04/06/2026
STRONG GEOMAGNETIC STORMING AND AURORA POSSIBLE ————————————————————————
Strong Geomagnetic Storming (G3) has been forecast by NOAA SWPC as a result of multiple fast-moving, Halo Coronal Mass Ejections (CME) associated with eruptive M9.3, M7. and X1.0 Flares
GOES-19 and LASCO C2/C3 coronagraph imagery indicate an asymmetrical CME Halo associated with this event biased toward the north and west with partial earth directed components.
Current WSA–ENLIL modelling places solar wind speed estimates at around 800-1000km/s due to a double impact.
As a result, NOAA SWPC and UKMO have issued G3 Geomagnetic Storm Watches respectively, with combined effects from multiple CME's possible.
Current averaged estimated arrival times: 4/6/2026 18:00 UTC ± (7 to 12 hrs). CME impact probabilities range from 60-90% due to the complex nature of multiple CME influences ————————————————————————
At least three Coronal Mass Ejections were noted in the observed imagery, most notable however is the modelled scenario where the initial CME associated with the M9.3, is followed by the X1.0 associated flare with the former eventually catching up.
This may result in a combination or cannibalistic effect.
HUXt Ensemble modelling also indicates similar impact probabilities and uncertainties; however, it differs slightly from other model runs, suggesting a later impact arrival time and solar wind speed estimates of 650 to 800km/s.
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Confidence of Earth arrival is moderate, shrouded by difficulty in modelling these CMEs due to the complex nature of the event.
The general consensus among Major Space Weather forecasts suggests G3 (STRONG) conditions are possible.
The estimated radial velocity of the CMEs is around 1400 km/s.
If all factors align and modelling verifies, visible auroras could be possible over the next day or so in major cities including Hobart, Melbourne, Sydney, and Perth, as well as locations in between.
The CME’s estimated travel time is around 20 to 40 hours, though this is not guaranteed and could vary.
Upon the CME’s physical arrival, periods of geomagnetic activity may increase and decrease over the course of a day or so as the CME structure begins impacting Earth. (Conditional to Impact) This occurs in stages: the shock front/sheath followed by the main body/core.
The configuration of the flux rope determines how well its magnetic alignment couples with the magnetosphere. If the flux rope configuration is poor and contains mostly +Bz, aurora potential will be inhibited.
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IMPORTANT:
While the physical setup looks interesting, sustained southward magnetic field alignment (−Bz) upon arrival is essential for strong geomagnetic storming.
Sustained northward alignment (+Bz) can significantly inhibit or even prevent auroral activity. Think of this as how magnets behave: opposites attract (allowing charge flow), while like poles repel. For success, the Bz field component must trend negative (∂Bz/∂t < 0). ————————————————————————
The overall setup offers potential for aurora chasers, and could produce good displays if magnetic connection occurs in a favourable southward alignment for extended periods.
However, as previously mentioned, nothing is guaranteed.
If the CME is a MISS, unfavourable magnetic alignment occurs or the CME is delayed, aurora potential can be significantly diminished. Keep hope high, but expectations realistic.
Updates will follow once data is received at the L1 (Lagrange Point 1) ACE/DSCOVR satellites, clarifying exactly what this event may bring for us here on Earth.
Stay tuned, and feel free to ask any questions!
More updates will follow as data becomes available. Useful info in the comments ⬇️ ————————————————————————
NOAA Estimated Impact Times (Local)
AEST: 0400
ACST: 0330
AWST: 0200
(June 5th, 2026)
*SUBJECT TO CHANGE*
Australian-based weather conditions are listed below in the comments, including cloud coverage percentages (ACCESS-G, ECMWF & GFS).
The included map is based on past captures and comparative data from similar geomagnetic storming conditions and their potential extent.
It should be used as a guide only, as conditions can vary greatly depending on numerous factors.
Additionally, Earth weather effects are not considered by the map. ————————————————————————