Lead flare producer: AR4566 stayed at the top of the list, producing six of the period’s eight flares.

Sunspot regions: The sun shows seven numbered sunspot regions on its Earth-facing side. One newcomer got its number this period: AR4576. In addition, two more regions are waiting for numbers. One in the southeast and one in the southwest each look like a pair of small spot groups.

• AR4566 (beta-gamma): This region kept decaying and fired fewer flares, but it’s still the top flare producer. It’s now nearing the sun’s western limb, where it will soon rotate out of view.
• AR4568 (beta): This region grew slightly.
• AR4572 (alpha): This region stayed stable and produced no flares.
• AR4573 (beta): This region stayed stable and produced one B flare.
• AR4574 (beta): This region produced no flares during the period.
• AR4575 (alpha): This region stayed stable and produced no flares.
• AR4576 (beta): This newcomer emerged in the southwest quadrant. It grew quickly into a beta configuration and fired one C1.1 flare.

Blasts from the sun? Analysts found no Earth-directed coronal mass ejections (CMEs) in available coronagraph imagery from SOHO or other sources.

Past 24 hours in space weather

Solar wind: Solar wind speeds kept dropping and reached low levels by the end of the period. Meanwhile, a new coronal hole is now turning to face Earth.

Bt, Bz and magnetic coupling: The total interplanetary magnetic field (Bt) stayed weak on average, though it rose slightly at the time of this writing. The north-south component (Bz) flipped between north and south, but its southward dips stayed weak, and its biggest swings pointed north. As a result, little solar wind energy reached Earth’s magnetosphere for most of the period.

Earth’s magnetic field: Geomagnetic conditions dropped to very quiet levels, with Kp index values of 0 to 1. At the time of this writing, Kp sits just above 1.

Sun news November 12: When the sun helped Philae phone home

Our sun doesn’t just power life on Earth. It also powers space exploration. Solar panels supply the electricity for most Earth-orbiting satellites and for many probes exploring the inner solar system. And 12 years ago today, sunlight played a key role in a nail-biting space exploration story.

On November 12, 2014, the Philae lander from the European Space Agency’s Rosetta mission made the first-ever landing on a comet, 67P/Churyumov-Gerasimenko.

But the landing went wrong. Philae’s anchoring harpoons failed to fire. So instead of settling at its planned landing site, the lander bounced twice. Eventually, it came to rest in the shadow of a cliff. That was a serious problem, because Philae ran on sunlight. A primary battery powered its first round of science, but its solar panels were supposed to recharge a second battery for longer-term work. Without enough sunlight to recharge, Philae went silent after about three days.

But eventually, the sun woke it up. As comet 67P swung closer to the sun, brighter sunlight warmed Philae and generated more electricity. Then, on June 13, 2015, after seven months of silence, Philae phoned home! Sadly, it never resumed regular science operations. Its last contact came on July 9, 2015. The saga is a reminder of just important our star’s energy is for space exploration.

Past 24 hours on the sun

(11 UTC November 11 – 11 UTC November 12)

Flare activity: Moderate. The sun produced 19 flares this period: one M-class (moderate) and 18 C-class (common) flares.

• Strongest flare: M1.7 from AR4566, peaking at 21:21 UTC on November 11. It caused an R1 (minor) radio blackout over the South Pacific Ocean, near Easter Island.
• Lead flare producer: Once again, AR4566 topped the list, producing almost all of the period’s flares. The only exception was a C1.3 that peaked at 20:44 UTC on November 11, from AR4575 in the southeast.

Sunspot regions: The sun shows six numbered sunspot regions on its Earth-facing side. Two newcomers got their numbers this period: AR4574 and AR4575.

• AR4566 (beta-gamma magnetic configuration): This region kept decaying and lost its delta complexity. Even so, it remains a prolific flare producer. It fired the period’s M flare and almost all of the C flares.
• AR4568 (beta): This region grew slightly.
• AR4572 (alpha): This region stayed stable and produced no flares.
• AR4573 (beta): This region stayed stable and produced no flares.
• AR4574 (beta): This newcomer rotated into view in the northeast and grew during the period.
• AR4575 (alpha): This newcomer rotated into view in the southeast and fired one C1.3 flare.

Blasts from the sun? Analysts found no Earth-directed coronal mass ejections (CMEs) in available coronagraph imagery from SOHO or other sources.

