Sol (Sun) and its phenomena

SOLAR CYCLE 25 ACTIVITY REPORT NOVEMBER 04_2023

FILAMENTS ERUPTIONS AND A COMET CRASHING INTO THE SUN:. Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C4 event observed at 0132 UTC from Region 3480 (S11E64).

The twisted structure of the eruption stretches over 100,000 km from end to end. It is not violent enough to throw the hot plasma (50,000K) into interplanetary space as most of it falls back on to the Sun's surface.
Note the dark filament running diagonally across the NW quadrant of the Sun. It starts to get dynamic and lifts off - it as about 700,000km long. That then causes a second slightly smaller filament to erupt to its north.
The Sun-diving comet comes in from about 5 o'clock. It is small and relatively faint so it might be best to view this full-screen. It disappears when the CME passes over it, though the CME may not have hit it directly.

There are currently 8 sunspot regions on the solar disk: AR3472, AR3473 AR3474 AR3476, AR3477, AR3478, AR3479 and new region AR3480
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Total number of sunspots has decreased to 106 (36 of these are grouped into 8 active regions) NOAA forecasts for the next 24h: 90% chance for C flares, 40% chance M flares and 5% chance for X flares.

AR3474 (S18W58) has a beta-gamma magnetic field that harbors energy for M-class flares.​

● Auroral Activity

The geomagnetic field has been at quiet levels for the past 24 hours. On November 03 Solar wind speed reached a peak of 506 km/s at 0844 UTC Total IMF reached 3 nT at 05:30 UTC​

GEOMAGNETIC STORM WATCH (G2): High-latitude sky watchers should be alert for auroras this weekend when as many as three CMEs could make contact with Earth's magnetic field. The first two CMEs are mostly off-target, but they could deliver glancing blows on Nov. 4th. If they combine to form a Cannibal CME, the result could be a minor G1-class geomagnetic storm.​

Of greater interest is the third CME, which left the sun yesterday:​

This halo CME appears to be heading directly toward Earth. It was hurled into space by a complex eruption of magnetic filaments snaking across the sun's northern hemisphere: movie.

A NASA model of the CME suggests it will arrive on Nov. 5th between 1200 UT and 1800 UT. Its impact could add to that of the preceding two CMEs, boosting geomagnetic storms to category G2--a level that may require all three CMEs to be effective. If such a storm occurs, it could produce auroras in the USA from New York to Oregon. SpaceWeather.com​

Aurora Oval Bz: -2.67 nT South
aurora-map.jpg
● Current Conditions at 03:30 UTC on November 04

▪︎ Geospace quiet (kp 1)
▪︎ Solar wind speed record: 472.5 km/sec (Elevated speed)
▪︎ density: 4 p/cm³ (low density)
▪︎ Interplanetary Magnetic Field (IMF)
Bt: 3.5 nT
▪︎ Thermosphere Climate Index
today: 19.48x1010 W Warm
▪︎ Neutron Counts today: - 3.6 % (Low)
▪︎ X-ray Solar Flare: C3 2238 UT Nov03
▪︎ Sunspot number: 106 (SN 113 November 03)
▪︎ Spotless Days 2023 total: 0 days (0%)
▪︎ Solar wind flowing from a coronal hole should reach Earth on Nov. 7th.
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SOLAR CYCLE 25 ACTIVITY REPORT NOVEMBER 05_2023

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C3 event observed at 22:38 UTC from Region 3480 (S11E64) on November 04
There are currently 7 sunspot regions on the solar disk: AR3472, AR3474, AR3477, AR3478 AR3479, AR3480 and new region AR3481
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AR3473 & AR3476 are gone

Total number of sunspots has decreased to 95 (25 of these are grouped into 7 active regions) NOAA forecasts for the next 24h: 95% chance for C flares, 25% chance M flares and 5% chance for X flares. All regions have stable magnetic fields

● Auroral Activity

The geomagnetic field has been at quiet to minor storm levels (G1) levels for the past 24 hours. On November 04 Solar wind speed reached a peak of 484 km/s at 10:24 UTC Total IMF reached 17 nT at 17:39 UTC Active Geomagnetic conditions reached at 19:45, Minor G1 geomagnetic storm (kp5) threshold reached at 20:55 UTC
GEOMAGNETIC STORM WATCH (G2): NASA and NOAA now agree: A full halo CME is expected to hit Earth's magnetic field this weekend. Its arrival probably during the late hours of Nov. 5th could spark a G2-class geomagnetic storm with auroras in northern Europe, Canada and US states from New York to Oregon.
The CME was hurled in our direction on Nov. 3rd by a complex eruption of solar magnetic filaments. SOHO corographraphs recorded this movie of the cloud leaving the sun:​

Not shown are two to three other CMEs, which left the sun just before and just after the halo event. Analysts had to untangle multiple CMEs to produce a forecast. To get a sense of the uncertainties, compare the NASA model to the NOAA model. Predicted arrival times range from 1200 UT on Nov. 5th to 0000 UT on Nov. 6th, with NASA favoring earlier, NOAA later.

