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NOAA issues G2 geomagnetic storm watch for October 9

NOAA's Space Weather Prediction Center has issued a G2 (Moderate) geomagnetic storm watch for October 9 following a coronal mass ejection from active sunspot region AR4549.

||6 min read

BOULDER, Colo. Stargazers and aurora chasers across northern latitudes are preparing for a potential skywatching treat this week.

NOAA's Space Weather Prediction Center (SWPC) has officially issued a G2 (Moderate) Geomagnetic Storm Watch for Friday, October 9, 2026. The forecast comes following a long-duration solar eruption that launched a direct Coronal Mass Ejection (CME) toward Earth.

If the incoming plasma cloud impacts Earth's magnetosphere with favorable magnetic alignment, vibrant displays of the aurora borealis (northern lights) could descend into lower latitudes across more than 20 northern U.S. states.

The Origin: Sunspot Region AR4549 Erupts

The space weather event traces back to active sunspot region AR4549.

The rapidly growing magnetic cluster unleashed a long-duration M1.4-class solar flare. The flare was accompanied by a full-halo coronal mass ejection, a billion-ton cloud of magnetized solar plasma blasted directly along the Sun-Earth line.

Solar Storm Propagation Parameters
├── Eruption Source: Sunspot Active Region AR4549
├── Primary Solar Event: Long-duration M1.4 Solar Flare
├── Plasma Vector: Full-Halo Coronal Mass Ejection (Earth-Directed)
└── Estimated Transit Speed: ~500 to 600 kilometers per second

Using 3D solar wind propagation models (WSA-ENLIL), SWPC forecasters determined that the leading edge of the CME will make initial contact with Earth's protective magnetic envelope during the early morning hours of October 9.

                       CME Earth Impact Timeline
   [Sunspot AR4549 Eruption (M1.4 Flare)]
                      |
                      v
   [Full-Halo CME Discharged Into Deep Space]
                      |
                      v
   [~48-Hour Interplanetary Transit Window]
                      |
                      v
   [Impact Earth's Magnetosphere: Oct. 8 (Late Night) - Oct. 9 (Early Morning)]
                      |
                      v
   [Geomagnetic Disturbance Phase (G1 to G2 / Kp 5 to 6 Peak)]

Aurora Viewing Footprint and Impact Risk

A G2-class geomagnetic storm corresponds to a planetary Kp index of 5 to 6. Under these conditions, the auroral oval expands significantly southward from its typical Arctic boundaries.

Expected Geographic Aurora Visibility (Clear Dark Skies)
├── Primary Tier: Alaska, Northern Canada, Scandinavia, Iceland
├── High-Probability U.S. States: Washington, Idaho, Montana, North Dakota, Minnesota, Wisconsin
└── Secondary "Horizon View" States: South Dakota, Iowa, Michigan, New York, Maine, Vermont

Ideal viewing conditions will be aided by a favorable lunar phase. With a nearly new Moon providing dark night skies in rural areas, observers equipped with cameras or modern smartphone dark-mode settings stand a high chance of capturing the auroral glow.

NOAA Space Weather Scale Breakdown
├── G1 (Minor): Weak grid fluctuations; auroras visible in high latitudes (Canada/Alaska)
├── G2 (Moderate): Voltage alarms in high-latitude grids; auroras push into Northern US (Kp 6)
└── G3 (Strong) to G5 (Extreme): Widespread grid disruptions; auroras push down to Mid-Atlantic/Sunbelt

In terms of infrastructure impact, a G2 storm poses minimal danger to the general public. High-latitude power systems may experience minor voltage fluctuations, and satellite operators may log slight atmospheric drag increases. High-frequency (HF) radio communications near polar routes may also experience temporary fading. For a deeper look at how extreme space weather threatens electrical infrastructure, see our analysis of where a massive solar storm could take down the US power grid.

What Watchers Should Expect

SWPC forecasters emphasize that the precise strength of the storm depends heavily on the orientation of the CME's internal magnetic field (Bz) upon impact.

If the magnetic field points strongly southward, it will cancel out Earth's northward-pointing field lines, allowing solar energy to enter the upper atmosphere and supercharge the auroral display. Space weather agencies will continue monitoring real-time telemetry from L1 solar wind satellites (such as SOLAR-1) as the CME approaches.

Metric / ParameterEvent Operational Baseline
Monitoring AgencyNOAA Space Weather Prediction Center (SWPC)
Alert LevelG2 (Moderate) Geomagnetic Storm Watch
Peak Kp ForecastKp 5 (G1) to Kp 6 (G2)
Primary Viewing WindowLate night Thursday, Oct. 8 through pre-dawn Friday, Oct. 9

Aurora activity of this kind is a direct product of the solar cycle's active phase. For context on how solar maximum is shaping skywatching this year, see our guide to Spain's three solar eclipses this summer, and for the physics of auroral emission beyond Earth, read how astronomers captured auroral radio bursts from exoplanet Beta Pictoris b.

Frequently Asked Questions

As SWPC forecasters noted in the watch bulletin: "The precise timing and intensity of the storm will depend on the CME's magnetic field orientation upon arrival." For skywatchers across the northern United States, the late night of October 8 through pre-dawn October 9 shapes up as the prime window to look up, with a nearly new Moon and a G2-class solar storm potentially painting the sky green and violet.

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