Earth Facing M-Class Solar Flare September 23rd 2025!

James Koppman, World News Report, today. Ladies and gentlemen, we've had the second M-class solar flare in over seven days. Only the second M-class solar flare in over seven days. This was basically Earth-directed. It came from a Beta Gamma Sunspot group. It's going to be 4217. AR-4217 AR4217. It was an M1.09, not a very powerful solar flare, peaking at around 1036 UTC time, which would be about 336 last night central time here in the U.S. Alright, and looking at some detailed information, it looks like it actually picked a 1034 instead of 1036. It did come from a Beta Gamma region, the only Beta Gamma region on our star. There's 11 total sunspot groups on the star currently, so we're seeing very little activity based on 11 sunspot groups Earth facing. We only had a 1% chance of having an X-Class Solar Flare today. That was probably only from 4217. We only had a 35% chance of seeing an M-Class Solar Flare. Luckily, that ship has sailed. And we have been maintaining a C-Class baseline for the last several months. Take a look at Gong Intensigram. We can see those 11 sunspot groups, spoke of 4217 right here, being the one that just produced the M1.09 solar flare, and the only semi-complex sunspot on the Earth-facing side of our sun. Again, that's going to be a beta-gamma sunspot group, while the others are simple sunspots in the three areas. Taking a look at Lasco C-3, we have a ton of time missing right when the explosion occurs. Two and a half hours right there. That would be just before, just as the explosion occurs. It looks like it did, in fact, send a coronal mass ejection south. Earth does look that way. You can see it spreading out there. So it looks like they killed Lasco. Right as this occurred, it looks like an awful large coronal mass ejection, but we saw the M1. We'll take a look at the back of the star, because this very well could be a backside eruption instead, and just coincidental. The timing is perfect. Finally, over to our D region absorption station center, and see that the M5 peaked about 1135, as we assumed it did. It's like we had X-ray coverage of a lot of Africa and some of the Atlantic Ocean. We did not see a lot of radio alternation. We'll check the backside real quick. With that said, there are some backside sunspots, so it's going to be hard to tell until they actually get with us. Whether that coronal mass ejection was lifted from that sunspot in .109 or these larger flares on the backside. So as you can see, we have 024 in this way, probably already named here, 025 in blue in this way, 026 up here, 028 here, I guess 027 is deteriorating, 028 down here, and then we have a new one. You kind of get a good idea of how potent they are down here, like 025 is really potent. And the two sunspots trailing it, 029 and 028 in orange and red, also look fairly potent down here. With that said, again, very hard to tell if the coronal mass ejection was headed this way, although the timing was perfect. But if so, it was a fairly large coronal mass ejection for such a small solar flare. We had an M1. 0.09 at 10.36, 3.36 central here in the U.S. That's the only activity we've seen all day long. Only the second M flare in 10 days. And again, that came from AR-4217, a beta gamma sunspot group. God bless. Share, subscribe, and always remember, anything's possible, bizarro world.