Either way, high-latitude auroras are possible on the night of Nov. 5-6 SpaceWeather.com​

Aurora Oval Bz: 5.93 nT North
aurora-map.jpg
● Current Conditions at 04:15 UTC on November 05

▪︎ Geospace unsettled (kp 3)
▪︎ Solar wind speed record: 328 km/sec (Normal speed)
▪︎ density: 12 p/cm³ (low density)
▪︎ Interplanetary Magnetic Field (IMF)
Bt: 7.67 nT
▪︎ Thermosphere Climate Index
today: 19.37x1010 W Warm
▪︎ Neutron Counts today: - 3.3 % (Low)
▪︎ X-ray Solar Flare: C1 0221 UT Nov05
▪︎ Sunspot number: 95 (SN 106 November 04)
▪︎ Spotless Days 2023 total: 0 days (0%)
▪︎ Solar wind flowing from a coronal hole should reach Earth on Nov. 7th.
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CME IMPACT SPARKS STRONG GEOMAGNETIC STORM: Geomagnetic storms (now category G3) are underway on Nov. 5th in respond to the impact of a CME at 0905 UT. This could be the early arrival of a full-halo CME, which we warned readers about yesterday. But maybe not. We knew that another lesser CME was preceding the halo, and this could be it. If the full halo CME is still coming, it could intensify geomagnetic activity even more when it arrives later today.

The CME impact sparked auroras in more than a dozen US states. Dan Bush sends this picture from Albany, Missouri (+40.2N):


"This display lasted about 15-20 minutes," says Bush. "The red was intense enough that it was easily visible to the dark-adapted naked eye."

Other reports of mid-latitude auroras have come from Colorado (+40.1N) and Kansas (+38.2). Simiar displays may be seen again tonight if the persists after nightfall.

Meanwhile, inside the Arctic Circle, a rare display of naked-eye red auroras is in progress. "In 10 years plus of shooting aurora never seen anything like it," says Oliver Wright, a longtime guide for Lights over Lapland, who sends this picture from Abisko, Sweden:


"I could not belive my eyes as the whole sky was blood red to the naked eye," says Wright. "Unbelievable!"

Red auroras come from atomic oxygen in Earth's upper atmosphee shining at 6300 Å. The human eye is famously insensitive to this wavelength; it takes a strong geomagnetic storm (like today's) to make the red glow visible to the unaided eye.



Periods of geomagnetic storm

● Minor G1 geomagnetic storm (Kp5)
Threshold Reached: 15:28 UTC
● Moderate G2 geomagnetic storm (Kp6)
Threshold Reached: 16:05 UTC
● Strong G3 geomagnetic storm (Kp7)
Threshold Reached: 17:35 UTC

▪︎ Current Conditions at 20:30 UTC on November 05

▪︎ strong geomagnetic storm (kp 6)
▪︎ Solar wind speed record: 473 km/sec (Elevated speed)
▪︎ density: 33.19 p/cm³ (low density)
▪︎ Interplanetary Magnetic Field (IMF)
Bt: 15.6 nT

Aurora Oval Bz: -0.99 nT South

aurora-map.jpg

 
SOLAR CYCLE 25 ACTIVITY REPORT NOVEMBER 06_2023

RED SKIES AND PURPLE BEAMS
Solar activity has been at moderate levels for the past 24 hours. The largest solar event of the period was a M1 event observed at 1143 UTC from Region 3480 (S09E40) on November 05. This flare caused a Minor R1 radio blackout over Atlantic Ocean

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A second M class flare from the same AR3480 occurred at 14:32 UTC and caused a Minor R1 radio blackout over Atlantic Ocean.

There are currently 8 sunspot regions on the solar disk: AR3472, AR3474, AR3477, AR3478 AR3479, AR3480, AR3481 and new region
AR3482
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Total number of sunspots has decreased to 81 (25 of these are grouped into 8 active regions) NOAA forecasts for the next 24h: 95% chance for C flares, 25% chance M flares and 5% chance for X flares. All regions have stable magnetic fields

● Auroral Activity

The geomagnetic field has been at quiet to strong storm levels (G3) levels for the past 24 hours. On November 05 Active geomagnetic conditions (Kp4) were reached at 10:02 UTC Minor G1 geomagnetic storm (Kp5) threshold reached at 10:18 UTC Moderate G2 geomagnetic storm (Kp6) threshold reached at 11:05 UTC Solar wind speed reached a peak of 517 km/s at 12:33 UTC Strong G3 geomagnetic storm (Kp7)
threshold reached at 17:35 UTC
Minor G1 geomagnetic storm (Kp5) threshold reached at 03:42 UTC. Total IMF reached 44 nT at 11:51 UTC
WHAT JUST HAPPENED? Two CMEs hit Earth over the weekend--one on Saturday, Nov. 4th, another on Sunday, Nov. 5th. The double blow sparked a strong G3-class geomagnetic storm with auroras as far south as Colorado (+40.1N) and Texas (+33.6N). The storm is now subsiding with isolated periods of minor G1-class storming expected through Nov. 6th SpaceWeather.com​

