Sun news: Stunning far-side eruption steals the show

Sun news November 26: Stunning far-side eruption steals the show

Today’s top story: A towering, gorgeous prominence on the northeast solar horizon shows that activity on the far side of our sun remains high. This dramatic eruption began around 19:44 UTC on November 25. Although we do not yet know which active region produced it, we know the resulting blob of solar plasma—a coronal mass ejection (CME)—is not headed toward Earth, since the event occurred on the far side of the sun. Meanwhile, the Earth-facing side remains in a lull, producing only faint, small C- and B-class flares. Stay tuned for updates.

Past 24 hours: The details

(11 UTC November 25 – 11 UTC November 26)

• Flare activity: The number of flares increased compared to yesterday. The sun produced 13 flares during this period—up from nine the previous day—but activity remained at low levels, with only faint C- and B-class flares. We observed eight C-class (common) and five B-class (weak) flares.
  • Strongest flare: A faint C2.2 flare from AR4290 at 3 UTC on November 25. These low-level flares do not cause radio blackouts.
  • Other notable flares: C2.1 from AR4292 at 15:56 UTC; C1.9 from AR4291 at 14:35 UTC; C1.6 from AR4288 at 16:28 UTC; and a C1.1 from AR4292 at 21:12 UTC— all on November 24. On November 25, AR4291 produced a C1.0 at 5:22 UTC, and AR4292 produced a C1.1 at 5:56 UTC and a C1.2 at 6:12 UTC.
• Sunspot regions: The Earth-facing solar disk shows six numbered active regions today.
  • AR4291 (beta-gamma) remains the largest and most complex region on the disk. It produced two C-class flares and still holds the potential for larger events.
  • AR4292 (beta-gamma) showed growth and gained a gamma component. Its flare production increased, and it now has similar potential for stronger flares.
  • AR4290 (alpha) and AR4288 (beta) each produced one faint C-class flare and otherwise remained simple and stable.
  • The remaining regions stayed mostly stable or in gradual decay, producing no significant flares.
• Blasts from the sun? The CME linked to the prominence eruption near 19:44 UTC on November 25 was launched from the far side of the sun, so none of the plasma is headed toward Earth. Aside from this far-side activity, no Earth-directed CMEs appeared in available satellite imagery.
• Solar wind: Solar wind speeds fluctuated dramatically. Winds hovered near 800 km/s for much of November 25, peaking around 820 km/s. By 10 UTC on November 26, speeds measured 755 km/s. The interplanetary magnetic field (IMF) averaged around 6 nT. The Bz component repeatedly switched between northward and southward, with the strongest southward dips reaching -10 nT. At 10 UTC, Bz was northward— a configuration that limits auroral activity.
• Earth’s magnetic field: Earth’s magnetic field remained disturbed, ranging from unsettled to active levels. No G1 (minor) geomagnetic storm occurred, but the Kp index stayed near 4 for much of the period — just one step below storm level (Kp 5). At the time of writing, Kp remains at 4.

What’s ahead? Sun–Earth forecast

• Flare activity forecast: Low activity is expected today. Chances for moderate M-class flares remain near 15%, while the chance for X-class events stays low (1%). Two regions—AR4291 and AR4292—now show beta-gamma configurations, so the potential for larger flares may increase in the days ahead.
• Geomagnetic activity forecast:
  • November 26: High-speed solar wind from a coronal hole high-speed stream (CH HSS) will keep Earth’s geomagnetic field at unsettled to active levels. Isolated G1 (minor) storming remains possible as this coronal hole stays in a geoeffective position, especially with added influence from a co-rotating interaction region (CIR).
  • November 27: Active conditions (Kp 4–5) and G1 storm levels are likely as the coronal hole continues to affect Earth. These conditions are expected to begin decreasing on November 28.

Sun news November 25: Solar coronal holes spark geomagnetic storms!

Today’s top story: Surprise! We got a G1 (minor) geomagnetic storm last night, with auroras at high latitudes, beginning around 0 UTC on November 25. The stormy conditions stemmed from an early-arriving co-rotating interaction region (CIR), which is fast solar wind streams interacting with slower solar wind ahead of it. Long story short … the solar wind disturbed Earth’s magnetic field and pushed the Kp index (a measure of the disturbance) to level 5 during two three-hour synoptic periods. As of this writing, Kp = 5 remains ongoing. And here’s more exciting news! The coronal holes are still in a geoeffective position, where they are capable of affecting Earth. So active conditions with isolated G1 geomagnetic storming might continue through November 27. Did you see the auroras last night? Took photos? Share them with our community!

