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Is anyone concerned about this? (low latitude aurora)


kota
Go to solution Solved by Sam Warfel,

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Low latitude aurora was observed in the following years (to 1859) 

- 1859 (Carrington Event)

- 1882 (Feb. 4th) 

- 1903 (Oct. 31st Halloween Storm Kp9)

- 1921 (May 14th Kp8, 13 degrees)

- 1972 (Aug. 4-7, Kp9)

 

 

- 1998 (Nov. 6-10, Kp7)

- 1991 (Jun. 4-6, Kp8)

- 2003 (Oct. 28-30 Halloween Storms Kp9)

- 2001 (Mar. 24, kp7)

 

I made the indention here because all of a sudden we are seeing a ramp up in these storms reaching low latitude levels. Just this year, we had 5 low latitude aurora observations with only a small number of these events resulting from x class events. 

This isn't normal to me, is it normal to ya'll? Is this something to be concerned about with this uptick in low latitude observations?  Thanks. 

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3 minuten geleden, kota zei:

Just this year, we had 5 low latitude aurora observations

None resulted in a Kp9/G5 storm like the other examples you’ve mentioned… 

the 5 times in 2023 where mostly in middle latitude locations with only once on low latitude locations and only photographic not visually.

all of this is nothing unusual and normal in the years around solar max. If you compare it with SC23 it’s very normal. 

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Posted (edited)
9 minutes ago, kota said:

1998 (Nov. 6-10, Kp7)

9 minutes ago, kota said:

2001 (Mar. 24, kp7)

KP7? Hardly worth noting. Happens all the time during the maximum of the Sun’s 11 year cycle. Just this spring we had two KP8s. 

9 minutes ago, kota said:

Just this year, we had 5 low latitude aurora observations with only a small number of these events resulting from x class events. 

That’s cause we are approaching the peak of the sun’s 11-year activity cycle, likely in 2024. So the increased activity is perfectly normal, and happens every 11 years. Nothing surprising. 

9 minutes ago, kota said:

This isn't normal to me, is it normal to ya'll? Is this something to be concerned about with this uptick in low latitude observations?  Thanks. 

So yes, it’s normal. And no, it’s not something to be concerned about. We’ll see more of this strong activity as we pass max, maybe even a G5 (KP9) event. Hopefully some lovey aurora! And our power grids and satellites will weather it just fine, as they were designed to do and have done in the past. 

Edited by Sam Warfel
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Douglass Adams line "we demand well defined areas of doubt and uncertainty" blended with "I much rather be Happy than right" definitely apply. Our reality will only become apparent when we have full understanding of human purpose. It is doubful if even then we can. Enjoy the wonders along the way to enlightenment.

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Well, this is a bit subjective, just like the KP-index in general. Low latitude is just a rough and short description to inform about a possible aurora to reach Mediterranean Sea, Mexico or Japan. Take Budapest for example, the SWL site suggests KP 9+ is required, but what does that exactly mean, what should be visible?

  • It's only photographic in Budapest? Recent aurorae shown that K7 is enough.
  • It's visible to naked eye in Budapest? April 2023 (G4) and November 2023 (G3) are examples.
  • The pillars can reach zenith in Budapest? I agree, somewhat KP 9+ is required.

Time's changing, technology gets better and there's greater awareness of aurora coming on mid and low latitude skies. We simply don't skip any chance today, hundreds of chasers are ready in my country (Poland) when it's just G1, because K4 is often enough while official maps suggest KP 6-8 is for Poland. But 20 years ago it was all about luck and rare knowledge that ACE exists to monitor Bz or wind speed indicators. Nobody monitored, because people didn't know and didn't have good cameras as we have today.

Here are all dates when Bz level reached at least once -30 or below, in a DD/MM/YYYY format. Basically in all these cases a photographic aurora was present what truly means "low latitude". As I remember in nearly all cases Bz was low long enough to trigger aurora getting further south. This is just a brief list where to start searching for best views in last 26 years in ACE/DSCOVR data. Roughtly, -30 is photographic, -40 is visible to naked eye, -50 is overhead.