Aurora Oval Bz: -3.11 nT South
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NOT ALL THE LIGHTS WERE AURORAS: At the apex of the storm, bright lights danced across the skies of northern Europe. Not all the lights were auroras. "To our utter amazement we observed a striking phenomenon," reports Martin McKenna of Swatragh, N. Ireland. "It was STEVE!"​
"We were blown away by the intensity of the purple beam," continues McKenna."We could see it plainly with the naked eye, swelling and flickering in brilliance with delicate structures like those seen within a feather. My mate Conor likened it to a celestial funnel cloud or tornado changing form in real time."​
STEVE is a recent discovery. It looks like an aurora, but it is not. The soft purple glow is caused by hot (3000°C) rivers of gas flowing through Earth’s magnetosphere at speeds exceeding 6 km/s (13,000 mph). These rivers are energized by strong geomagnetic storms like the one that happened over the weekend.​
Wil Cheung observed an even more dramatic apparition of STEVE over Whitley Bay, England:​
"It lasted for more than an hour," marvels Cheung. "Strong auroras danced in the north while STEVE flowed through the sky to my south."​
Red aurora in Greece
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● Current Conditions at 04:45 UTC on November 06

▪︎ Minor G1 Geomagnetic storm (kp 5)
▪︎ Solar wind speed record: 522 km/sec (Moderately high speed)
▪︎ density: 12 66 p/cm³ (low density)
▪︎ Interplanetary Magnetic Field (IMF)
Bt: 16.49 nT
▪︎ Thermosphere Climate Index
today: 19.42x1010 W Warm
▪︎ Neutron Counts today: - 3.3 % (Low)
▪︎ X-ray Solar Flare: C9 0330 UT Nov06
▪︎ Sunspot number: 81 (SN 95 November 05)
▪︎ Spotless Days 2023 total: 0 days (0%)
▪︎ Solar wind flowing from a coronal hole should reach Earth on Nov. 7th.
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September 1, 2023
On September 1st, 1859, a ferocious solar storm took place that impacted much of the planet. This ferocious solar storm is now known as the “Carrington Event”, named after the British astronomer, Richard Carrington, who witnessed the largest solar flare from his own private observatory which caused a major coronal mass ejection (CME) to travel directly toward Earth. Recent studies of solar storms have warned that these type of “Carrington Events” may not be quite as rare as once thought (e.g., Hayakawa et al). Many previous studies leaned heavily on Western Hemisphere accounts, omitting data from the Eastern Hemisphere. A super storm of the same magnitude as the “Carrington Event” in today’s world would very likely have a much more damaging impact than it did in the 19th century potentially causing widespread power outages along with disruptions to navigation, air travel, banking, and all forms of digital communication.

Discussion

The sun has been quite active this year as Solar Cycle 25 progresses towards a solar maximum which is anticipated to take place in late 2024 or early 2025. In fact, there has not been a single day in 2023 without sunspots which can be compared and contrasted to 281 such days in 2019…the time of the last solar minimum. Solar Cycle 25 has turned out to be stronger with more sunspot activity than its predecessor, Solar Cycle 24, which featured the fewest number of sunspots since Solar Cycle 14 peaked in February 1906. Even weak solar cycles, however, can produce significant solar storms. In fact, the “Carrington Event” of 1859 took place during a weak solar cycle (#10).
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Drawings of the Carrington sunspot by Richard Carrington on Sept. 1, 1859, and (inset) Heinrich Schwabe on Aug. 27, 1859. [Ref]

The solar storm of September 1, 1859

Coming just a few months before the solar maximum of 1860, numerous sunspots began to appear on the sun's surface on 28 August 1859 and were being observed in different parts of the world. Just before noon on the cloudless morning of Thursday, September 1, 1859, 33-year-old astronomer Richard Carrington - widely acknowledged at the time to be England’s best - was in his own private observatory and, as he usually did on sunny days, he used his telescope to project an 11-inch wide image of the sun on a screen and carefully drew the sunspots that he saw. Suddenly, two brilliant beads of blinding white light appeared over the sunspots, intensified rapidly, and became kidney-shaped. He realized that he was witnessing something unprecedented and left for about one minute to find another witness. On returning within 60 seconds, he and his witness found that much had already subsided in that short time.
Picture3.jpg

Circled areas on plot indicate locations that experienced the northern lights (auroras) during the “Carrington Event” of 1859

The next morning, Friday, September 2nd, 1859, when the CME arrived, it crashed into Earth's magnetic field, causing the global bubble of magnetism that surrounds our planet to shake and quiver. The CME reached the Earth some 17.6 hours after the eruption which is much quicker than the normal journey time of 3 or 4 days as an earlier CME actually cleared the way of the ambient solar plasma for the second blast to move so quickly. Rapidly moving fields induced enormous electric currents that surged through telegraph lines and disrupted communications. In fact, telegraph systems all over Europe and North America went haywire and, in some cases, telegraph operators were literally shocked as sparks were flying and telegraph paper was often set on fire. Some systems actually continued to work despite being disconnected from their power supplies as aurora-induced electric currents still allowed messages to be transmitted. Skies all over Earth erupted in red, green and purple auroras - even in tropical locations like Cuba, Jamaica, El Salvador, the Bahamas and Hawaii. The auroras were so bright over the Rocky Mountains that their glow awoke gold miners who began preparing breakfast because they thought it was morning. People in the northeastern US could read a newspaper by the aurora’s light.
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31 Aug 1859, 1 – The Cadiz Sentinel at Newspapers.com

