Aurora Australis 6 - Photoshots - the web folio of Tony Stewart.

Aurora Australis 6

Aurora Sat May 11th 2024 Lead Up

So a couple of days out, I thought these alerts are starting to ramp up, and could turn into something serious.

Until now I have to say I have been a bit disappointed with the lack of display, given we are headed right into the crest of the current solar cycle (#25).

I could see late in the week here was increased auroral activity forecast, which given solar phase and seasonal equinox, all sounded promising. Being on the winter side of daylight saving and quite dark early, I knew too that was good news. I could see that the sky was looking to clear, and weather was looking on side. Added to that, the moon phase was not at all bright. Woohoo!!

So in all, I was on standby and quietly hopeful for Thurs / Fri.

Fri night levels were actually pretty amazing and I thought if that was the entree, Sat was actually going to be a blinder. I actually made a Facebook post to friends, suggesting if anyone was interested, that Sat night could be worth a look. It isn’t often it is warm enough, and not too late, so if it doesn’t kick off, it doesn’t really matter.

It turns out that at its peak, last week’s geomagnetic storm reached the highest possible level on the G-scale (Extreme – G5), making this the first G5 storm since 2003.

Aurora Oval Graph

 

The CMEs that caused last week’s spectacular auroral displays originated from a cluster of sunspots designated Sunspot Region 3664, a region which also produced significant solar flares during the same period. At one point last week, this massive and complex sunspot cluster was about 17 times the diameter of Earth. It was like wave after wave of ejections and flares combined to make for a full earth bound punch.

According to NOAA’s Space Weather Prediction Center, a solar flare with a magnitude of X8.7 has since been detected from Sunspot Region 3664, at 1651 UTC on May 14. X-Class flares are the strongest of four categories and this X8.7 flare is stronger than anything measured last week. So as the sun turns away from Earth, this activity is likely to linger further. The question is, is the initial sunspot, and subsequent going to last long enough for a second blow as the rotation comes back round to face us in a few weeks/!

In fact, it’s the strongest solar flare detected in the current solar cycle, which begun in 2019 and is expected to peak next year.

It was enough for Transpower to suspend part of its power grid, knowing a similar event damage lines in Quebec in 1989. Though still comes short of what is regarded as the most severe solar event in modern history – the Carrington Event of 1859.

The current solar cycle is expected to peak in 2025 before declining over the next 5 to 7 years. Sunspot activity will remain elevated around the solar cycle’s peak, maintaining an elevated likelihood of aurora displays on Earth.

Solar cycle graph

 

Photo of solar activity in the sun

Image: The X8.7 solar flare – as seen in the bright flash on the right – on May 14, 2024. Credit: NASA/SDO

So I was actually very excited at the thought of a ‘big one’. I packed my kit, charged batteries, checked my torch(s), filled the car with fuel in eager anticipation. I set up at Tumbledown Bay, on Banks Peninsula. South facing views, right to the Southern Ocean, with foreground interest, away from city lights. I arrived early, knowing where I wanted to be, as well as keeping myself safe as the walk out on the cliff edge is a bit precarious! I set up in daylight and waited. Other people came after, and things slowly darkened after a stunning sun set.

As soon as it got dark enough to clear the sunset around 6.40pm, the aurora was on. It was there waiting doing its thing the whole time, the biggest and brightest I have ever seen. By actual darkness at 7pm, it was punching. Clearly visible with the naked eye, with pillars, waves and a overall glowing dome nearly 180degress West to East.

You can see here some of the app readings just before / after 9pm.

Aurora App reading May 11 Kp 8Aurora App reading May 11 Oval

Aurora App reading May 11 storm progress  Aurora App reading May 11 DensityAurora App reading May 11 Bz south  Aurora App reading May 11 Red kp Aurora App reading May 11 red Oval Aurora App reading May 11 2604 nT

Then again after 11pm

Aurora App reading May 11 Max Oval     Aurora App reading May 11 sightings Aurora App reading May 11 graphAurora App reading May 11 levels

But then at close to midnight we got a Kp9!

Aurora App reading May 11 kp 9

Aurora App reading May 11 density 9pmAurora App reading May 11 south 9pmAurora App reading May 11 storm

 

Reviewing the Data in Hindsight

Writing this nearly one week on, we have a bit more information.

From May 3 through May 9, 2024, NASA’s Solar Dynamics Observatory observed 82 notable solar flares. The flares came mainly from two active regions on the Sun called AR 13663 and AR 13664. This video highlights all flares classified at M5 or higher with nine categorized as X-class solar flares.

