Geomagnetic conditions are currently quiet, though the solar disk remains magnetically complex. Despite the calm Kp-index, the high probability of M-class flares necessitates continued monitoring for potential impulsive radio interference.
⚠ ALTPC0 · 4 more below
Geomagnetic stability is expected to persist through the next 24 hours with the Kp-index hovering between 1.0 and 2.0. The primary activity will remain confined to solar flare production rather than geomagnetic storming.
Aurora visibility is not expected at mid-latitudes over the next 24 hours.
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Observation should be limited to high-latitude polar regions where background auroral activity may be visible under clear, dark skies.
Monitor AR4498 and AR4499 for sudden magnetic evolution that could trigger impulsive X-ray emissions despite the lack of geomagnetic storming.
▸ Detailed readings
R0
(24 h max R0)
S1
(24 h max S0)
111.0
sfu
| Region | Location | Class | Flares C/M/X |
|---|---|---|---|
| AR4495 | S03W69 | Axx/A | 0/0/0 |
| AR4499 | N04E05 | Dao/BGD | 0/0/0 |
| AR4500 | N18E44 | Cao/B | 0/0/0 |
| AR4498 | N14E37 | Cai/BG | 1/0/0 |
| AR4492 | N16W74 | Hsx/A | 0/1/0 |
| AR4494 | S04W55 | Hsx/A | 0/0/0 |
| AR4496 | N05W23 | Hsx/A | 0/0/0 |
| AR4501 | S08E03 | Dso/B | 0/0/0 |
Helios Observer · Data: NOAA SWPC · updated every 12 h