On Saturday, September 3, 1859, the Baltimore American and Commercial Advertiser reported, "Those who happened to be out late on Thursday night had an opportunity of witnessing another magnificent display of the auroral lights. The phenomenon was very similar to the display on Sunday night, though at times the light was, if possible, more brilliant, and the prismatic hues more varied and gorgeous. The light appeared to cover the whole firmament, apparently like a luminous cloud, through which the stars of the larger magnitude indistinctly shone. The light was greater than that of the moon at its full, but had an indescribable softness and delicacy that seemed to envelop everything upon which it rested. Between 12 and 1 o'clock, when the display was at its full brilliancy, the quiet streets of the city resting under this strange light, presented a beautiful as well as singular appearance.”
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Sunspot drawings by German astronomer Heinrich Schwabe on 27 August 1859 (left), 1 September 1859 (center), and close‐up figure of 1 September 1859 (right), reproduced from RAS MS Schwabe 31 (p. 131 and p. 136; Image courtesy of the Royal Astronomical Society, Hayakawa et al. Circles in the upper halves correspond to the solar disk, on which the sunspots are drawn with the numbers.

Back in the 19th century there were no X-ray satellites or radio telescopes and no one knew solar flares existed until that September morning. "What Carrington saw was a white-light solar flare—a magnetic explosion on the sun," explains David Hathaway, solar physics team lead at NASA's Marshall Space Flight Center in Huntsville, Alabama. "It's rare that one can actually see the brightening of the solar surface," says Hathaway. "It takes a lot of energy to heat up the surface of the sun!" The explosion witnessed by Carrington produced not only a surge of visible light, but also a mammoth cloud of charged particles and detached magnetic loops—a "CME"—and hurled that cloud directly toward Earth.

“Carrington Event” - not as rare as once thought

Most experts today regard the “Carrington Event” of 1859 as one of the most powerful geomagnetic storms in recorded history. However, new findings suggest that it may be something that occurs more frequently than previously thought and perhaps more of an imminent threat to modern society. A good example is the great storm of mid-September 1770, when extremely bright red auroras blanketed Japan and parts of China. Captain Cook himself saw the display from near Timor Island, south of Indonesia. Hayakawa and colleagues recently found drawings of the instigating sunspot, and it is twice the size of the Carrington sunspot group — paintings, dairy entries, and other newfound records, especially from China, depict some of the lowest-latitude auroras ever, spread over a period of 9 days. “We conclude that the 1770 magnetic storm was comparable to the Carrington Event, at least in terms of auroral visibility,” wrote Hayakawa and colleagues in a 2017 Astrophysical Journal Letter. Moreover, “the duration of the storm activity was much longer than usual.”
Picture6.jpg

An eyewitness sketch of red auroras over Japan in mid-September 1770. [Ref]

Hayakawa’s team has delved into the history of other storms as well, examining Japanese diaries, Chinese and Korean government records, archives of the Russian Central Observatory, and logbooks from ships at sea–all helping to form a more complete picture of events. They found that superstorms in Feb 1872 and May 1921 were also comparable to the “Carrington Event”, with similar magnetic amplitudes and widespread auroras.
Picture7.jpg

Oriental reports of a giant naked-eye sunspot group (left) and auroras (right) in Feb. 1872. [Ref]

Impact of a “Carrington-type” event on today’s world

Today we know that solar flares happen frequently, especially during solar sunspot maximums. In today’s world, electronic technologies have become embedded into everyday life and are, of course, quite vulnerable to solar activity. Power lines, long-distance telephone cables, radar, cell phones, GPS, and satellites – all could be significantly affected by an event like this one. In other words, the world’s high-tech infrastructure could grind to a halt disrupting daily activities from purchasing a gallon gas to using the Internet.
Of particular concern is the fear about what this kind of solar storm could do to the electrical grid since power surges caused by solar particles can blow out giant transformers. If numerous transformers happened to be destroyed at once, it would likely take a painfully long time to replace them. The eastern US is especially vulnerable since the power infrastructure is highly interconnected so that failures in one location could cause failures in other regions. One long-term solution to this vulnerability would be to rebuild the aging power grid to be less susceptible to solar disruptions.

Final thoughts

On the positive side, there is comfort in the fact that observations of the sun in today’s world are a constant with a fleet of spacecraft in position to monitor the sun and gather data on solar flares. Also, there is better forecasting today and solar scientists could give some sort of warning as to when solar flares might appear and whether a given storm is pointed at Earth. Improved forecasting can allow for mitigating actions to be taken since the most damaging emissions travel slowly enough to be detected by satellites well before the particles strike the Earth. For example, power companies could protect valuable transformers by taking them offline before a solar storm strikes. One thing is certain, we should be prepared for another massive solar storm of the magnitude of the “Carrington Event” of 1859 as new information suggests these have likely been occurring much more often than previously thought.
Meteorologist Paul Dorian
Arcfield
arcfieldweather.com

Discussion A Tasty Solar Storm Sandwich Arrives | Informal Forecast Briefing 4 November 2023
Streamed live on Nov 5, 2023
 
SOLAR CYCLE 25 ACTIVITY REPORT NOVEMBER 07_2023

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C9 event observed at 2134 UTC from Region 3480 (S09E40).

There are currently 8 sunspot regions on the solar disk: AR3477, AR3478 AR3479, AR3480, AR3482
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AR3472 & AR3481 are gone, AR3474 will be gone in a few hours.

Total number of sunspots has decreased to 67 (16 of these are grouped into 8 active regions) NOAA forecasts for the next 24h: 80% chance for C flares, 20% chance M flares and 5% chance for X flares.

AR3480 (S08E25) has developed a beta-gamma magnetic field that harbors energy for M-class flares​

● Auroral Activity

The geomagnetic field has been at unsettled to major storm levels levels for the past 24 hours. On November 06 Moderate G2 geomagnetic storm (Kp6) threshold reached at 05:59 UTC. Minor G1 geomagnetic storm (Kp5) threshold reached at 08:33 UTC Solar wind speed reached a peak of 611 km/s at 15:49 UTC Total IMF reached 24 nT at 22:33 UTC​
GEOMAGNETIC STORM WATCH (G2): NOAA forcasters say there is a chance of G2-class geomagnetic storms today, Nov. 7th, when the subsiding effects of Sunday's CME might overlap with an incoming solar wind stream. Earth's magnetosphere is already humming with G1-class activity, and it won't take much to push it across the threshold to G2​
Aurora Oval Bz: -4.79 nT South
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● Current Conditions at 05:00 UTC on November 07

▪︎ Minor G1 Geomagnetic storm (kp 5)
▪︎ Solar wind speed record: 487 km/sec (Moderately high speed)
▪︎ density: 5.97 p/cm³ (low density)
▪︎ Interplanetary Magnetic Field (IMF)
Bt: 4.62 nT
▪︎ Thermosphere Climate Index
today: 19.42x1010 W Warm
▪︎ Neutron Counts today: - 4.4 % (Low)
▪︎ X-ray Solar Flare: C1 0025 UT Nov07
▪︎ Sunspot number: 67 (SN 81 November 06)
▪︎ Spotless Days 2023 total: 0 days (0%)
▪︎ Solar wind flowing from a coronal hole should reach Earth on Nov. 8th.
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SOLAR CYCLE 25 ACTIVITY REPORT NOVEMBER 08_2023

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C2 event observed at 16:13 UTC from Region 3479 (N23W58)

There are currently 5 sunspot regions on the solar disk: AR3477, AR3479, AR3480, AR3482 and new region AR3483
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AR3478 is gone

Total number of sunspots has increased to 74 (24 of these are grouped into 5 active regions) NOAA forecasts for the next 24h: 80% chance for C flares, 15% chance M flares and 1% chance for X flares. All regions have stable magnetic fields​

● Auroral Activity

The geomagnetic field has been at quiet to minor storm levels for the past 24 hours. On November 07 Solar wind speed reached a peak of 664 km/s at 20:34 UTC Total IMF reached 8 nT at 22:33 UTC​

GEOMAGNETIC STORM WATCH (G1): Minor G1-class geomagnetic storms are possible on Nov. 8th and 9th when Earth enters a stream of fast-moving solar wind. The gaseous material is flowing from a southern hole in the sun's atmosphere. High-latitude sky watchers should be alert for auroras. SpaceWeather.com​

Aurora Oval Bz: 5.63 nT North
aurora-map.jpg
EARTH'S RING CURRENT JUST SPRANG A LEAK: During this past weekend's strong G3-class geomagnetic storm, low-latitude auroras spread as far south as Texas and Arizona. Upon further review, most of those lights were not auroras at all. Everything red in this montage is an "SAR arc":​

Credits: Texas (Anita Oakley); Missouri (Dan Bush); New York (James Perez-Rogers); Arizona (Jeremy Perez)​

"This was a new phenomenon to me," says Jeremy Perez, who took the Arizona picture. "I had never heard of SARs before, but I kept shooting anyway."​
SAR arcs were discovered in 1956 at the beginning of the Space Age. Researchers didn't know what they were and unwittingly gave them a misleading name: "Stable Auroral Red arcs" or SAR arcs. In fact, SAR arcs are neither stable nor auroras.
Auroras appear when charged particles rain down from space, hitting the atmosphere and causing it to glow. SAR arcs form differently. They are a sign of heat energy leaking into the upper atmosphere from Earth's ring current system–a donut-shaped circuit carrying millions of amps around our planet.​

An artist's concept of Earth's ring current, quiet (left) and active (right) [more]​

"On Nov. 5th, the ring current was pumped up by hours of strong geomagnetic storming, with energy dissipating into these SAR arcs," says Jeff Baumgardner of Boston University's Center for Space Physics. "It was a global event. Our cameras registered SAR arc activity from Italy to New Zealand."
Recent research has linked SAR arcs to another phenomenon that is not an aurora: STEVE. The mauve ribbon in the sky was not originally thought to have anything to do with Earth's ring current. Yet in 2015, observers in New Zealand caught a bright red SAR arc transforming itself into STEVE like a caterpillar into a butterfly.​
On Nov. 5th, Mark Savage may have witnessed the same metamorphosis over Northumberland, UK:​
Visible to the naked eye, STEVE materialized from an overhanging red arc. "The entire process took about 10 minutes," says Savage. This timescale roughly matches that of another SAR-to-STEVE transition observed over Canada in April 2022. Clearly, the two phenomena are linked, but researchers aren't sure how.
"The connection is still elusive," says Carlos Martinis, a leading researcher in the field at Boston University. "Sometimes SAR arcs evolve into STEVE--but not always. This is a very active field of research, involving citizen scientists and researchers." SpaceWeather.com​