Past 24 hours: The details

(11 UTC November 24 – 11 UTC November 25)

• Flare activity: Sun activity remained at a very low level, with mostly B-class (weak) flares during the 24-hour period. A total of nine flares were observed: two C-class (common) and seven B-class flares.
  • Strongest flare: A faint C1.6 flare from AR4291 at 22:03 UTC on November 24. These common, low-level eruptions do not produce radio blackouts.
  • Other notable flares: A C1.3 from AR4291 at 22:20 UTC on November 24. All remaining flares were B-class.
• Sunspot regions: Six numbered active regions appeared on the Earth-facing side of the sun.
  • AR4291 (beta-gamma) remained the most complex region on the disk, producing both C- and B-class flares. It retains the potential for larger flares.
  • AR4290 (beta) showed decay and produced no flares.
  • AR4289 (alpha) produced one faint B-class flare and otherwise remained simple and stable.
  • AR4293, a newcomer in the northeast quadrant, remained quiet.
  • The remaining numbered regions stayed mostly stable or in gradual decay, contributing minimal flare activity.
• Blasts from the sun? No Earth-directed coronal mass ejections (CMEs) appeared in available satellite imagery during the period. Coronagraph data from SOHO and other spacecraft showed no significant eruptions heading toward Earth.
• Solar wind: Solar wind speeds fluctuated dramatically. Speeds hovered near 700 km/s during the first half of the period (on November 24), dropped to 260 km/s by 5 UTC today, then surged to 765 km/s by 10 UTC on November 25. The interplanetary magnetic field (IMF) remained moderate, averaging around 8 nT. The Bz component repeatedly switched from northward to southward, with the strongest southward peaks reaching -10 nT. Bz remained southward at 10 UTC on November 25, a configuration that favors auroral activity.
• Earth’s magnetic field: Earth’s magnetic field ranged from unsettled to active levels. G1 (minor) geomagnetic storm conditions occurred, with the Kp index reaching 5 from 0–3 UTC and again from 6–9 UTC on November 25. At the time of this writing, Kp remains at 5.

What’s ahead? Sun–Earth forecast

• Flare activity forecast: Low activity is expected through November 26. Chances for moderate M-class flares remain near 15%, driven mainly by AR4291. This region’s beta-gamma magnetic configuration gives it the potential to produce isolated M-class flares as it rotates further into a geoeffective position. The probability of stronger X-class flares remains low (1%) but cannot be fully ruled out.
• Geomagnetic activity forecast:
  • November 25: Earth’s geomagnetic field to continue enhanced to unsettled to active conditions with more isolated G1 (minor) geomagnetic storming as fast wind from a coronal hole high-speed stream (CH HSS) now at geoeffective position continues sending its fast solar wind to us combined with a co-rotating interaction region (CIR).
  • November 26: Active conditions (Kp 4–5) with G1 storm levels likely as the coronal hole continues to influence Earth. Solar wind speeds are expected to remain elevated at 600–700 km/s through the day. Auroras may be visible from Toronto, Chicago, Boston, northern England and Scotland. Enhanced conditions may persist through the end of the forecast period.

Sun news November 24: Solar activity breather continues

Our star appears to be taking a breather, firing only C (common) and B (weak) flares over the past day. The strongest of these was a C2.5 flare from sunspot region AR4290, which briefly lit up the solar disk. The most productive region, however, was AR4291 in the southeast, which shows promising complexity and continues to develop more sunspots. This region is the one to watch, especially as it starts to rotate into a more geoeffective position.

Past 24 hours: The details

(11 UTC November 23 – 11 UTC November 24)

• Flare activity: Solar activity remained at low levels, with 8 C-class flares and 3 B flares observed during the 24-hour period.
  • Strongest flare: C2.5 from AR4290 at 6:21 UTC on November 24. This common, low-level eruption produced no radio blackouts.
  • Other notable flares: C2.5 from AR4291 at 6:03 UTC on November 24; C1.6 from AR4290 at 20:10 UTC on November 23; C1.5 from AR4291 at 12:30 UTC on November 23; C1.3 from AR4290 at 2:32 UTC on November 24.
  • Sunspot regions: The Earth-facing solar disk currently displays 6 numbered active regions, with one newly formed region appearing over the past day.
    • AR4291 (beta-gamma) remained the most complex region on the disk, developing additional intermediate spots and maintaining its status as the lead flare producer. This southeast region is responsible for the majority of C-class activity and bears watching as it rotates into a more geoeffective position.
    • AR4292 (beta) was newly numbered during the period. This fresh region remained mostly inactive but adds to the overall sunspot count.
    • AR4290 produced multiple C-class flares including the period’s strongest C2.5 event. This region shows modest activity despite its simpler magnetic configuration.
    • AR4288 contributed a single C1.0 flare but otherwise remained relatively quiet.
    • The remaining numbered active regions were either mostly stable or in gradual decay, showing minimal flare production during the period.
  • Blasts from the sun? No Earth-directed coronal mass ejections (CMEs) were observed in available satellite imagery during the period. Coronagraph data from SOHO and other spacecraft showed no significant plasma eruptions heading toward Earth.
  • Solar wind: Solar wind speeds initially hovered near 350 km/s – typical background conditions – before rising to around 500 km/s at 16:44 UTC on November 23. The interplanetary magnetic field (IMF) remained moderate, with total field strength peaking at 13 nT at 18:33 UTC on November 23. The important north–south Bz component reached as far south as –8 nT at 11:57 UTC on November 23. A southward Bz favors aurora displays.
  • Earth’s magnetic field: Earth’s magnetic field ranged from quiet to unsettled levels, with Kp indices reaching 4 during an isolated active period from 15–18 UTC on November 23. Geomagnetic activity remained below storm levels throughout the period. The brief active interval corresponded with the moderately southward Bz orientation, which enhanced energy coupling between the solar wind and Earth’s magnetosphere. Conditions returned to quiet-to-unsettled levels following this period.

  

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  Bottom line: Sun news November 26, 2025: A towering far-side prominence lit up the northeast limb as Earth-facing activity stayed low with only faint C and B flares.

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