Space Weather by SolarHam


Space Weather for June 11, 2026 UTC Time
Indices:
(6/10 @ 21:05 UTC)
SFI
124
6
SSN
114
6

HMI Intensity
 Latest | Movie | HARP

HMI Magnetogram
Latest | Movie

Coronal Holes
Analysis | Movie

AIA 131 (Latest)
Movie

SUVI 304 (Latest)
Movies
Imagery: SDO | AIA | GOES | GONG | STEREO | CORONAGRAPH
Video: SDO | GSFC | SUVI | SOHO | STEREO | Helioviewer | YouTube

3 Day Geomagnetic Forecast
June 11
June 12
June 13
3 (G0)
4 (G0)
5 (G1)
Max Kp
M-Lat 05%
H-Lat 35%
M-Lat 10%
H-Lat 45%
M-Lat 05%
H-Lat 35%
Probabilities
Latest SWPC Forecast (@ 00:30 + 12:30 UTC)

Current Moon Phase:
23% Illumination
Waning Crescent

Noteworthy Flare Events (Past 72h)

Visible Sunspot Regions


AR 4466
B
N06W31
Declining
AR 4465
BG
N09E40
Stable
AR 4464
B
S12W03
Stable
AR 4463
A
N16W04
Stable
AR 4462
B
N16W35
Declining

Updated @ 11:35 UTC (June 11)

CME Tracking

1 Event(s) Logged

Cactus | SEEDS (GMU)
CCOR-1 Realtime RD

Farside Watch

Updated @ 13:20 UTC (June 10)
Latest Image | JSOC | STEREO

AIA Composite

Filaments + Coronal Holes

Latest AIA Composite

Solar Oribiter PHI Continuum (ESA)

Latest Available

STIX Light Curves | More Imagery

Real Time Solar Wind (BETA) | Expand Data
[フレーム]
Updated every minute.


X-Rays

Current

Global D-LAYER Absorption
Current Solar Flare Threat
C-Flare: 95%
M-Flare: 40%
X-Flare: 10%
Proton: 05%

Geomagnetic Field and Aurora
Past 24 Hours
Unsettled

Auroral Oval Forecast | South Pole
Kp-Index | A-Indices | Magnetometers

Latest Space Weather News
Long Duration C-Flare + CME
June 11, 2026 @ 01:45 UTC (UPDATED)
This long duration mid level C-Flare was observed around AR 4465 in the northeast quadrant peaking at 00:02 UTC (June 11). While this may not seem like much, coronal dimming is evident and a coronal mass ejection (CME) with a possible Earth directed component is associated. More to follow once a tracking model is available.

UPDATE: A minor (G1) geomagnetic storm watch was added beginning June 13th. The CME associated with the duration C6 flare appears to be heading mostly to the east with a glancing blow possible late on Saturday (UTC). High latitude sky watchers should be alert this weekend should local light and weather conditions allow.

ALERT: Type II Radio Emission
Begin Time: 2026 Jun 11 0013 UTC
Estimate Velocity: 918 km/s

Storm Watch Cancelled For Now
June 8, 2026 @ 22:20 UTC (UPDATED)
According to an update by NOAA/SWPC, the strong (G3) storm watch for today and moderate (G2) storm watch for Tuesday has been cancelled. As of this update, there is still no sign of the anticipated CME passing Earth. If a late CME passage is detected, I will provide a further update. For now, geomagnetic activity is at quiet levels.

Earth Facing Eruption + CME
June 6, 2026 @ 14:40 UTC (UPDATED)
A wide area of coronal dimming is evident this morning following an apparent eruption in the vicinity of AR 4461 located in the southeast quadrant. GOES solar X-Rays reached a peak of M1.8 at 14:00 UTC (June 6). The event is associated with a type II radio emission with an estimated velocity of 838 km/s. More to follow regarding a likely CME and if it is Earth directed. Image below by SDO/AIA.

UPDATE #2: A strong (G3) geomagnetic storm watch was issued beginning midday June 8th and into the 9th when the CME associated with this event is predicted to pass Earth.

CME Update:
An asymmetrical halo coronal mass ejection (CME) is leaving the Sun today following the eruption in the southeast quadrant. Although the mail bulk of plasma is heading southeast, there does appear to be an Earth directed component. An automated CME model by NASA is showing a passage past Earth by June 8th. Another round of geomagnetic storming may be possible. Stay tuned for more updates regarding this event.

Geomagnetic Storm Watch Continues
June 5, 2026 @ 12:50 UTC
Earth continues to pass through a multiple CME disturbance on Friday. After an initially weak impact very early this morning, solar wind data is looking a little more promising the past couple of hours. A secondary solar wind speed increase to around 650 km/s was observed, along with the Bz tipping south (-17 nT max). NOAA/SWPC are keeping a moderate (G2) to strong (G3) geomagnetic storm watch in place for the next 6 hours. Obviously not great timing for aurora sky watchers across Europe and North America.

Incoming CME Detected
June 5, 2026 @ 03:10 UTC (UPDATED)
Geomagnetic activity remains at quiet levels as an expected incoming CME is running late. The latest ACE EPAM data at 03:00 UTC (June 5) however is showing a sharp particle increase. This may be a sign that an interplanetary shockwave is approaching. I will continue to monitor the solar wind data and post any updates whenever necessary.

CME Detected: An incoming CME was detected at 04:31 UTC (June 5) by the ACE spacecraft and swept past Earth at 05:11 UTC. Initially the solar wind speed increased from 400 km/s to around 500-550 km/s with the Bz/IMF component pointing north. It is still early in the passage phase and fluctuations will be likely in the hours ahead. A geomagnetic storm watch remains in effect.

SUMMARY: Geomagnetic Sudden Impulse
Observed: 2026 Jun 05 0511 UTC
Deviation: 70 nT
Station: MEA


Site Information

SolarHam.com launched on March 15, 2006 with the purpose of providing real time Space Weather news and data from various sources, all in one location for easy navigation. The site was created and is still maintained solely by amateur (HAM) radio station Kevin VE3EN.

Data Sources

This website relays data and imagery from the following sources.

- NOAA Space Weather Prediction Center (SWPC)
- Solar Dynamics Observatory (SDO)
- Atmospheric Imaging Assembly (AIA)
- Solar Terrestrial Relations Observatory (STEREO)
- Deep Space Climate Observatory (DSCOVR)
- Large Angle and Spectrometric Coronagraph Experiment (LASCO)
- Solar and Heliospheric Observatory (SOHO)
- Lockheed Martin Solar & Astrophysics Laboratory (LMSAL)
- Global Oscillation Network Group (GONG)
- Space Weather Canada
- Australia Space Weather Services (SWS)

Contact Information

Any comments or questions regarding this website can be sent via E-Mail by clicking HERE .

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