Past 24 hours in space weather

Solar wind: Solar wind speeds held at moderate levels until 19:30 UTC on November 11. After that, they eased to low-moderate levels for the rest of the period. Meanwhile, the high-speed stream from a coronal hole kept fading. However, a new coronal hole has rotated into view on the southeast limb, and it will soon turn toward Earth.

Bt, Bz and magnetic coupling: The total interplanetary magnetic field stayed weak on average. The north-south component (Bz) pointed mostly north, and its southward dips stayed weak. As a result, little solar wind energy reached Earth’s magnetosphere for most of the period.

Earth’s magnetic field: Geomagnetic conditions stayed quiet to unsettled, with Kp index values of 2 to 3. At the time of this writing, Kp sits just below 2.

Sun news November 11: A very different star 1 year later

The current roughly 11-year solar cycle peaked in late 2024. Since then, activity has been waning. And you get a clear indication of that when you compare today’s sun with the sun a year ago! While activity over the past day has been low, with only 10 C flares produced, this day last year saw our star fire an enormous X5.1 (strong) flare. It came from active region AR4274, which had also blasted an X flare on each of the two prior days. That was the last time we saw three X flares in three days. Now, exactly a year later, we haven’t seen a single X flare since July 4. Enjoy watching your star breathe after a frenzied solar maximum!

Past 24 hours on the sun

(11 UTC November 10 – 11 UTC November 11)

Flare activity: Low. The sun produced 11 flares this period: 10 C-class (common) and one B-class (weak) flare.

• Strongest flare: C2.8 from AR4566, peaking at 13:28 UTC on November 10.
• Lead flare producer: Once again, AR4566 produced almost all of the period’s flares. The only C-class exception was a C1.9 that peaked at 3:48 UTC on November 11, from the northeast newcomer now numbered AR4573.

Sunspot regions: The sun shows five numbered sunspot regions on its Earth-facing side. A newcomer in the northeast received a number this period: AR4573.

• AR4566 (beta-gamma-delta magnetic configuration): This region showed general signs of decay. Even so, it kept its delta complexity and remains the largest and most magnetically complex group on the sun.
• AR4565 (alpha): This small, magnetically simple region stayed stable and quiet.
• AR4568 (beta): This region grew slightly.
• AR4572 (alpha): This newcomer kept its simple alpha configuration. It stayed stable and produced no flares.
• AR4573 (beta): This newcomer emerged just south of AR4572 in the northeast quadrant, and it has already fired a C flare.

Blasts from the sun? Analysts found no Earth-directed coronal mass ejections (CMEs) in available coronagraph imagery from SOHO or other sources.

Past 24 hours in space weather

Solar wind: Solar wind speeds held at moderate levels during the period. Meanwhile, the high-speed stream from a coronal hole kept fading.

Bt, Bz and magnetic coupling: The total interplanetary magnetic field stayed weak on average. The north-south component (Bz) pointed mostly north, and its southward dips stayed weak. As a result, little solar wind energy reached Earth’s magnetosphere for most of the period.

Earth’s magnetic field: Geomagnetic conditions stayed quiet to unsettled, with Kp index values of 2 to 3. At the time of this writing, Kp sits at 2.

Sun news November 10: Powerful sunspot region facing Earth

A powerful sunspot region is staring right at us. AR4566 is the largest sunspot group currently visible on our star, and the most volatile, too. It has the highest possible magnetic complexity — beta-gamma-delta — which means it has the potential to fire large M (moderate) or even X (strong) flares. And now that it’s just rotated past the center of the Earth-viewed sun, it’s in the perfect position to send an eruption our way. So if it fires a flare strong enough to launch a coronal mass ejection (CME), that blob of solar stuff could head straight for Earth and potentially trigger beautiful auroras. Stay tuned!

Past 24 hours on the sun

(11 UTC November 9 – 11 UTC November 10)

Flare activity: Low. The sun produced 19 flares this period, all C-class (common).

• Strongest flare: C9.3 from AR4566, peaking at 08:34 UTC on November 10.
• Other notable flares: AR4566 also fired a C5.3 that peaked at 14:26 UTC and a C5.1 at 17:14 UTC on November 9. Then, this morning, it added a C8.6 at 08:06 UTC on November 10.
• Lead flare producer: AR4566 produced 18 of the period’s 19 flares. The only exception was a C1.9, that peaked at 01:45 UTC on November 10, from the newcomer in the northeast.