4/5/1998 (-37.03)
22/10/1999 (-31.49)
6/4/2000 (-32.76)
24/5/2000 (-30.70)
15/7/2000 (-59.27)
17/9/2000 (-35.34)
31/3/2001 (-46.86)
11/4/2001 (-36.61)
6/11/2001 (-78.17)
24/11/2001 (-49.29)
17/4/2002 (-31.18)
23/5/2002 (-41.37)
29/5/2003 (-33.32)
26/7/2003 (-31.99)
29/10/2003 (-53.85)
30/10/2003 (-35.50)
20/11/2003 (-52.80)
7/11/2004 (-50.19)
9/11/2004 (-32.81)
15/5/2005 (-45.89)
24/8/2005 (-55.55)
26/9/2011 (-31.01)
22/6/2015 (-39.42)
7/9/2017 (-32.99)
24/4/2023 (-33.32)

There have been a lot of such moments in SC23, but those weren't greatly monitored. Nowdays, Bz -30 seems extreme, but official G5 was counted only some cases that got -40 or deeper (!). That means, if you see Bz getting -25, you may think of G5 coming shortly, but G5 is still far from that. G4 is very stretched, as poor G4 (but not G3) may show aurora down to Hungary, but great G4 (but not G5) may reach Greece. KP 8- and KP 8+ only slightly helps, as KP isn't K index.

But it isn't generally stated if we talk about photographic or visual. When one says about G5, I talk about a photographic aurora that reaches northern Africa, not a visual aurora that reaches Rome. Individual stuff.

Usually, the Bz level reach KP levels based on list below:

  • K4 = -8 to -10 (official counts may be KP3-G1)
  • K5 = -10 to -15 (official counts may be KP4-G2)
  • K6 = -15 to -20 (official counts may be G1-G3)
  • K7 = -20 to -25 (official counts may be G2-G4)
  • K8 = -25 to -40 (official count may be G3; KP9 is less expected)
  • K9 = -40 and lower (SWL archive shown that official count may be G4 if Bz doesn't reach -50)

Interesting fact is, you mentioned about March 2001 that isn't in list above. I think that date was incorrect, because Bz didn't reach -10 or below at all.

I'm hoping for a repetition of Bz -40 for aurora to see if modern cameras can catch in Canary Islands, what I expect from archive data. Not even -50, but I give chances for -40.

What's the conclusion? To see if a low latitude aurora could be present, seek for indicators rather than official KP values. This what you listed are just best displays of aurora that are visually seen above your head in latitudes not like Paris or Vienna, but rather Rome or Bucharest. All dates above should give a good start. If SC25 becomes active as SC23, you may have several low latitude aurora in year.

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13 hours ago, Sam Warfel said:

KP7? Hardly worth noting. Happens all the time during the maximum of the Sun’s 11 year cycle. Just this spring we had two KP8s. 

That’s cause we are approaching the peak of the sun’s 11-year activity cycle, likely in 2024. So the increased activity is perfectly normal, and happens every 11 years. Nothing surprising. 

So yes, it’s normal. And no, it’s not something to be concerned about. We’ll see more of this strong activity as we pass max, maybe even a G5 (KP9) event. Hopefully some lovey aurora! And our power grids and satellites will weather it just fine, as they were designed to do and have done in the past. 

Thanks for that clarification. I'm coming from the Suspicious Observer's community and the author brought up that point. I am curious though, what are your thoughts on our magnetosphere weakening? Ben Davidson brings up the point that as we see a weakening, these solar event's impact on the earth will be leveraged arguing that these 5 LLO events just this year are the result of weaker magnetosphere allowing our global energy grid to become imperiled. Does this sound accurate? I apologize for my lack of understanding in geophysics. 

36 minutes ago, libmar96 said:

Well, this is a bit subjective, just like the KP-index in general. Low latitude is just a rough and short description to inform about a possible aurora to reach Mediterranean Sea, Mexico or Japan. Take Budapest for example, the SWL site suggests KP 9+ is required, but what does that exactly mean, what should be visible?

  • It's only photographic in Budapest? Recent aurorae shown that K7 is enough.
  • It's visible to naked eye in Budapest? April 2023 (G4) and November 2023 (G3) are examples.
  • The pillars can reach zenith in Budapest? I agree, somewhat KP 9+ is required.

Time's changing, technology gets better and there's greater awareness of aurora coming on mid and low latitude skies. We simply don't skip any chance today, hundreds of chasers are ready in my country (Poland) when it's just G1, because K4 is often enough while official maps suggest KP 6-8 is for Poland. But 20 years ago it was all about luck and rare knowledge that ACE exists to monitor Bz or wind speed indicators. Nobody monitored, because people didn't know and didn't have good cameras as we have today.

Here are all dates when Bz level reached at least once -30 or below, in a DD/MM/YYYY format. Basically in all these cases a photographic aurora was present what truly means "low latitude". As I remember in nearly all cases Bz was low long enough to trigger aurora getting further south. This is just a brief list where to start searching for best views in last 26 years in ACE/DSCOVR data. Roughtly, -30 is photographic, -40 is visible to naked eye, -50 is overhead.