● Current Conditions at 04:45 UTC on November 08

▪︎ Active geomagnetic conditions (Kp4)
Threshold Reached ar 04:22 UTC
▪︎ Solar wind speed record: 467 km/sec (Elevated speed)
▪︎ density: 6.52 p/cm³ (low density)
▪︎ Interplanetary Magnetic Field (IMF)
Bt: 6.28 nT
▪︎ Thermosphere Climate Index
today: 20.40x1010 W Warm
▪︎ Neutron Counts today: - 5.9 % (Low)
▪︎ X-ray Solar Flare: C4 0309 UT Nov08
▪︎ Sunspot number: 74 (SN 67 November 07)
▪︎ Spotless Days 2023 total: 0 days (0%)
▪︎ Solar wind flowing from a coronal hole should reach Earth on Nov. 8th or 9th
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SOLAR CYCLE 25 ACTIVITY REPORT NOVEMBER 09_2023

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C6 event observed at 08:48 UTC from Region 3483 (N09W09)

There are currently 6 sunspot regions on the solar disk: AR3477, AR3479, AR3480, AR3482 AR3483 and new region AR3484
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Total number of sunspots has increased to 92 (32 of these are grouped into 6 active regions) NOAA forecasts for the next 24h: 80% chance for C flares, 10% chance M flares and 1% chance for X flares.

AR3483 (N10W08) has a 'beta-gamma' magnetic field that harbors energy for M-class solar flares.​

● Auroral Activity

The geomagnetic field has been at quiet to active levels for the past 24 hours. On November 08 Solar wind speed reached a peak of 780 km/s (High speed) at 19:43 UTC Total IMF reached 8 nT at 21:15 UTC​

GEOMAGNETIC STORM WATCH--CANCELED: As expected, Earth has entered a stream of fast-moving solar wind. However, it is doing little to disturb our planet's magnetic field. Geomagnetic storms are unlikely on Nov. 9th. SpaceWeather.com​

Aurora Oval Bz: 0.02 nT North
aurora-map (1).jpg
● Current Conditions at 03:50 UTC on November 09

▪︎ Geospace unsettled (Kp3)
▪︎ Solar wind speed record: 478 km/sec (Elevated speed)
▪︎ density: 3.88 p/cm³ (low density)
▪︎ Interplanetary Magnetic Field (IMF)
Bt: 3.91 nT
▪︎ Thermosphere Climate Index
today: 20.47x1010 W Warm
▪︎ Neutron Counts today: - 5.4 % (Low)
▪︎ X-ray Solar Flare: C1 0119 UT Nov09
▪︎ Sunspot number: 92 (SN 74 November 08)
▪︎ Spotless Days 2023 total: 0 days (0%)
▪︎ There are no significant coronal holes on the Earthside of the sun
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Spaceweather.com.
GEOMAGNETIC STORM WATCH--CANCELED:
As expected, Earth has entered a stream of fast-moving solar wind. However, it is doing little to disturb our planet's magnetic field. Geomagnetic storms are unlikely on Nov. 9th. Aurora alerts: SMS Text

The Watchers —
Screenshot 2023-11-09 at 15-35-25 SWX - Space Weather Monitor.png

Professor Peter Becker is working with a team whose goal is to create an early warning system for dangerous solar activity that could damage critical technology.
We may marvel at the Northern Lights, but that same solar storm energy could one day create what one researcher described as an "internet apocalypse."

"The internet has come of age during a time when the sun has been relatively quiet, and now it's entering a more active time," said Professor Peter Becker of George Mason University. "It's the first time in human history that there's been an intersection of increased solar activity with our dependence on the internet and our global economic dependence on the internet."

Becker is the lead investigator on a project with the school and the Naval Research Laboratory to create an early warning system.

NORTHERN LIGHTS ACTIVITY TO INCREASE, INCLUDE AURORAS FURTHER SOUTH DUE TO INCREASING SUN ACTIVITY

Screenshot 2023-11-09 at 15-00-19 Solar superstorm could 'wipe out the internet' for weeks or ...png

What can a solar super storm do to Earth?

"There have been a lot of (solar) flares," Becker said. "Flares are when the sun brightens, and we see the radiation, and that's kind of the muzzle flash. And then the cannon shot is the coronal mass ejection (CME). So, we can see the flash, but then the coronal mass ejection can go off in some random direction in space, but we can tell when they're actually going to head towards Earth. And that gives us about 18 hours of warning, maybe 24 hours of warning, before those particles actually get to Earth and start messing with Earth's magnetic field."

Large blobs of plasma, or superheated matter, fly through space in a CME. A percentage hit the Earth, which distorts our planet's magnetic field. That third prong on the electric plug, which usually gives excess electrical charges a safe place to go, becomes "like a big electrical circuit."

Screenshot 2023-11-09 at 15-01-56 Solar superstorm could 'wipe out the internet' for weeks or ...png

"And then you get this kind of insidious thing where you could actually get current from ground," Becker said. "So everybody thinks, 'Oh, my computer's grounded, I'm okay,'" but in an event like this, if you drive inductive currents to the surface of the Earth, it can almost work backwards, and you can end up actually frying things that you thought were relatively safe."

The power grid, satellites, underground fiber optic cable with copper sheaths, navigation and GPS systems, radio transmitters and communications equipment are all vulnerable.

This has happened before

It has happened before. Becker points to the Carrington Event in 1859. That was the last time a CME reached Earth.

THE DAY THE NORTHERN LIGHTS COVERED THE PLANET: HISTORY OF EARTH'S GREATEST SOLAR STORMS

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Thermal image of an eruption or flare on the surface of the Sun. Solar flares are giant explosions on the Sun that send energy, light and high speed particles into space.
(Heritage Space/Heritage Images)


"It actually took out the telegraph system, sparks were literally flying off the telegraph lines," Becker said. "Some operators got electrocuted because the wires ended up carrying high voltage, which they were never supposed to do, but the magnetic field variations became so strong it almost became a generator system and drove these currents down telegraph wires."

The heavy-duty wires of the telegraph were robust compared to the fragile electronics of today, he said.

"So you lay that on top of the internet with its very delicate electronics, you're talking about something that could really fry the system for a period of several weeks to months in terms of the time it would take to repair all the infrastructure – all of the electronic switches, all of these closets of electronics in all these office buildings," Becker said. "That could all be fried. So we're talking pretty major. And it's not just communications. It's economic disruption, too, obviously."

An economic disruption to the tune of $10-$20 billion per day to the U.S. economy alone, Becker estimated.

The solar cycle is peaking making solar storms more plentiful

Tree rings and ice cores are evidence of much larger superstorms in the past. About 14,000 years ago, a solar flare, possibly hundreds of times stronger than the Carrington flare, impacted Earth.

NOAA forecast the current solar cycle to ramp up and peak in 2024.


NOAA PREDICTS STRONGER PEAK OF SOLAR ACTIVITY IN 2024 THAN ORIGINALLY ANTICIPATED

Becker said predicting solar storms is like predicting earthquakes – we just don't have control over the situation. He said that the odds are about 10% that over the next decade, "something really large is going to happen that could potentially wipe out the internet."

How can we protect electronics?

So he and his team are watching the sun and modeling flares. Flares, he said, reach Earth in 8 minutes. That sets the clock ticking for the possible magnetic field disruption in 18 to 24 hours.

"If we have a warning, every minute counts because you can put satellites in safe mode. You can take transformers off-line from the grid, so they don't fry," Becker said. "So there's things you can do to mitigate the problem. And then, more long term, you're talking about hardening the internet. And that's, of course, an economic challenge because it's sort of like an insurance policy. You may never need it, and it would cost trillions to really harden the system."

He said most large corporations don't have the economic incentive to harden their system at this point.




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NOTICE This morning shortly after midnight a new M5.0 earthquake occurred in #Reykjanes #Islandia the strongest since the seismic swarms began on October 25. Its epicenter was near the Blue Lagoon and it has been closed for a week due to the possibility of a volcanic eruption.#Iceland #volcano #BlueLagoon
 
SOLAR CYCLE 25 ACTIVITY REPORT NOVEMBER 10_2023

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C2 event observed at 11:18 UTC on November 09

There are currently 6 sunspot regions on the solar disk: AR3477, AR3479, AR3480, AR3481
AR3482 AR3483
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Total number of sunspots has increased to 93 (32 of these are grouped into 6 active regions) NOAA forecasts for the next 24h: 80% chance for C flares, 15% chance M flares and 1% chance for X flares. All regions have stable magnetic fields.

● Auroral Activity

The geomagnetic field has been at quiet to unsettled levels for the past 24 hours. On November 09 Solar wind speed reached a peak of 637 km/s at 13:49 UTC. Total IMF reached 5 nT at 21:08 UTC
EARTH-DIRECTED CME (UPDATED): Today, coronagraphs onboard the Solar and Heliospheric Observatory (SOHO) detected a halo CME leaving the sun. It is heading straight for Earth. NOAA and NASA models agree that the CME should arrive during the late hours of Nov. 11th (UT), bringing a chance of G2-class geomagnetic storms. SpaceWeather.com
Aurora Oval Bz: 0.85 nT North
aurora-map.jpg
● Current Conditions at 04:10 UTC on November 10

▪︎ Geospace quiet (Kp2)
▪︎ Solar wind speed record: 490.2 km/sec (Elevated speed)
▪︎ density: 6.47 p/cm³ (low density)
▪︎ Interplanetary Magnetic Field (IMF)
Bt: 2.74 nT
▪︎ Thermosphere Climate Index
today: 20.52x1010 W Warm
▪︎ Neutron Counts today: - 5.3 % (Low)
▪︎ X-ray Solar Flare: C1 0221 UT Nov10
▪︎ Sunspot number: 93 (SN 92 November 09)
▪︎ Spotless Days 2023 total: 0 days (0%)
▪︎ There are no significant coronal holes on the Earthside of the sun
.......
SpaceWeatherlive.com
SpaceWeather.com
EarthSky.org
 
EARTH-DIRECTED CME (UPDATED): Today, coronagraphs onboard the Solar and Heliospheric Observatory (SOHO) detected a halo CME leaving the sun. It is heading straight for Earth. NOAA and NASA models agree that the CME should arrive during the late hours of Nov. 11th (UT), bringing a chance of G2-class geomagnetic storms. SpaceWeather.com

According to Nasa model, we're in for a direct hit...