Sunspot regions: Four numbered regions currently dot the sun’s Earth-facing side. AR4571 is gone from view. However, a newcomer in the northeast got its number this period: AR4572.

• AR4566 (beta-gamma-delta): This region showed slight signs of decay, and its spots began to spread apart. Even so, it kept its delta complexity and remains the largest and most magnetically complex group on the sun.
• AR4565 (alpha): This small, magnetically simple region stayed stable and quiet.
• AR4568 (beta): This region grew a little during the period.
• AR4571 (beta): This region in the southwest is no longer visible.
• AR4572 (alpha): This newcomer rotated into view near the northeast limb, or edge, with a simple alpha configuration.

Blasts from the sun? Analysts found no Earth-directed CMEs in available coronagraph imagery from SOHO or other sources.

Past 24 hours in space weather

Solar wind: Solar wind speeds eased from high to moderate levels during the period. That’s because the high-speed stream from a negative-polarity coronal hole started to fade.

Bt, Bz and magnetic coupling: The total interplanetary magnetic field (Bt) weakened again. The north-south component (Bz) kept flipping between north and south, but its southward dips stayed weak. As a result, little solar wind energy reached Earth’s magnetosphere.

Earth’s magnetic field: Geomagnetic conditions settled to quiet and unsettled levels, with Kp index values of 2 to 3. At the time of this writing, Kp sits at 2.

Sun news November 9: Auroras continue! More tonight at northern U.S. latitudes?

A powerful stream of fast solar wind kept buffeting Earth over the past 24 hours. Speeds peaked near 814 km/s, even faster than yesterday. The stream pushed Earth’s magnetic field to G1 (minor) geomagnetic storm levels. The source is the large coronal hole we’ve been tracking in the sun’s atmosphere. Its influence should gradually fade over the coming days.

Meanwhile, AR4566, the sun’s most complex sunspot region, stayed restless. It fired one M-class (moderate) flare and a steady stream of C flares (common). It has now crossed the center of the sun’s face, so its future big eruptions would aim more directly at Earth. Forecasters expect more M flares in the days ahead, with a slight chance of an X-class (strong) flare.

So what about tonight? Forecasters see a chance of more G1 (minor) storm intervals today, November 9, before conditions settle toward midweek. If you live at high latitudes, keep an eye out for auroras tonight. Still, displays will likely be less widespread than the weekend show, when auroras reached northern Minnesota.

Past 24 hours on the sun

(11 UTC November 8 – 11 UTC November 9)

Flare activity: Moderate. The sun produced 20 flares during the period: one M-class and 19 C-class.

• Strongest flare: M1.1 from AR4566, peaking at 18:27 UTC on November 8. It caused a brief R1 (minor) radio blackout.
• Other notable flares: AR4566 also fired a C8.0 that peaked at 20:53 UTC on November 8. Then, on November 9, it added a C4.7 at 01:14 UTC and a C5.7 at 04:10 UTC.
• Lead flare producer: AR4566 produced 19 of the 20 flares. Only one C1.3 flare, peaking at 08:33 UTC on November 9, came from an unidentified source.

Sunspot regions: Four numbered sunspot regions dot the sun’s Earth-facing side, down from six yesterday. AR4567 rotated out of view, while AR4569 and AR4570 decayed.

• AR4566 (beta-gamma-delta): This region sits near disk center and remains the largest and most magnetically complex group on the sun. Its intermediate and trailing spots grew larger. In addition to frequent C flares, it fired the period’s M1.1 flare. As a result, it’s the main threat for stronger flares in the days ahead.
• AR4565 (alpha): This small, magnetically simple region stayed stable and quiet.
• AR4568 (beta): This region re-emerged but stayed relatively simple and quiet.
• AR4571 (beta): This newcomer is the region we saw developing in the southwest yesterday. Now numbered, it stayed quiet this period.

Blasts from the sun? Analysts found no Earth-directed coronal mass ejections (CMEs) in available coronagraph imagery from SOHO or other sources.

Past 24 hours in space weather

Solar wind: Solar wind speeds stayed high throughout the period, driven by a high-speed stream from a negative-polarity coronal hole. Speeds peaked at about 814 km/s. Meanwhile, particle density ran below average and slowly fell.

Bt, Bz and magnetic coupling: The total interplanetary magnetic field (Bt) reached 10 nT. The north-south component (Bz) dipped as far south as about -9 nT. However, it swung back and forth and never stayed south for long. The phi angle pointed mostly in the negative (toward-sun) sector, matching the coronal hole’s negative polarity.

