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AR 13229, X2.28 flare!


MinYoongi
Go to solution Solved by arjemma,

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The region is in the zone where eruptive events cause protons to be accelerated and proton levels rise. Also electron levels are rising on EPAM indicating the eruptive event. If EPAM low level protons also rise there is a CME on the way. We’ll have to wait a bit more for LASCO imagery to be complete for better analysis. 

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Haaaaa, another Friday getting off of work. It is certainly STEREO A directed, so it's comin' for us.

....

We'll get a better impact this time, but the question now is how close to the main bulk of the CME are we.

.....

I'll have a preliminary arrival time at STEREO A of 2023/02/26 19:00Z +-6 hours at roughly 46.5 hours travel time. L1 should be a few hours earlier, but all eyes on SOHO now to compare.

Edited by Jesterface23
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1 hour ago, Jesterface23 said:

2 new frames, but the northwest side of the CME is almost out of SOHO's C3 imagery already. I'm sitting at around 35-45 hours of travel time to L1, not my preliminary forecast yet. Certainly G3 potential at this point in time.

G3 would be amazing! Are you sure it’s partial halo and has an Earth-directed component?

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Just now, Sam Warfel said:

G3 would be amazing! Are you sure it’s partial halo and has an Earth-directed component?

Yeah. This time there is a slightly bigger CH in center disk, but more of the shock is getting by it in C3 imagery than the X2.2 flare CME.

I believe STEREO A is missing the bulk, but L1 may be right on the edge.

I'll go with a preliminary arrival time of 2023/02/26 12:00Z  with a chance of error -4/+6 hours. Roughly a 39:30 travel time. If timing is close, the only reason I'm not going with G4 potential is it that the CME isn't aimed further towards us.

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Hope Jesterface23 you are right and you can make better forecasts than the other forecasters on
the website with the dozens of game casino advertisements...

But its' always a thing with hope, you know, you can hope one time, two times, hundred times - but
maybe it needs thousand times before your hope gets fulfilled - in other words we maybe need
thousand CMEs around the sun before we get a very direct hit and I guess that we have already felt
a few hundred behind us last two years with no hit.

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9 hours ago, Jesterface23 said:

Yeah. This time there is a slightly bigger CH in center disk, but more of the shock is getting by it in C3 imagery than the X2.2 flare CME.

I believe STEREO A is missing the bulk, but L1 may be right on the edge.

I'll go with a preliminary arrival time of 2023/02/26 12:00Z  with a chance of error -4/+6 hours. Roughly a 39:30 travel time. If timing is close, the only reason I'm not going with G4 potential is it that the CME isn't aimed further towards us.

The news article from SWL suggests G1 or maybe G2, the full halo part of the CME is pretty slow/faint. If it was symmetrical I’d definitely say G3, but sadly it seems like we are missing the bulk of it 

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3 hours ago, Sam Warfel said:

The news article from SWL suggests G1 or maybe G2, the full halo part of the CME is pretty slow/faint. If it was symmetrical I’d definitely say G3, but sadly it seems like we are missing the bulk of it 

What did noaa say? 

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3 hours ago, Sam Warfel said:

The news article from SWL suggests G1 or maybe G2, the full halo part of the CME is pretty slow/faint. If it was symmetrical I’d definitely say G3, but sadly it seems like we are missing the bulk of it 

SWL is going with a later arrival time, so G2 being possible would be reasonable.

We may end up getting an impact between the bulk of the CME and a glancing blow, that's how close to the edge we may be. SA will get a glancing blow.

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1 minute ago, mozy said:

Yes, looks decent aswell.

Deja Vu indeed!

1 minute ago, Solarflaretracker200 said:

Nice flare going on, right now. Kinda a steep incline 

That’s caused by the filament eruption we’re talking about above. A slow-peaking flare that just reached R2!

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9 minutes ago, mozy said:

We're literally having a repeat of the last filament eruption, this filament doesn't seem as dense.

Looks a bit more westward, correct me if im wrong ?

Also how do you determine density in imagery available rn? I never paid much attention to that

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