Latest Helios Report

  • Solar Watch — April 24, 2026 | 18:00 UTC

    Solar Flare Activity — Last 12 Hours
    Peak: M-class @ 18:15 UTC (2h 14min ago)
      M @ 08:30 UTC  ·  M @ 09:04 UTC  ·  M @ 12:52 UTC  ·  M @ 18:03 UTC  ·  M @ 18:34 UTC

    ☀ HELIOS SOLAR WATCH · 2026-04-24 20:29 UTC
    Active solar regions producing frequent M-class flares; geomagnetic field quiet
    SOLAR: ACTIVE
    GEO: QUIET

    Active Regions
    7
    X-Ray
    A/B (quiet)

    Solar activity is currently characterized by significant flaring from AR4419 and AR4423, despite a quiet geomagnetic environment. While Earth’s magnetic field remains undisturbed, the high frequency of solar flares necessitates vigilance for potential impulsive radio disruptions.

    HMI Continuum Intensity

    HMI Continuum · Visible Light

    SUVI 304 — Extreme UV

    SUVI 304Å · Extreme Ultraviolet

    R0
    Radio Blackouts
    24h max: R0

    S0
    Solar Radiation
    24h max: S0

    G0
    Geomagnetic Storm
    24h max: G0

    Planetary Kp-Index
    1.3
    0–9 scale · ≥5 = geomagnetic storm

    F10.7 Solar Flux
    113.0
    sfu · >150 = high activity

    The sun is currently hosting seven active regions, with AR4419 exhibiting complex magnetic structures capable of X-class events. The F10.7 index is at 113.0 sfu, indicating moderate solar activity. Geomagnetic conditions are stable with a Kp-index of 1.3, showing no current influence from the recent flare activity.

    Key Metric

    The M-class flare frequency is the most critical metric, as it suggests underlying magnetic instability in active regions that could impact shortwave radio propagation.

    Geomagnetic activity is expected to remain quiet to unsettled, reaching a Kp of 3.0 by early April 25. Flare potential remains elevated, with a 30% probability of further M-class events as the active regions continue to evolve.

    🌌 Aurora Outlook

    Aurora visibility is not expected at mid-latitudes over the next 24 hours. Observations should be confined to high-latitude regions, where only minor, isolated auroral displays are possible.

    Region Location Class Flares C/M/X
    AR4419 N15W79 Eso/BGD 1/1/2
    AR4420 N17E10 Eki/BGD 0/0/0
    AR4421 S11E24 Hsx/A 1/0/0
    AR4422 N08W73 Hrx/A 0/0/0
    AR4423 S05E30 Dai/BD 5/1/0
    AR4425 N06E76 Dso/B 0/0/0
    AR4424 N17E45 Cro/B 0/0/0
    2026-04-24 18:35:25.930Space Weather Message Code: SUMXM5
    2026-04-24 18:12:55.427Space Weather Message Code: ALTXMF
    2026-04-24 10:42:00.107Space Weather Message Code: ALTTP4
    2026-04-24 09:28:15.750Space Weather Message Code: ALTTP2
    2026-04-24 09:27:04.090Space Weather Message Code: ALTTP2

    Monitor the magnetic complexity of AR4419 as it rotates toward the solar limb, as it remains the primary candidate for further impulsive X-ray events.