Earth’s magnetic field: Geomagnetic conditions ranged from unsettled to G1 (minor) storm levels. The Kp index reached 5, with the stormiest stretch from 00 to 3 UTC on November 9. After that, conditions eased slightly. Auroras were possible at high latitudes, including northern Scotland, as well as far southern New Zealand.

Energetic particles: The greater than 2 MeV electron flux at geostationary orbit reached high levels. Meanwhile, the greater than 10 MeV proton flux stayed at background levels.

Sun news November 8: Auroras glowed over northern Minnesota last night

The fast solar wind has arrived, and so have the auroras! A coronal hole high-speed stream slammed into Earth’s magnetic field late on November 7. It pushed solar wind speeds above 700 km/s and sparked a G1 (minor) geomagnetic storm. As a result, auroras reached all the way down to the lower 48 U.S. states, where observers spotted a green glow over northern Minnesota.

And the show might not be over. Forecasters expect unsettled-to-active conditions to continue through November 9, with a chance of G2 (moderate) storm levels. So aurora watchers across the northern U.S., Canada and northern Europe, head outside after dark tonight and look north. If you catch the lights, share your photos with our community!

Meanwhile, AR4566, the sun’s most complex sunspot region, kept churning out flares at a remarkable pace over the past day. It fired 20 flares in the past 24 hours, including three M-class flares. Moreover, it still has its beta-gamma-delta magnetic setup. That keeps the door open for more moderate to strong flares in the next few days. And there’s a new twist: AR4566 has now rotated close to the center of the sun’s face, where any big eruption would aim more directly at Earth.

For now, though, observers spotted no Earth-directed coronal mass ejections (CMEs). The coronal hole wind alone is driving today’s geomagnetic forecast.

Past 24 hours on the sun

(11 UTC November 7 – 11 UTC November 8)

Flare activity: Moderate. The sun produced 20 flares during the period: three M-class (moderate) and 17 C-class (common). All of them came from a single active region.

• Strongest flare: M1.9 from AR4566 (S06E04), peaking at 18:42 UTC on November 7. It caused an R1 (minor) radio blackout.
• Second M flare: M1.7 from AR4566, peaking at 07:46 UTC on November 8. It also caused an R1 (minor) radio blackout.
• Other notable flares: AR4566 also fired an M1.4 that peaked at 17:17 UTC on November 7, with another R1 radio blackout. Among the C flares, a C9.1 peaked at 03:31 UTC and a C8.0 peaked at 08:43 UTC on November 8. Both came close to M-class territory.
• Lead flare producer: AR4566 produced every flare of the period.

Sunspot regions: Six numbered regions dot the sun’s Earth-facing side. In addition, a new region is developing in the southwest.

• AR4566 (beta-gamma-delta): This region sits near the center of the solar disk (S06E06) and remains the sun’s dominant feature. Its intermediate and trailing spots kept developing, so it held on to its complex magnetic setup. It produced all 20 of the period’s flares, including the three M flares. As a result, it’s the top candidate for more M flares and possible X-class flares.
• AR4569: This small region continued to fade and produced no notable activity.
• Remaining regions: The four other numbered regions were stable or decaying, with simple magnetic setups. None produced reportable flares. Meanwhile, the new region in the southwest is still developing, and forecasters haven’t classified it yet.

Blasts from the sun? Observers detected no Earth-directed CMEs during the period. Analysts cataloged two CMEs, but neither poses a threat to Earth.

Past 24 hours in space weather

Solar wind: Solar wind speeds rose sharply as a high-speed stream from a negative-polarity coronal hole arrived. Speeds climbed from a low of about 425 km/s to a peak near 736 km/s.

Bt, Bz and magnetic coupling: The total interplanetary magnetic field (Bt) reached 15 nT. Meanwhile, the north-south component (Bz) dipped as far south as -11 nT. That allowed solar wind energy to couple efficiently into Earth’s magnetosphere.

Earth’s magnetic field: Geomagnetic activity ranged from quiet to active (Kp 2 to 4) for most of the period. However, Kp reached 5, a G1 (minor) geomagnetic storm, between 18:00 and 21:00 UTC on November 7. Then, after dark, auroras appeared as far south as northern Minnesota in the U.S.

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Bottom line: Sun news November 14, 2026: Farewell, AR4566! A big new sunspot region is peeking over the sun’s northeast edge and has already fired the top flare.

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