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SOLAR CYCLE 25 ACTIVITY REPORT NOVEMBER 11_2023

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C3 event observed at 16:04 UTC on November 10 from Region 3477 (S15W53).

There are currently 7 sunspot regions on the solar disk: AR3477, AR3480, AR3481, AR3482 AR3483 and new regions AR3484, AR3485
hmi200.gif
AR3479 is gone

No change in the total number of sunspots 93 (34 of these are grouped into 7 active regions) NOAA forecasts for the next 24h: 80% chance for C flares, 15% chance M flares and 1% chance for X flares. All regions have stable magnetic fields.

● Auroral Activity

The geomagnetic field has been at quiet to active levels for the past 24 hours. On November 10 Solar wind speed reached a peak of 697 km/s at 05:38 UTC.


Aurora Oval Bz: -0.16 nT South
aurora-map.jpg

● Current Conditions at 05:10 UTC on November 11

▪︎ Geospace quiet (Kp2)
▪︎ Solar wind speed record: 532 km/sec (Moderately high speed)
▪︎ density: 1.07 p/cm³ (low density)
▪︎ Interplanetary Magnetic Field (IMF)
Bt: 2.16 nT
▪︎ Thermosphere Climate Index
today: 20.55x1010 W Warm
▪︎ Neutron Counts today: - 4.9 % (Low)
▪︎ X-ray Solar Flare: C7 0359 UT Nov11
▪︎ Sunspot number: 93 (SN 93 November 10)
▪︎ Spotless Days 2023 total: 0 days (0%)
▪︎ There are no significant coronal holes on the Earthside of the sun
.......
SpaceWeatherlive.com
SpaceWeather.com
EarthSky.org
 
SOLAR CYCLE 25 ACTIVITY REPORT NOVEMBER 12_2023

Solar activity has been at moderate levels for the past 24 hours. The largest solar event of the period was a M1 event observed at 17:29 UTC on November 11 from Region 3477 (S15W67) The flare caused a Minor R1 radio blackout over South America
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There are currently 6 sunspot regions on the solar disk: AR3477, AR3480, AR3481,AR3483, AR3484, AR3485
hmi200.gif
AR3482 is gone

Total number of sunspots has decreased to 85 (37 of these are grouped into 6 active regions) NOAA forecasts for the next 24h: 95% chance for C flares, 30% chance M flares and 5% chance for X flares.

AR3483 has developed a beta-gamma magnetic field that harbors energy for M-class flares

● Auroral Activity

The geomagnetic field has been at quiet to active levels for the past 24 hours. On November 11 Solar wind speed reached a peak of 591 km/s at 21:16 UTC.​

Aurora Oval Bz: -1.25 nT South
aurora-map.jpg
● Current Conditions at 03:30 UTC on November 12

▪︎ Geospace quiet (Kp1)
▪︎ Solar wind speed record: 463 km/sec (Elevated speed)
▪︎ density: 3.49 p/cm³ (low density)
▪︎ Interplanetary Magnetic Field (IMF)
Bt: 1.77 nT
▪︎ Thermosphere Climate Index
today: 20.55x1010 W Warm
▪︎ Neutron Counts today: - 4.9 % (Low)
▪︎ X-ray Solar Flare: C1 2120 UT Nov11
▪︎ Sunspot number: 85 (SN 93 November 11)
▪︎ Spotless Days 2023 total: 0 days (0%)
▪︎ There are no significant coronal holes on the Earthside of the sun
.......
SpaceWeatherlive.com
SpaceWeather.com
EarthSky.org
 
SOLAR CYCLE ACTIVITY REPORT NOVEMBER 13_2023

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C8 event observed at 04:41 UTC from Region 3484 (S15W60) on November 12.

There are currently 6 sunspot regions on the solar disk: AR3477,AR3481,AR3483, AR3484
AR3485 and new region AR3486
hmi200.jpg
AR3480 is gone

Total number of sunspots has decreased to 78 (29 of these are grouped into 6 active regions) NOAA forecasts for the next 24h: 99% chance for C flares, 45% chance M flares and 5% chance for X flares.

AR3483 has a beta-gamma magnetic field that harbors energy for M-class flares

● Auroral Activity

The geomagnetic field has been at quiet to active levels for the past 24 hours. On November 12 Solar wind speed reached a peak of 585 km/s at 07:37 UTC. Total IMF reached 10 nT at 2030 UTC​


Aurora Oval Bz: 2.33 nT North
aurora-map.jpg

● Current Conditions at 04:00 UTC on November 13

▪︎ Minor G1Geomagnetic storm in progress (Kp5) Threshold Reached: 01:23 UTC
▪︎ Solar wind speed record: 421.7 km/sec (Elevated speed)
▪︎ density: 21 p/cm³ (Moderate density)
▪︎ Interplanetary Magnetic Field (IMF)
Bt: 11 nT
▪︎ Thermosphere Climate Index
today: 20.34x1010 W Warm
▪︎ Neutron Counts today: - 4.9 % (Low)
▪︎ X-ray Solar Flare: C2 0146 UT Nov13
▪︎ Sunspot number: 78 (SN 85 November 12)
▪︎ Spotless Days 2023 total: 0 days (0%)
▪︎ There are no significant coronal holes on the Earthside of the sun
.......
SpaceWeatherlive.com
SpaceWeather.com
EarthSky.org
 
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