4/5/1998 (-37.03)
22/10/1999 (-31.49)
6/4/2000 (-32.76)
24/5/2000 (-30.70)
15/7/2000 (-59.27)
17/9/2000 (-35.34)
31/3/2001 (-46.86)
11/4/2001 (-36.61)
6/11/2001 (-78.17)
24/11/2001 (-49.29)
17/4/2002 (-31.18)
23/5/2002 (-41.37)
29/5/2003 (-33.32)
26/7/2003 (-31.99)
29/10/2003 (-53.85)
30/10/2003 (-35.50)
20/11/2003 (-52.80)
7/11/2004 (-50.19)
9/11/2004 (-32.81)
15/5/2005 (-45.89)
24/8/2005 (-55.55)
26/9/2011 (-31.01)
22/6/2015 (-39.42)
7/9/2017 (-32.99)
24/4/2023 (-33.32)

There have been a lot of such moments in SC23, but those weren't greatly monitored. Nowdays, Bz -30 seems extreme, but official G5 was counted only some cases that got -40 or deeper (!). That means, if you see Bz getting -25, you may think of G5 coming shortly, but G5 is still far from that. G4 is very stretched, as poor G4 (but not G3) may show aurora down to Hungary, but great G4 (but not G5) may reach Greece. KP 8- and KP 8+ only slightly helps, as KP isn't K index.

But it isn't generally stated if we talk about photographic or visual. When one says about G5, I talk about a photographic aurora that reaches northern Africa, not a visual aurora that reaches Rome. Individual stuff.

Usually, the Bz level reach KP levels based on list below:

  • K4 = -8 to -10 (official counts may be KP3-G1)
  • K5 = -10 to -15 (official counts may be KP4-G2)
  • K6 = -15 to -20 (official counts may be G1-G3)
  • K7 = -20 to -25 (official counts may be G2-G4)
  • K8 = -25 to -40 (official count may be G3; KP9 is less expected)
  • K9 = -40 and lower (SWL archive shown that official count may be G4 if Bz doesn't reach -50)

Interesting fact is, you mentioned about March 2001 that isn't in list above. I think that date was incorrect, because Bz didn't reach -10 or below at all.

I'm hoping for a repetition of Bz -40 for aurora to see if modern cameras can catch in Canary Islands, what I expect from archive data. Not even -50, but I give chances for -40.

What's the conclusion? To see if a low latitude aurora could be present, seek for indicators rather than official KP values. This what you listed are just best displays of aurora that are visually seen above your head in latitudes not like Paris or Vienna, but rather Rome or Bucharest. All dates above should give a good start. If SC25 becomes active as SC23, you may have several low latitude aurora in year.

Very fascinating information. Thank you for setting that foundation. Yes my data seems skewed. I sourced it from this (timestamp included): 

 

So it seems that i observed incorrect data - apologies for that. 

With that being said, is it more likely then not for us to have a stronger solar cycle for SC25 over SC23? I know it's hard to say either way, i mean even NOAA underestimated this new cycle - but what are your thoughts? 

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7 hours ago, tniickck said:

there is absolutely no reasons to be concerned about aurora until it harms power grids

Which is,  i think, very unlikely until we surpass even the strongest storm we had (lets say Directly hit by X100 flare and very very strong southwards IMF etc.) so worst worst case scenario. but i think the odds for that is unimaginable low so no needs to worry. our grids are mostly designed to withstand such events

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3 hours ago, libmar96 said:
  •  
  • K4 = -8 to -10 (official counts may be KP3-G1)
  • K5 = -10 to -15 (official counts may be KP4-G2)
  • K6 = -15 to -20 (official counts may be G1-G3)
  • K7 = -20 to -25 (official counts may be G2-G4)
  • K8 = -25 to -40 (official count may be G3; KP9 is less expected)
  • K9 = -40 and lower (SWL archive shown that official count may be G4 if Bz doesn't reach -50) 

it is not as easy as you think. solar wind speed plays a significant role in G5 storm. for example the aforementioned event on 6th Nov 2001 with bz reaching nearly -80 was only G4 because the solar wind speed was about 700-800 km/s which is not enough for G5 storm

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1 hour ago, tniickck said:

it is not as easy as you think. solar wind speed plays a significant role in G5 storm. for example the aforementioned event on 6th Nov 2001 with bz reaching nearly -80 was only G4 because the solar wind speed was about 700-800 km/s which is not enough for G5 storm

Thanks! That's a very important information in my search how to calculate K-index based on indicators instead of DST. I use wind speed to calculate as well, but I have no data "how good the aurora is" with speeds above 800 km/s, because there weren't any recently. Severe G4-G5 storms were just too long ago to say if 900 km/s and Bz -40 better than 1100 km/s and Bz -55 etc; there's insufficent data, so I gave it as a rough estimate.

Edited by libmar96
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