 

NASA’s Goddard Space Flight Center

 

Traveling at speeds up to 3 million mph, the CMEs bunched up in waves that reached Earth starting May 10, creating a long-lasting geomagnetic storm that reached a rating of G5 — the highest level on the geomagnetic storm scale, and one that hasn’t been seen since 2003.“The CMEs all arrived largely at once, and the conditions were just right to create a really historic storm,” said Elizabeth MacDonald, NASA heliophysics citizen science lead and a space scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

By one measure of geomagnetic storm strength, called the disturbance storm time index which dates back to 1957, this storm was similar to historic storms in 1958 and 2003. And with reports of auroras visible to as low as 26 degrees magnetic latitude, this recent storm may compete with some of the lowest-latitude aurora sightings on record over the past five centuries, though scientists are still assessing this ranking.

You can see the Magnetometer readings (note in UTC time, not NZDT).

Aurora app screenshot magnetometer

Also written in hindsight of the event, the week later, Benjamin Alldridge wrote on the Southern Hemisphere Aurora Group Facebook page

“Those of you who caught the majesty of the aurora: you have witnessed once in a century conditions. Last time we had this level of activity in one 24 hour period was early in the last century. In terms of absolute magnitude, we peaked at -412nT DST (essentially the level of “agitation” the magnetosphere has experienced), the greatest since the 1989 solar storms that took down the entire power grid of Quebec, which was on paper about 20% bigger but lasted for a shorter amount of time. We had confirmed captures in FNQ near Cairns, New Caledonia, and Florida – about 6,000km from the geomagnetic poles. People captured it in most major cities on the planet, and saw it clearly in many others. Even Africa and South America didn’t miss out, which is unprecedented in modern times”.

1989 vs 2024 aurora comparison

I have since read another post by Ian Cooper on the Aurora Australis NZ Facebook page, that I will post and credit fully here:

And now for something completely different! Some of you may be wondering how our recent “Great Geo-Magnetic Storm” compares to the past. There was an early comparison with the now famous “Carrington Event,” a massive storm in 1859. This comparison was based upon the size and shape of the giant sunspot group that caused the huge white flare and ensuing CME that brought about the Carrington Event, compared to the sunspot group that caused our recent show. There are better ways to compare such storms. Unfortunately, the data that we use doesn’t go back to 1859. That data is what we call the AA Index for ‘Auroral Activity.’ The AA Index is based upon the Planetary ‘K-Index.’ “A global 3-hr K Index was the first to provide an objective and quantitative monitoring of the irregular variations of the transient geomagnetic field observed in a given place. The use of K indices from a network of observatories to derive a planetary index of geomagnetic activity was suggested by Bartels when defining these indices. Other indices such as Kp were successively designed and accepted as International Association of Geomagnetism and Aeronomy indices.
The Table shows the 62 Greatest Auroral Storms between 1868 and 2024 based upon their K indices over the 3hr periods. I have only included the nighttime period for New Zealand rather than the complete days’ worth of data. The number for each 3 Hr period is the Global figure. This can be more or less than what is being recorded in N.Z. A good example of this is seen in one of my favourite storms, No. 54, the 31st of March 2001. In the period of 9hrs-12hrs for that night the reading was only 80, and yet that is when the first major “Break-up” occurred?
The storms are ranked by adding the 3hourly totals and dividing by 4 to get the Mean Maximum for the 12 hours. Some Great Storms should be included in the top ten just by what happened in one 3hr period. A good example of this is the famous storm from 103 years ago. On May 15th, 1921, there was a storm to rival the Carrington Event, but for N.Z. it only lasted for a few hours. From what I have been reading from eyewitness accounts the storm of 1921 was even greater than our recent one, but because it didn’t sustain over the whole night, the 1921 storm sits at No. 39. That same storm carried on at slightly lower levels on the next night, May 16th, 1921, but was far less impressive, yet because it held good numbers through the whole night it sits higher in the rankings at No. 28!
The graphic showing the Kp levels for the top 10 storms shows that our recent storm sitting at No. 7, is certainly not out of place, and would have easily been higher if activity had not dropped off in the last 3 hours before dawn. Stats are useful but don’t always tell the whole story, but it is a place to start. In many ways we don’t need the numbers to tell us how amazing it was, but it is still satisfying to have it quantified in some way. This information is up to date as of May 22nd 2024″.

Posted on 22/05/2024, Ian Cooper, Astronomer, Aurora Australis NZ Facebook page.

Solar storm history over time
Graph of solar storm history over time
Credit: